Seattle Snowmass Summer Meeting 2022
News:
- The POSTER abstract submission has closed.
- The student support application is HERE! Students with active contributions (including poster presentations) will be prioritized to be considered for sponsorship.
Introduction:
The Particle Physics Community Planning Exercise (a.k.a. “Snowmass”) is organized by the Division of Particles and Fields of the American Physical Society. Snowmass is a scientific study. It provides an opportunity for the entire particle physics community to come together to identify and document a scientific vision for the future of particle physics in the U.S. Snowmass will define the most important questions for the field of particle physics and identify promising opportunities to address them.
The Snowmass Community Study has 10 frontiers addressing different aspects of the field. They are:
- Energy Frontier,
- Neutrino Physics Frontier,
- Rare Processes and Precision Measurements Frontier,
- Cosmic Frontier,
- Theory Frontier,
- Accelerator Frontier,
- Instrumentation Frontier,
- Computational Frontier,
- Underground Facilities,
- Community Engagement.
In addition, there are Snowmass Early Career Scientists forum. At the summer study the frontiers will agree on their final, individual, reports. The frontier conveners, along with the US High Energy Physics community, will draft a final summary document that presents the big questions facing the field and science of particle physics along with research paths forward. The Snowmass Report will provide input to the High Energy Physics Advisory Panel. The Particle Physics Project Prioritization Panel (P5), a sub-panel of HEPAP, will produce a strategic report for the field later in 2022.
Summer meeting page: http://seattlesnowmass2021.net/
Supporters
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Conference Logistics: Pre-Registration Lobby (Kane Hall)
Lobby
Kane Hall
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Conference Logistics: Pre-Registration Denny Room (Oak Hall)
Denny Room
Oak Hall
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Conference Logistics: Registration Lobby (Kane Hall)
Lobby
Kane Hall
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Physics Highlights from the Frontiers: Snowmass Workshop Charge - I 130 (Kane Hall)
130
Kane Hall
17Bdescription here
Conveners: R. Sekhar Chivukula (UC San Diego), Tao Han (University of Pittsburgh)-
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CSS Welcome and Meeting LogisticsSpeaker: Gordon Watts (University of Washington)
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Welcome from the University of WashingtonSpeakers: Prof. Dianne Harris (University of Washington - Dean of Arts and Sciences), Prof. Laurence Yaffe (University of Washington - Chair of the Department of Physics), Dr Mari Ostendorf (University of Washington - Vice Provost Of Research)
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DPF Greeting and Snowmass Organization OverviewSpeaker: Joel Butler (Fermilab)
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Accelerator Frontier WorkplanSpeaker: Steve Gourlay (LBNL)
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Community Engagement Frontier WorkplanSpeaker: Ketevi Adikle Assamagan (Brookhaven National Laboratory)
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Coffee Break
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Energy Frontier WorkplanSpeaker: Alessandro Tricoli (BNL)
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Theory vision: the questions before us (Working title, may change)Speaker: Hitoshi Murayama (University of California, Berkeley & IPMU, University of Tokyo)
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Physics Highlights from the Frontiers: Snowmass Workshop Charge II 130 (Kane Hall)
130
Kane Hall
17Ddescription here
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Instrumentation Frontier WorkplanSpeakers: Jinlong Zhang (ANL), Jinlong Zhang (ANL)
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Experimental Landscape (Working title, may change)Speaker: Andrew Lankford (UC Irvine)
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Rare Processes and Precision Measurements Frontier WorkplanSpeaker: Robert Bernstein (Fermilab)
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Underground Facilities Frontier (UF) WorkplanSpeaker: John Orrell (Pacific Northwest National Laboratory)
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16:00
Coffee 225 and Lobby (Kane Hall)
225 and Lobby
Kane Hall
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Afternoon Plenary: Planning US HEP - past present future 130 (Kane Hall)
130
Kane Hall
17EConveners: Joel Butler (Fermilab), R. Sekhar Chivukula (UC San Diego)-
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Perspectives from Snowmass to P5 in 2013/2014Speaker: Steve Ritz (UCSC and SCIPP)
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Perspectives from NSFSpeaker: James Shank (NSF)
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Perspectives from FermilabSpeaker: Lia Merminga (FNAL)
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Questions/Comments
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Accelerator Frontier: (auxillary-reserved room - AF3 continue) 248 (MGH)
248
MGH
37AConveners: Frank Zimmermann (CERN), Georg Hoffstaetter (Cornell University) -
Accelerator Frontier: AF3 Report (2 hrs) and AF4 Report (2 hrs) 220 (Kane Hall)
220
Kane Hall
19GConveners: Alexander Valishev (Fermilab), Frank Zimmermann (CERN), Georg Hoffstaetter (Cornell University), Mark Palmer (Brookhaven National Laboratory), Nadia Pastrone (INFN-Torino)- 24
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Cool Copper ColliderSpeaker: Emilio Nanni (SLAC National Accelerator Laboratory)
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ILCSpeaker: Angeles Faus-Golfe
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Lepton Colliders with Higher Gradient at Lower Capital and Operational CostsSpeaker: Emanuela Barzi (Fermilab)
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Accelerator Frontier: AFx Internal (TBD) 242 (MGH)
242
MGH
19H -
Computational Frontier: CompF5 End User Analysis 254 (MGH)
254
MGH
20GConveners: Amy Roberts (CU Denver), Gavin Davies (University of Mississippi), Peter Onyisi (University of Texas at Austin)-
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CompF5 introductionSpeakers: Amy Roberts (CU Denver), Gavin Davies (University of Mississippi), Peter Onyisi (University of Texas at Austin)
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Summary of ContributionsSpeakers: Amy Roberts (CU Denver), Gavin Davies (University of Mississippi), Peter Onyisi (University of Texas at Austin)
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Recommendations & Highlights of ReportSpeakers: Amy Roberts (CU Denver), Gavin Davies (University of Mississippi), Peter Onyisi (University of Texas at Austin)
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Cosmic Frontier: CF1 Discussion 340 (HUB)
340
HUB
18IConveners: Hugh Lippincott (UCSB), Jodi Cooley (SMU), Tien-Tien Yu (University of Oregon), Tracy Slatyer (MIT) -
Cross frontier sessions: XF CEF-EF-NF-RF-CF-TF-AF-IF-CompF-UF CEF Feedback 334 (HUB)
334
HUB
18AA panel during the 22j session discussing the intersections of the AF and EF frontiers
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To collect feedback from other frontiers on CEF reports
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Feedback on Applications and Industry
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Feedback on Career pipeline & development
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Feedback on Diversity, Equity & Inclusion
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Feedback on Physics Education
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Feedback on Public Educcation & Outreach
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Feedback on Government Enggaement & Public Policy
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Feedback on Environmental & Societal Impacts
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Energy Frontier: EF - Strong Interactions I 238 (MGH)
238
MGH
18LConveners: Huey-Wen Lin (MSU), Michael Begel (Brookhaven National Lab), Pavel Nadolsky (Southern Methodist University), Stefan Hoeche (Fermilab)-
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The strong coupling: State-of-the-art and the decade aheadSpeaker: David d'Enterria (CERN)
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Discussions of Strong Coupling Constant for QCD Report
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Overview of the Proton Structure at the Precision FrontierSpeaker: Keping Xie (University of Pittsburgh)
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QCD at a Forward Physics Facility at the High-Luminosity LHCSpeaker: Mary Hall Reno (University of Iowa)
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Coffee Break
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Open Questions in Perturbative and Nonperturbative Diffractive QCDSpeaker: Mark Strikman (Penn State)
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QCD report discussion
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Energy Frontier: Higgs and BSM I 332 (HUB)
332
HUB
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CP violation at future colliders
10’ after the talk is reserved for Q&A
Speaker: Andrei Gritsan (Johns Hopkins University) -
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HL-LHC Results
10’ after the talk is reserved for Q&A
Speaker: Saptaparna Bhattacharya (Northwestern University) -
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Discussion of experimental portion of EF01/02 report
15’ after the talk is reserved for Q&A
Speaker: Isobel Ojalvo (Princeton University (US)) -
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Discussion of theory portion of EF01/02 report
15’ after the talk is reserved for Q&A
Speaker: Patrick Meade (Stony Brook University) -
10:30
Break
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EF08 Model Dependent Searches introduction
10’ after the talk is reserved for Q&A
Speaker: Elliot Lipeles (University of Pennsylvania) -
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Direct searches at hadron colliders
10’ after the talk is reserved for Q&A
Speaker: Sarah Eno (U. Maryland) -
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Direct searches at lepton colliders
10’ after the talk is reserved for Q&A
Speaker: Mikael Berggren (DESY)
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Instrumentation Frontier: IF1 288 (MGH)
288
MGH
23HConveners: Reina Maruyama (Yale University), Tom Cecil (Argonne)-
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Introduction
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Review of coordinated white papers
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Community White Paper Input
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Break
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Review of Topical Group Report
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Topical Group Report Hack session
The hack session has been canceled. Please send any comments on the topical group report to the conveners.
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Instrumentation Frontier: IF2 284 (MGH)
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MGH
23GConveners: Carlos Escobar (FERMILAB), Guillermo Fernandez Moroni, Juan Estrada Vigil (FNAL)- 63
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MKIDsSpeaker: Benjamin Mazin (UCSB)
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3D digital silicon photomultipliersSpeaker: Serge Charlebois (Université de Sherbrooke)
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09:40
Coffee break
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Quantum imaging applicationsSpeaker: Agustina Gabriela Magnoni
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Ge DetectorsSpeaker: Christopher Leitz (MIT Lincoln Laboratory)
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Multiplexing electronicsSpeaker: Gustavo Cancelo (fermilab)
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SNSPD cold readout: activities and plansSpeaker: Davide Braga
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Future photon-based neutrino detectorsSpeaker: Joshua Klein (University of Pennsylvania)
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Report Discussion
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Neutrino Physics Frontier: NF General Meeting 130 (Kane Hall)
130
Kane Hall
18NConveners: Elizabeth Worcester (BNL), Kate Scholberg (Duke University), Patrick Huber (Virginia Tech)-
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Frontier Business and LogisticsSpeakers: Elizabeth Worcester (BNL), Kate Scholberg (Duke University), Patrick Huber (Virginia Tech)
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Current Program: SBNSpeakers: Robert Wilson, Robert Wilson (Colorado State University)
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Current Program: Low Energy NeutrinosSpeakers: Bryce Littlejohn (Illinois Institute of Technology), Bryce Littlejohn, Bryce Littlejohn (IIT)
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09:45
Coffee Break
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DUNE: OverviewSpeaker: Chris Marshall (University of Rochester)
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Neutrino Town Hall
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Cosmic Frontier: CF2 Discussion 340 (HUB)
340
HUB
18PConveners: Gray Rybka (University of Washington), Joerg Jaeckel, Lindley Winslow (MIT) -
Computational Frontier: CompF2 Theoretical Calculations and Simulation 254 (MGH)
254
MGH
20VConveners: Kevin Pedro (Fermilab), Peter Boyle (Brookhaven National Laboratory), ji qiang (LBNL)- 81
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Accelerator SimulationSpeaker: Axel Huebl (Lawrence Berkeley National Laboratory, USA)
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Perturbative CalculationsSpeakers: Tobias Neumann, Tobias Neumann (BNL)
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Coffee break
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CompF2 Report RecommendationsSpeakers: Kevin Pedro (Fermilab), Peter Boyle (Brookhaven National Laboratory), ji qiang (LBNL)
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Discussion
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Cosmic Frontier: CF3 Discussion 340 (HUB)
340
HUB
18SConveners: Alex Drlica-Wagner (Fermilab), Chanda Prescod-Weinstein (University of New Hampshire), HAI-BO YU (UNIVERSITY OF CALIFORNIA, RIVERSIDE) -
Cosmic Frontier: CF4 Discussion 340 (HUB)
340
HUB
18TConveners: Anze Slosar (BNL), James Annis (Fermilab), Jeffrey Newman (University of Pittsburgh and PITT-PACC) -
Social: Remotely Green - Early Career Networking Virtual
Virtual
50Dhttps://washington.zoom.us/j/98883066364?pwd=UjVOajdLMFpMQWVibUtsR010T1AzUT09
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Remotely Green - Early Career Networking
One of recognized challenges with the virtual and/or hybrid meeting formats is that they offer limited opportunities for chance or planned encounters with other participants.
In partnership with Remotely Green we are running a couple of “virtual networking” events this week.
Each event lasts 45 minutes and allows you to meet and have around 7 rounds of 6 minute chats with up to 3 people in each round. Some icebreaker topics will be suggested based on some topic choices you will choose. See the short video at the bottom of the Remotely Green webpage for a better idea.
See the web page for more information: http://seattlesnowmass2021.net/green/
To connect to this event and get started (or read up on it) go to https://app.remotely.green/event/snowmass-2022-early-careers
Speaker: Peter Elmer (Princeton University)
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Afternoon Plenary: A Tour of Underground Facilities & Science: Today and Tomorrow 130 (Kane Hall)
130
Kane Hall
18UConvener: Jeter Hall (SNOLAB)-
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Introduction and overview of UFSpeaker: Jeter Hall (SNOLAB)
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International Underground LaboratoriesSpeaker: Clarence Virtue (Laurentian University)
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Outline of UF activities at SnowmassSpeaker: Jeter Hall (SNOLAB)
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Afternoon Plenary: AI/ML Modern Machine Learning for HEP 220 (Kane Hall)
220
Kane Hall
30AConveners: Benjamin Nachman (LBNL), Daniel Elvira (Fermilab), Steven Gottlieb (Indiana Univ.)-
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IntroductionSpeakers: Benjamin Nachman (LBNL), Daniel Elvira (Fermilab), Kazuhiro Terao (SLAC National Accelerator Laboratory), Steven Gottlieb (Indiana Univ.)
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How is modern ML different from what has been done in the past?Speaker: Daniel Whiteson (UC Irvine)
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Questions/Discussion
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How can ML go beyond traditional project / frontier boundaries?Speaker: Nhan Tran (FNAL)
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Questions/Discussion
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Places where ML could have a big impact, but where it has not been widely used traditionallySpeaker: David Shih (Rutgers University)
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Questions/Discussion
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Accelerator Frontier: Future Accelerators for HEP, Report of the Accelerator Frontier Implementation Task Force (IF) 130 (Kane Hall)
130
Kane Hall
30CConveners: Thomas Roser (BNL), Tor Raubenheimer (SLAC), Vladimir Shiltsev (FNAL)-
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ITF (Implementation Task Force) Report on Future Colliders - from Higgs Factories to Energy Frontier
talk by the ITF Chair T.Roser "ITF (Implementation Task Force) Report on Future Colliders - from Higgs Factories to Energy Frontier "
Speaker: Thomas Roser (BNL) -
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Panel Discussion
General Discussion after the ITF presentation
Speakers: Steve Gourlay (LBNL), Tor Raubenheimer (SLAC), Vladimir Shiltsev (FNAL)
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Afternoon Plenary: Lattice QCD 220 (Kane Hall)
220
Kane Hall
30BConveners: Aida El-Khadra (University of Illinois at Urbana-Champaign), Csaba Csaki (Cornell University), Nathaniel Craig (UC Santa Barbara)-
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Enabling precision quark- and lepton-flavor physics with lattice QCDSpeaker: Andreas Kronfeld (Fermilab)
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Uncovering new-physics signals in nucleons and nuclei with lattice QCD,Speaker: Zohreh Davoudi (University of Maryland)
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Questions and discussion
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103
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17:00
Coffee Lobbe & 225 (Kane Hall)
Lobbe & 225
Kane Hall
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Afternoon Plenary: In Search of Excellence and Equity in Physics 130 (Kane Hall)
130
Kane Hall
18ZConveners: Ketevi Adikle Assamagan (Brookhaven National Laboratory), Mu-Chun Chen (University of California, Irvine)-
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IntroductionSpeaker: Mu-Chun Chen (University of California, Irvine)
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Panel Discussion
Kevin Black, Sekhar Chivukula, Haiyan Gao (online), Jim Gates (online), Julie Renee Posselt (online)
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Q&A
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Poster Session 211 South Ballroom (HUB)
211 South Ballroom
HUB
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Distributed Coupling Linac for Efficient Acceleration of High Charge Electron Bunches
The Electron Ion Collider requires a pre-injector linac to accelerate large electron bunches from 4 MeV up to 400 MeV over 35 m[1]. Currently this linac is being designed with 3 m long traveling wave structures, which provide a gradient of 16 MV/m. We propose the use of a 1 m distributed coupling design as a potential alternative and future upgrade path to this design. Distributed coupling allows power to be fed into each cavity directly via a waveguide manifold, avoiding on-axis coupling[2]. A distributed coupling structure at S-band was designed to optimize for shunt impedance and large aperture size. This design provides greater efficiency, thereby lowering the number of klystrons required to power the full linac. In addition, particle tracking analysis shows that this linac maintains lower emittance as bunch charge increases to 14 nC and wakefields become more prevalent. We present the design of this distributed coupling structure, as well as progress on structure manufacturing and characterization.
[1] F. Willeke, "Electron ion collider conceptual design report 2021," tech. rep., United States, 2021.
[2] S. Tantawi et al., Phys. Rev. Accel. Beams, vol. 23, p. 092001, Sep 2020Speaker: Ankur Dhar (SLAC National Accelerator Lab) -
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Weighing the Axion with Muon Haloscopy
Axions in the local dark matter halo of the galaxy collide with virtual photons dressing the electromagnetic vertex of the muon. The collisions shift the muon magnetic moment in a way that scales with the volume of the muon beam and transforms like the axion under the charge conjugation, parity, and time-reversal symmetries of quantum electrodynamics. Analysis of measurements of the muon magnetic moment suggests that axions saturate the local halo density.
Speaker: Dr Noah Bray-Ali (Mt St Mary's University-Los Angeles) -
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The Axion Plasma Haloscope
We summarize the recent progress of the ALPHA Consortium, a new experimental collaboration to build a plasma haloscope to search for axions and dark photons. The plasma haloscope is a novel method for the detection of the resonant conversion of light dark matter to photons. Unlike traditional cavity haloscopes, which are generally limited in volume by the Compton wavelength of the axion, plasma haloscopes use a wire metamaterial to create a tuneable plasma frequency. This decouples the wavelength of light from the Compton wavelength and allows for much larger conversion volumes. We outline a baseline design for ALPHA and a potential experimental setup and show that it would lead to competitive sensitivity for well-motivated high mass axions.
Speaker: Marcel Demarteau (Oak Ridge National Laboratory) -
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GAMBIT (The Global and Modular BSM Inference Tool)
GAMBIT is a flexible and extensible open-source framework that can be used to undertake global fits of essentially any BSM theory to a wide range of relevant experimental data sets. The code currently has the ability to recast and combine results from collider searches for new physics, cosmological probes, neutrino experiments, astrophysical and terrestrial dark matter searches, and precision measurements. I will present the status of this project and some recent results obtained with it.
Speaker: Jonathan Cornell (Weber State University) -
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A Novel Dense Fiber Array for Astronomical Spectroscopy
With a Phase I Small Business Innovation Research (SBIR) grant from the National Science Foundation (NSF) we are building a high-density fiberscope. We propose a novel method for constructing a fiberscope for measuring the spectra of a large number of distant, celestial objects. Our design will provide a tenfold increase in the rate of red-shift measurements for cosmological surveys. We solder cylindrical, piezo-electric actuators to a rigid base, arranging them on a 5-mm grid. We glue a steel mast to each actuator. At the tip of each mast is an optical fiber. We bend each actuator by up to 6 mrad in two directions by applying ±250 V to its four electrodes. The tip of a 300-mm mast moves in a 3.8-mm square and locates the optical fiber with a precision of 10 µm rms. The positioner is mechanically simple but electrically complex. There are no moving parts other than the bending of the tube, but every tube requires its own amplifiers, converters, and control logic. Our miniaturized actuator electronics fit in the 5-mm square cross-section beneath each fiber. The positioner provides continuous adjustment of each fiber at a cost of only 10 mW per actuator. By making fibers available on a 5-mm pitch, our positioner makes it possible to place 50,000 fibers on a 1.3-m diameter focal plane, or 1,000 fibers in an 18-cm diameter. We are building a 16-fiber prototype now, and in the next two years we propose to build a 500-fiber fully-functional fiberscope for a collaborating telescope.
Speaker: Sayer Nathan (Open Source Instruments, Inc.) -
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A novel ML-based method of primary vertex reconstruction in high pile-up condition
The High-Luminosity LHC (HL-LHC) is expected to reach the peak instantaneous luminosity of $7.5×10^{34}\mathrm{cm}^{−2}\mathrm{s}^{−1}$ at a center-of-mass energy of $\sqrt{s}$= 14 TeV. This leads to an extremely high density environment with up to 200 interactions per proton-proton bunch crossing. Under these conditions event reconstruction represents a major challenge for experiments due to the high pileup vertices present.
To tackle the dense environment, we adapted a novel ML-based method named Sparse Point-Voxel Convolution Neural Network(SPVCNN), the current state-of-the-art techniques in computer vision, which leverages point-based method and space voxelization to categorize tracks into primary vertices.
In this poster, the performance of SPVCNN vertexing will be presented, as well as the comparison with the conventional Adaptive Multi-Vertex Finding(AMVF) algorithm.Speaker: Haoran Zhao (University of Washington) -
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A sample Algorithm Processing Unit implementation with the deployment of the deep neural network model for the Global Event Processor trigger subsystem for HL_LHC Upgrade at ATLAS
During the next update of the High-Luminosity Large Hadron Collider (HL-LHC) of ATLAS, a new global trigger subsystem will be installed into the L0 Trigger. New and improved hardware and algorithms will be deployed during the upgrade to increase the performance of the trigger system. The global trigger subsystem consists of various components, including the FPGA-based Global Event Processor (GEP), which processes the data through the trigger algorithm. Within the GEP, data will be pipelining through different Algorithm Processing Units (APU), which handle individual subtasks of the overall trigger. We present our work in creating an APU specification and sample APU as a guide to future APU developers. We also present a redesign of the APU interface to follow the AXI-stream protocol, which allows streaming computations that overlap operations at multiple pipeline levels, potentially improving overall throughput. Finally, we present our work deploying HLS4ML (high-level synthesis for machine learning) into the APU development. HLS4ML is a design tool for generating a deep neural network (DNN) algorithm model with ultra-low delays, and has been developed specifically to support the needs of high-energy physics experiments. Our goal is to demonstrate that the application of HLS4ML to APU development is practical, and we have already implemented a convolution neural network (CNN) model for the APU. The performance of the CNN APU is tested using a test vehicle and a sandbox provided by the ATLAS developers. The next step is developing another new algorithm using a deep neural network.
Speaker: Zhixing Jiang -
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A study of simulation tools and manufacturing methods for multi-functional carbon composite particle detector mechanics and support structures
Improvements in Detector mechanics need in-depth study of thermal and mechanical loading conditions to have more integrated design concepts that save on material budgets and optimize performance. Particle detectors at future colliders rely on ever more lightweight and radiation-hard charged particle tracking devices, which are supported by structures manufactured from composite materials. This article lays out engineering techniques able to solve challenges related to the design and manufacturing of future support structures. Novel manufacturing methods like Extrusion Deposition Additive Manufacturing (EDAM) along with associated simulation tools like Additive3D for prediction of part production and performance are highlighted with case studies from the High-Luminosity Phase Upgrade project for the CMS detector. Methodology for manufacturing of integrated support structures using simulation tools like COMPRO from Convergent Manufacturing Technologies is showcased for lightweight and highly thermally conductive support structures for future tracking detectors. Examples of current efforts at Purdue University related to the high-luminosity upgrade of the CMS detector are provided to demonstrate the prospects of suggested approaches for detectors at new colliders: a future circular collider or a muon collider. Specific geometric and design considerations for the proposed CMS Inner Tracker Rails are discussed to illustrate advantages and constraints for additively manufactured structures. The applicability, benefits, and uses of this technique to replace conventional tooling methodologies for composite layup part manufacturing are also highlighted.
Speaker: Sushrut Karmarkar (Purdue University) -
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ADMX Run 1c HiRes Analysis
The Axion Dark Matter eXperiment (ADMX) aims to detect axions from the
galactic halo. The experiment consists of a microwave cavity in a magnetic field.
When an axion passes through the cavity, it has a small probability to decay
into microwave photons. ADMX has two primary analysis channels, Medium
Resolution (MedRes) and High Resolution (HiRes), with frequency resolutions
of 200 Hz and 20 mHz, respectively. The HiRes channel is concerned with
detecting nonvirialized axions from flows with small velocity dispersions, whose
signals would have a width of approximately 100 mHz or less. The most recent
run, 1c, covered approximately 800 MHz to 1 GHz, corresponding to an axion
mass of 3.3-4.1 μeV. This poster will cover how this data was collected and
processed, the HiRes analysis procedure, and prelimenary results.*This work was supported by the U.S. Department of Energy through Grants
No DE-SC0009800, No. DE-SC0009723, No. DE-SC0010296, No. DE-SC0010280,
No. DE-SC0011665, No. DEFG02-97ER41029, No. DE-FG02-96ER40956, No.
DEAC52-07NA27344, No. DE-C03-76SF00098 and No. DE-SC0017987. Fer-
milab is a U.S. Department of Energy, Office of Science, HEP User Facility.
Fermilab is managed by Fermi Research Alliance, LLC (FRA), acting under
Contract No. DE-AC02-07CH11359. Additional support was provided by the
Heising-Simons Foundation and by the Lawrence Livermore National Labora-
tory and Pacific Northwest National Laboratory LDRD offices.Speaker: Alexander Hipp -
118
Advanced RF Structures for Wakefield Acceleration and High-Gradient Research
Structure wakefield acceleration (SWFA) is one of the most promising AAC schemes in several recent strategic reports, including DOE's 2016 AAC Roadmap, report on the Advanced and Novel Accelerators for High Energy Physics Roadmap (ANAR), and report on Accelerator and Beam Physics Research Goals and Opportunities. SWFA aims to raise the gradient beyond the limits of conventional radiofrequency (RF) accelerator technology, and thus the RF to beam energy efficiency, by reducing RF breakdowns from confining the microwave energy in a short (on the order of about 10 ns) and intense pulse excited by a drive beam. We envision that the following research topics, within the scope of AF7, are of great interest in the next decade: advanced wakefield structures, terahertz and sub-terahertz (THz) structures, and RF breakdown physics. Research on SWFA in the above directions would directly contribute to long-term large-scale applications, including AAC-based linear colliders and compact light sources. There is also potentially a strong synergy between SWFA and other AAC concepts, when structures are combined with plasmas into hybrid AAC schemes. Research on novel structures is at the core of advancing SWFA, and is critical to future AAC-based linear colliders; at the same, it has a strong synergy with other directions, such as cavity designs, high-power microwave systems and sources, and compact light sources.
Speaker: Xueying Lu (Northern Illinois Univ / Argonne National Laboratory) -
119
Anomalous quartic gauge couplings at a muon collider
Prospects for searches of anomalous quartic gauge couplings at a future high-energy muon collider using the production of WW boson pairs are reported. Muon-muon collision events are simulated at √s = 6 TeV corresponding to an integrated luminosity of 4 ab−1. The simulated events are used to study the WWνν and WWμμ final states with the W bosons decaying hadronically. The events are analyzed to report expected constraints on the structure of quartic vector boson interactions in the framework of dimension-8 effective field theory operators.
Speaker: Alexander Schuy (University of Washington) -
120
Beam Test Facilities for R&D in Accelerator Science and Technologies
Demonstrating the viability of emerging accelerator science ultimately relies on experimental validation. A portfolio of beam test facilities at US National Laboratories and Universities, as well as international facilities in Europe and Asia, are used to perform research critical to advancing accelerator science and technology (S&T). These facilities have enabled the pioneering accelerator research necessary to develop the next generation of energy-frontier and intensity-frontier User Facilities. This report provides an overview of the current portfolio of beam test facilities outlining: the research mission, the recent achievements, and the upgrades required to keep the US competitive in light of the large investments in accelerator research around the world.
Speaker: John Power (Argonne National Lab) -
121
Bootstrapping the Muon Collider: Massless Neutrinos in the g-2 Delivery Ring
The impedance model opens an old window on the roots of string theory via the S-matrix bootstrap. There is no Lagrangian. Equations of motion calculate mode impedances of the S-matrix. These govern amplitude and phase of energy transmission, such that the S-matrix impedance representation is also the gauge group, with direct interaction of both flavor and color matrix elements the citizens of Chew’s ‘nuclear democracy’. Naturalness comprises the consistency conditions[1]. The model requires just three assumptions - geometry, fields, and a mass gap - is finite without renormalization, and appears to be maximally analytically continued. There are no free parameters. It suggests a simple proof-of-principle experiment in the Fermilab muon g-2 delivery ring, demonstrating both massless oscillation and possibility of low-energy Muon Collider lifetime enhancement, complementary to high-energy time dilation of the Lorentz transform[2].
[1]https://www.researchgate.net/publication/335240613_Naturalness_begets_Naturalness_An_Emergent_Definition
[2]https://www.researchgate.net/publication/359592916_Bootstrapping_the_Muon_Collider_Massless_Neutrinos_in_the_g-2_Delivery_RingSpeaker: Peter Cameron (Michigan/MIT/Brookhaven (retired)) -
122
Bounds on Right Handed Neutrino Parameters from Observable Leptogenesis
We revisit the generation of a matter-antimatter asymmetry in the minimal extension of the Standard Model with two singlet heavy neutral leptons (HNL) that can explain neutrino masses. We derive an accurate analytical approximation to the solution of the complete set of kinetic equations, which exposes the non-trivial parameter dependencies in the form of parameterization-independent CP-invariants. The analytical approximation reveals various washout regimes that are relevant in different regions of parameter space, exposes the relevance of helicity-breaking corrections in the interaction rates, and clarifies the correlations of baryogenesis with other observables. In particular, requiring that the correct baryon asymmetry is reproduced, we derive robust upper or lower bounds on the HNL mixings depending on their masses, and constrain their flavour structure, as well as the CP-violating phases of the PMNS mixing matrix, and the amplitude of neutrinoless double-beta decay. We also find certain correlations between low and high scale CP phases. All these findings are confronted with numerical scans of parameter space with very good agreement. The methods developed in this work can help in exploring more complex scenarios.
Speaker: Stefan Sandner (IFIC UV / CSIC) -
123
BREAD: Broadband Reflector Experiment for Axion Detection
We present a novel dish antenna for broadband ~$\mu$eV-eV range axion and wave-dark matter detection, which allows to utilize state-of-the-art high-field solenoidal magnets. At these masses it is difficult to scale up traditional resonator setups to the required volume. However, at metallic surfaces in a high magnetic field dark matter axions can convert to photons regardless of axion mass. These photons can be successively focused onto a detector (dish antenna concept). We present progress on BREAD, a dish antenna proposal with a $\sim 10\,{\rm m}^2$ conversion area and a novel rotationally symmetric parabolic focusing reflector designed to take advantage of high-field solenoidal magnets. We recently demonstrated [PRL 128 (2022) 131801] that this concept has the potential to discover QCD axions of several decades in mass range. Besides the experimental concept this poster shows our progress towards first stage hidden photon and axion pilot experiments for two distinct frequency ranges - GigaBREAD and InfraBREAD - with expected sensitivities to unexplored coupling strengths. We detail R&D on reflector characterization, horn antenna & sensor testing and signal readout. We also outline sensitivity estimates for future large-scale versions.
Speaker: Stefan Knirck (Fermi National Accelerator Laboratory) -
124
Can tabletop experiments discover the graviton?
We argue that if the Newtonian gravitational field of a body can mediate entanglement with another body, then it should also be possible for the body producing the Newtonian field to entangle directly with on-shell gravitons. Our arguments are made by revisiting a gedankenexperiment previously analyzed by Belenchia et al., which showed that a quantum superposition of a massive body requires both quantized gravitational radiation and local vacuum fluctuations of the spacetime metric in order to avoid contradictions with complementarity and causality. We provide a precise and rigorous description of the entanglement and decoherence effects occurring in this gedankenexperiment, thereby significantly improving upon the back-of-the-envelope estimates given in the analysis of Belenchia et al. and also showing that their conclusions are valid in much more general circumstances. As a by-product of our analysis, we show that under the protocols of the gedankenexperiment, there is no clear distinction between entanglement mediated by the Newtonian gravitational field of a body and entanglement mediated by on-shell gravitons emitted by the body. This suggests that Newtonian entanglement implies the existence of graviton entanglement and supports the view that the experimental discovery of Newtonian entanglement may be viewed as implying the existence of the graviton.
Based on Phys. Rev. D 105, 086001 (2022). arXiv:2112.10798.
Speakers: Daine Danielson, Gautam Satishchandran (University of Chicago), Robert M. Wald (University of Chicago) -
125
Celeritas: : HEP detector simulation on GPUs
The previous Particle Physics Project Prioritization Panel (P5) report was responsible for consolidating a set of long term High Energy Physics (HEP) programs to address scientific questions on all three Department of Energy (DOE) Cosmic, Energy, and Intensity Frontiers. Two of these efforts are the High Luminosity Large Hadron Collider (HL-LHC) and its main experiments, and the Deep Underground Neutrino Experiment (DUNE). The unprecedented scale of these endeavors demands equally challenging computing capacity and storage requirements, with a commensurate fraction of the total computing cost being driven by Monte Carlo (MC) detector simulations. To alleviate this bottleneck, we present Celeritas, a new GPU MC detector simulation code designed to take advantage of the massive processing power of the DOE's Leadership Computing Facilities (LCFs). With Celeritas we plan to bridge the gap between HEP computing frameworks and the expanding DOE LCF network, vastly increasing the total compute capacity available to experiments for MC production campaigns. Here we present a roadmap for Celeritas, including its architecture, physics capabilities, and strategies for its integration with existing and future experimental HEP computing workflows.
Speaker: Seth R. Johnson (Oak Ridge National Laboratory) -
126
Constraining nuclear matrix elements from lattice QCD for beyond the Standard-Model explorations
Understanding the structure and interactions of nuclei is of special interest to the HEP community given the role of nuclei in experimental searches for violation of fundamental symmetries and searches for new physics. From neutrino physics to dark matter searches, nuclei are used as targets to probe new particles and new interactions. Interpreting the results of these experiments with fully controlled uncertainties requires a better theoretical understanding of nuclear medium. The goal of the NPLQCD collaboration is to compute the required nuclear matrix elements for light nuclei using lattice QCD calculations, and then constrain phenomenological models or effective field theories that are used in nuclear many-body calculations, expanding the validity of QCD-based results to larger nuclei. Particular examples of such calculations are the extraction of the axial charge and momentum fraction of light nuclei, needed to study neutrino-nucleus cross sections, identifying the short- and long-distance contributions to neutrinofull and neutrinoless double beta decays, and computing scalar and tensor matrix elements for dark matter and CP violation searches.
Speaker: Marc Illa Subina (University of Washington) -
127
Cosmogenic Background Mitigation at the ICARUS
The ICARUS detector will search for LSND-like neutrino oscillations exposed at shallow depth to the FNAL BNB beam as the far detector in the Short-Baseline Neutrino (SBN) program. Cosmic backgrounds rejection is particularly important for the ICARUS detector due to its larger size and distance from neutrino production compared to the near detector SBND. In ICARUS the neutrino signal over cosmic background ratio is 40 times more unfavorable compared to SBND, in addition a greater than 3 times larger out-of-spill comics rate. On this talk, I will illustrate techniques for reducing cosmogenic backgrounds in the ICARUS detector with initial commissioning data.
Speaker: Biswaranjan Behera (Colorado State University) -
128
CUPID: a next-generation neutrinoless double beta decay experiment.
The CUORE Upgrade with Particle Identification (CUPID) is a next-generation tonne scale neutrinoless double beta decay experiment that will be able to probe the inverted neutrino mass ordering region, test lepton number violation, and test the Majorana nature of neutrinos. CUPID’s scientific program will be built upon the experience from previous experiments CUORE, CUPID-Mo, and CUPID-0, supported by the detailed background model studies from those experiments. CUPID will consist of 1500 Li$_2$MoO$_4$ scintillating bolometric detector crystals amounting to a mass of 250 kg of $^{100}$Mo, the isotope of interest. We will present the latest developments towards the construction of the experiment and the projected performance in terms of energy resolution and background rejection.
Speaker: Jorge Torres (Yale University) -
129
Deep Learning Development and Deployment for Low-Latency Gravitational-Wave Astronomy
The successful electromagnetic observation of the neutron star merger GW170817 led to explosive growth in the field of multi-messenger astronomy. With that growth has come new challenges and opportunities. The computational needs of gravitational-wave astronomy have risen alongside the sensitivity of the global network of gravitational-wave detectors, and will continue to rise as more detectors with even greater sensitivity come online in the next decade. As the scale of data ramps up, new techniques are desired that will allow for low-latency detection of gravitational-waves and enable multi-messenger followup. We present two deep learning networks that are being developed to address this demand: DeepClean and BBHnet. In combination, these networks form an end-to-end pipeline capable of denoising gravitational-wave strain data and detecting binary black hole mergers. We also present steps that have been taken in the development of these algorithms that will encourage their widespread adoption and use. Taking lessons from industry and the field of machine learning operations, tools and procedures have been created that simplify the process of consistently training, testing, and implementing machine learning networks. This lowers the barrier to entry for end users, and ensures that effective analysis tools are actually applied to important science questions.
Speaker: William Benoit (University of Minnesota) -
130
Deep Lorentz Invariants for Particle Physics
A lot of attention has been paid to the applications of machine learning methods in physics experiments and theory. However, less attention is paid to the methods themselves and their viability as physics modeling tools. One of the most fundamental aspects of modeling physical phenomena is the identification of the symmetries that govern them. Incorporating symmetries into a model can reduce the risk of over-parameterization, and consequently improve a model's robustness and predictive power. As usage of neural networks continues to grow in the field of particle physics and as research in computer vision has demonstrated the usefulness of exploiting symmetries in data via network design, there is renewed interest in embedding the symmetries relevant to physics problems in neural networks which analyze them, as a means of applying physically-meaningful network constraints.
We present our work on Lorentz group-invariant and equivariant networks, within the context of problems including jet tagging and particle four-momentum prediction. Building off of previous work, we demonstrate how careful choice in the details of network design -- creating a model drastically simpler than the traditional approaches -- can yield competitive performance. Such symmetry-respecting networks may not only serve as powerful analysis tools themselves, but by design may offer insights into which composite physical observables are relevant in particle identification and measurement tasks.
Speakers: Dr Alexander Bogatskii (Flatiron Institute), Jan Offermann (University of Chicago) -
131
Detecting Dark Matter with a Qubit
To perform experimental searches for low mass bosonic dark matter such as the hidden photon or axion, our group works to employ dielectric photonic bandgap cavities with a high quality factor to coherently accumulate the axion signal for readout using qubit-based single photon detectors. The advantage of the qubit-based detector is in overcoming the standard quantum noise limit through repeated quantum non-demolition measurements [1]. Other techniques being studied include preparing the dielectric cavity in a higher photon-number (n) Fock state to enhance the dark matter signal amplitude by a factor of (n+1). Given the large parameter space still unexplored by current dark matter searches, methods of tuning a resonant cavity by electronically controlling the magnetic field seen by a loop of two Josephson junctions is currently being studied.
[1] Dixit et al., Phys. Rev. Lett. 126, 141302 (2021)
Speaker: Morgan Lynn (University of Chicago/Fermilab) -
132
Detector performance for Higgs physics measurements at muon collider
The muon collider is the ideal machine for reaching multi-TeV centre-of-mass energy and high luminosity lepton collisions, thanks to the low beamstrahlung and synchrotron radiation loss compared to $e^{+}e^{-}$ colliders.
In such conditions, the number of produced Higgs bosons will allow to measure its couplings to fermions and bosons with an unprecedented precision.
However, in order to evaluate its physics reaches, the detector performance must be determined, since they may be strongly affected by very high fluxes of particles coming from muons decaying in circulating beams.
In this contribution beam-induced background effects on the detector components and physics object reconstruction strategies are discussed. Latest results on jet reconstruction and jet flavour identification performance, evaluated via full simulation of the muon collider detector, are presented.
Most recent results on the precision on the measurement of the $\mu^{+}\mu^{-} \to H \nu \bar{\nu}$ cross section, where the Higgs boson decay in two b-jets, are shown. The signal and the physics background are fully simulated and reconstructed at 3 TeV center of mass energy, including the beam-induced background.Speaker: Laura Buonincontri -
133
Development of a hybrid amorphous selenium/CMOS charge sensor for the Selena neutrino experiment
The Selena neutrino experiment couples an amorphous selenium (aSe) ionization target to a complimentary metal-oxide semiconductor (CMOS) active pixel array as an imaging detector for next generation neutrino physics. The high Q$_{\beta\beta}$ of $^{82}$Se and the excellent event classification allows for a search for neutrinoless $\beta\beta$ decay free from environmental backgrounds. Furthermore, we can take advantage of the spatiotemporal resolution to perform high efficiency electron neutrino spectroscopy for solar neutrino studies and sterile neutrino searches. The Selena experiment will operate with a 10-ton target for a 100-ton year exposure. We are currently characterizing our first prototypes of the Selena detectors, which consist of 500um of aSe deposited on the Topmetal-II$^-$ CMOS pixel charge sensor. We present R\&D results from our studies and show the induced tracks within our detector, as well as a noise performance of $22.7\pm0.4$ electrons. We also present status on the development of the next version of the Selena detectors.
Speaker: Xiaochen Ni (University of Washington) -
134
Development of ultrafast silicon sensors for precision timing and 4D tracking
Low Gain Avalanche Detectors (LGADs) are thin silicon detectors with moderate internal signal amplification, providing time resolution of <20 ps for minimum ionizing particles. LGADs are the key silicon sensor technology for the timing detectors of the CMS and ATLAS experiments in the HL-LHC. In addition, their fast rise time and short full charge collection time (as low as 1 ns) is suitable for high repetition rate measurements in photon science and other fields. However, while radiation hardness and fabrication of such sensors on a larger scale are maturing, electric field termination structures remain a major restricting factor for spatial resolution as they currently limit the granularity of LGAD sensors to the mm scale.
New ultrafast silicon sensors, produced by HPK, FBK, BNL and other vendors, are studied with C-V/I-V measurements, red and IR laser scans, radioactive sources and charged particle test beams. The results are used to recommend base-line sensors for near-future large-scale detector applications like the Electron-Ion Collider, where simultaneous precision timing and position resolution is required. The studies also serve research and development of silicon sensors for other future colliders.
AC-LGADs, also referred to as resistive silicon detectors, are a more recent variety of LGADs based on a sensor design where the multiplication and n+ layers are continuous, and only the metal layer is patterned. This simplifies sensor fabrication and reduces the dead area on the detector, improving the hit efficiency while retaining the excellent fast timing capabilities of LGAD technology. In AC-LGADs, the signal is capacitively coupled from the continuous, resistive n+ layer over a dielectric to the metal electrodes. A high spatial precision on the few 10‘s of micrometer scale is achieved by using the information from multiple pads, exploiting the intrinsic charge sharing capabilities provided by the common n+ layer. A balance between all tunable parameters (comprehending location, the pitch and size of the pads, as well as the doping concentrations) has to be identified for future uses of AC-LGADs: the sensor design can be optimized for each specific application to achieve the desired position and time resolution compromised with the readout channel density. Their precise temporal and spatial make AC-LGADs primary candidates for future 4-D tracking detectors, and they are currently the chosen technology for near-future large-scale application like the Electron-Ion Collider detector at BNL, or the PIONEER experiment at the Paul Scherrer Institute in Switzerland.
Another type of sensor design aimed at reducing the inactive area is the trench-insulated (TI-)LGAD, in which the gain regions are isolated from each other by etching narrow trenches into the silicon substrate between segments. Furthermore, prototypes of LGADs with a continuous, but buried gain layer (deep-junction, DJ-LGADs) are being investigated.
In all aforementioned varieties of LGADs, the contribution of Landau energy transfer fluctuations on the timing resolution are sought to be reduced by decreasing the substrate thickness, from a typical 50 µm to 25-35 µm and less, to approach a timing resolution of ultimately around 10 ps.
Speaker: Adam Molnar (SCIPP (Santa Cruz Institute for Particle Physics)) -
135
Exploring the lifetime and cosmic frontier with the proposed MATHUSLA experiment
The proposed MATHUSLA experiment (MAssive Timing Hodoscope for Ultra-Stable neutraL pArticles) could open a new avenue for discovery of Physics Beyond the Standard Model at the LHC. The large-volume detector will be placed above the CMS experiment with O(100) m of rock separation from the LHC interaction point. It is instrumented with a tracking system to observe long-lived particle decays inside its empty volume. The experiment is composed of a modular array of detectors covering together (100 × 100) m$^2$ × 25 m high. It is planned in time for the high luminosity LHC runs. With a large detection area and good granularity tracking system, MATHUSLA is also an efficient cosmic-ray Extensive Air Shower (EAS) detector. With good timing, spatial and angular resolution, the several tracking layers allow precise cosmic-ray measurements up to the PeV scale that compliment other experiments.
We will describe the detector concept and layout, the status of the project, the on-going cosmic ray studies, as well as the future plans. We will focus on the current R&D on 2.5 m long extruded plastic scintillator bars readout by wavelength shifting fibers connected to Silicon Photomultipliers (SiPM) located at each end of the bar. We will discuss the studies made on possible fiber layout, dopant concentration, as well as report on the timing resolution measurements obtained using Saint Gobain and Kuraray fibers. We will also describe the tests made on the Hamamatsu and Broadcom SiPM, a possible SiPM cooling system using chillers, as well as highlight the structure of the trigger and data acquisition. Moreover, we will discuss the proposal of adding a 10$^4$ m$^2$ layer of RPCs with both digital and analogue readout to improve significantly cosmic ray studies in the 100 TeV – 100 PeV energy range with a focus on large zenith angle EAS.Speaker: Mason Proffitt -
136
FASER Tracker Detector - Commissioning, Installation, and Functionality
FASER (ForwArd Search ExpeRiment) fills the axial blindspot of other, radially arranged LHC experiments. It is installed 480 meters from the ATLAS interaction point, along the collision axis. FASER will search for new, long-lived particles that may be hidden in the collimated reaction products exiting ATLAS. The tracking detector is an essential component for observing LLP signals. FASER's tracking stations use silicon microstrip detectors to measure the path of charged particles. This presentation is a summary of one of FASER's latest papers "The tracking detector of the FASER experiment" which describes the functionality, construction and testing of the tracker detector. FASER is currently installed in the LHC, where it is now collecting data.
Speaker: Savannah Shively (University of California Irvine (US)) -
137
Fast collider simulations with graph neural networks.
There has been significant development recently in generative models for accelerating collider simulations. Work on simulating jets, extremely prevalent at hadron colliders such as the LHC and potentially FCC-hh, has primarily used image-based representations, which tend to be sparse and of limited resolution. We advocate for the more natural ‘particle cloud’ representation of jets, i.e. as a set of particles in momentum space, and discuss four physics- and computer-vision-inspired metrics: (1) the 1-Wasserstein distance between high- and low-level feature distributions; (2) a new Fréchet ParticleNet Distance; (3) the coverage; and (4) the minimum matching distance as means of quantitatively and holistically evaluating generated particle clouds. We then present our new graph message-passing generative adversarial network (MPGAN), which has excellent performance on gluon, top quark, and lighter quark jets on all metrics, validated against real samples via bootstrapping as well as existing point cloud generative models. We measure a three-orders-of-magnitude improvement in latency as compared to traditional simple Monte Carlo simulations, and anticipate up to five-orders-of-magnitude improvements compared to full detector simulations at current and future colliders. This technique thus shows significant promise for addressing the computational needs of High-Luminosity-LHC and future colliders.
Speaker: Raghav Kansal -
138
Fiber-optic diagnostic system for future accelerator magnets
The next generation high energy physics accelerators will require magnetic fields at ~20 T. HTS coils will be an essential component of future accelerator magnets and several efforts are currently dedicated on designing 20 T HTS- LTS hybrid magnets. Among the existing challenges, there is the lack of a robust quench detection system for hybrid magnet technology. Another big challenge is represented by the high number of training quenches required by Nb3Sn magnets to reach performance level..
In this paper, we propose the use of fiber optics sensors for diagnostic and quench detection in future accelerator superconducting magnets. Discrete and distributed fiber optic sensors have demonstrated to be a promising tool. The goal is to instrument hundreds of accelerator superconducting magnets and to move beyond the proof-of-concept level. Significant developments are still needed. Here, we are going to present the most recent results and discuss the most urgent technical developments in order to make those sensors a robust and reliable diagnostic tool for accelerator superconducting magnets over the next 10 year.
We foresee that discrete fiber sensors will be a stable diagnostic probe for superconducting magnets over the next 3 to 5 years. More R&D work will be necessary for distributed fibers. The most urgent needs are the increase of sample rate and sensitivity. Close collaboration with vendors will be necessary to improve mechanical properties and fabrication processes to produce hundreds of meters of fiber and instrument many accelerator superconducting magnets. Those R&D efforts will last up to 10 years with a founding level that spans between 5-10 M$.Speaker: Maria Baldini (FNAL) -
139
Future Compact Multi-TeV e+e- and Gamma-Gamma Collider Opportunities Based on Advanced Plasma and Structure Accelerators
Plasma and structure accelerators present a long-term path to a new generation of more compact, multi-TeV, e+e- and gamma-gamma colliders. They provide ultrahigh (1–100+ GeV/m) acceleration gradients and have made rapid progress in the last decade. These acceleration concepts rely on the generation of a wakefield which contains intense electric fields enabling particle acceleration for example to 8 GeV in 20 cm or 42 GeV in 85 cm. In the laser wakefield accelerator (LWFA) and plasma wakefield accelerator (PWFA) the wakefields are driven in a plasma by intense laser or particle beams, respectively; in the structure wakefield accelerator (SWFA), the wake is excited by a particle bunch propagating through a slow-wave structure. These schemes accelerate ultrashort bunches (10 fs–1 ps) and hence mitigate current beamstrahlung limits in TeV lepton collisions. We propose an integrated design study for a machine that would address the future goals of particle physics, a polarized e+e- and gamma collider with up to 15 TeV in the center of mass and a path forward including an intermediate energy demonstrator facility at 20-100 GeV.
Speaker: Marlene Turner (LBNL) -
140
Gamma-Ray and AntiMatter Survey (GRAMS) for antimatter detection
Gamma-Ray and AntiMatter Survey (GRAMS) is a next-generation balloon-/satellite-based experiment using a Liquid Argon Time Projection Chamber (LArTPC) detector to detect Gamma-rays and antiparticles. With a cost-effective and large-scale LArTPC, GRAMS can achieve high sensitivity towards antiparticle searches within the low energy region ( <0.5GeV ), where we can have essentially background-free dark matter searches. We can potentially validate various dark matter models with this sensitivity.
Currently, we are building and testing prototype GRAMS devices parallelly at Northeastern University (US), Tokyo University (Japan), and Waseda University (Japan) to demonstrate our detection concept.
In this poster presentation, I will discuss the detection concept for antimatter measurements and hardware R&D at Northeastern University, as well as the GRAMS sensitivities to cosmic antinuclei, especially antihelium-3.Speaker: Jiancheng Zeng -
141
Graph Neural Network for Large Radius Tracking
Particle tracking is a challenging pattern recognition task in experimental particle physics. Traditionally, algorithms based on the Kalman filter are used for such tasks and show desirable performance in finding tracks originating from the interaction point. However, many Beyond Standard Model (BSM) theories predict the existence of long-lived particles (LLP). They have a longer lifetime and travel a distance before decaying to Standard Model particles, resulting in large radius tracks. For such displaced tracks, dedicated tunings are often required to reach sensible performance since the quality of seeds for the Kalman filter has a direct impact on its performance.
Recent studies show machine learning-based particle track finding algorithms using graph neural networks (GNN) achieve competitive physics and computing performance for tracks originating from the interaction point. In this work, we developed a GNN-based end-to-end particle track finding algorithm for the High Luminosity LHC and apply such an algorithm to displaced track datasets to study the performance of reconstructing displaced tracks. The algorithm is designed to be agnostic about global track position. The datasets are generated under the ACTS framework and simulated for a generic detector. As the result, we reconstruct prompt and displaced tracks simultaneously with high track efficiency and no significant drop for displaced tracks.
Speaker: Chun-Yi Wang (National Tsing Hua University, ) -
142
H → µµ at a 3-TeV muon collider
Among the projects currently under study for the next generation of
particle accelerators, the muon collider represents a unique machine,
which has the capability to provide leptonic collisions at energies of
several TeV. The multi-TeV energy regime is as yet unexplored and holds
a huge physical potential that will enable a novel research programme
ranging from high precision measurements of known standard model
processes to high-sensitivity searches for phenomena beyond the standard
model. A multi-TeV muon collider will produce huge samples of Higgs
bosons that will allow a determination of the Higgs boson properties
with unprecedented precision, like its couplings to fermions and bosons
and its trilinear and quartic self-couplings.
This contribution will present a study, based on a detailed detector
simulation and a full-fledged muon reconstruction, of the muon collider
prospects for the H → μμ production, one of the rarest Higgs boson
processes that represents a gateway to the determination of the Higgs
boson coupling to the second generation leptons.Speaker: Alessandro Montella -
143
Higgs boson decay width and couplings at muon collider
Among the facilities proposed for the next generation of particle accelerators for High Energy Physics, the muon collider represents a unique machine, which would be able to provide leptonic collisions at energies of several TeV.
Muons collisions at such energy scale holds a remarkable physic potential, both for searches of phenomena beyond the Standard Model, and precision measurements of known processes.
In particular, in the multi-TeV regime, Higgs production rates are so high that Higgs physics measurements, such as its couplings to bosons and fermions and its decay width, can be achieved with unprecedented precision.
This contribution aims to give an overview of the results obtained so far on Higgs couplings and width by studying single Higgs boson production occurring by vector boson fusion (VBF).
All the studies have been performed simulating the relevant physics processes at a 3 TeV muon collider, taking into account the effects of the Beam Induced Background on the detector performance.
The indirect measurement of the Higgs width is possible thanks to the simultaneous search for on-shell and off-shell Higgs boson decaying to a pair of vector bosons ($H \rightarrow WW$ and $H \rightarrow ZZ$), an analysis strategy already used by LHC experiments.
The knowledge of the Higgs width allows to determine, in a model-independent way, all Higgs boson couplings from $\sigma(\mu^+ \mu^- \rightarrow H) \cdot BR(H \rightarrow xx)$ measurements.Speaker: Luca Giambastiani (University and INFN, Padova) -
144
High efficiency microwave-optical transduction for quantum sensing and computing
Superconducting radio-frequency (SRF) cavities play a crucial role in quantum computing and various quantum applications. These cavities also provide powerful tools to probe fundamental physics. At Fermilab, we are exploring ways to use hybridized SRF cavities as quantum transducers to convert microwave-optical quantum signals with high fidelity and high efficiency. Currently, quantum transduction demonstrations are limited in conversion efficiency, with most schemes operating in the high-pump regime, therefore with large noise. Our strategy exploits Fermilab’s 3D bulk niobium cavities using high densities of electromagnetic fields in large RF volumes. We couple these cavities to noncentrosymmetric crystals, used as optical resonators. The large flexibility of the cavity geometry provides new degrees of freedom to optimize the microwave-optical coupling strength. The high microwave quality factor and large coupling strength between microwave and optical modes are expected to lead to orders of magnitude enhancements for transduction efficiency at a low pump power of tens of μW. We present ongoing and future research on optical-microwave transduction, which would have an impact on single-photon sensing and networks, with the ability to perform measurements below the standard quantum limit (SQL). In quantum sensing up/down photon conversion may also enable highly sensitive axion and dark photon haloscope searches in the THz regime. In quantum computing these hybrid devices would be a first building block for the realization of distributed quantum networks.
Speaker: Silvia Zorzetti (Fermilab) -
145
Improving DiHiggs sensitivity in the hadronic final state using machine learning
One of the central goals of the physics program at the future colliders is to elucidate the origin of electroweak symmetry breaking, including precision measurements of the Higgs sector. This includes a detailed study of Higgs boson pair production, which can reveal the Higgs self-interaction strength through the gluon fusion mode as well as the coupling between Higgs and vector bosons through the vector boson fusion mode. Since the discovery of the Higgs boson, a large campaign of measurements of the properties of the Higgs boson has begun and many new ideas have emerged during the completion of this program. One such idea is the use of highly boosted and merged hadronic decays of the Higgs boson (H→bb, H→WW→qqqq ) with machine learning methods to improve the signal-to-background discrimination. In this project, we champion the use of these modes to boost the sensitivity of future collider physics programs to Higgs boson pair production and the Higgs self-coupling. In this presentation, we aim to demonstrate the advantages of graph neural networks over standard cut-based event selection methods to achieve better sensitivity.
Speaker: Brian Sheldon (University of California San Diego) -
146
Improving the hadron EDM upper limit using doubly-magic proton and helion beams
The upper limit on (time reversal symmetry T-violating) permanent hadron electric dipole moments (EDMs) is the PSI neutron EDM value; $d_n = (0.0\pm1.1_{\rm stat}\pm0.2_{\rm sys}\times10^{-26}$\,e.cm. This paper describes an experiment to be performed at a BNL-proposed CLIP project which is to be capable of producing intense polarized beams of protons, $p$, helions (He${}^3$ nuclei), h, and other isotopes.
The EDM prototype ring PTR (proposed at COSY Lab, Juelich) is expected to measure individual particle EDMs (for example ${\rm EDM\_p}$ for the proton) using simultaneous coumter-rotating polarized proton beams, with statistical error $\pm10^{-30}$e.cm after one year running time, four orders of magnitude less than the PSI neutron EDM upper limit, and with comparable systematic error.
A composite particle, the helion faces T-symmetry constraints more challenging than the proton. Any measureably large value of $$\delta={\rm EDM}_h-{\rm EDM}_p$$ would represent BSM physics. The plan is to replicate PTR at BNL. The dominant systematic error would be cancelled two ways, both made possible by phase-locking ``doubly-magic'' 38.6\dots MeV proton and 39.2\dots MeV helion spin tunes. This stabilizes their MDM-induced in-plane precessions, without affecting their EDM-induced out-of-plane precessions. The dominant systematic error would therefore cancel in the meaurement of $\delta$ in a fixed field configuration.
Another systematic error cancellation will come from averaging runs for which both magnetic field and beam circulation directions are reversed. Precise magnetic field reversal is made possible by the reproducible absolute frequency phase-locking over long runs to eliminate the need for (impractically precise) magnetic field measurement.Speaker: Richard Talman (Laboratory of Elementary Particle Physics, Cornell University) -
147
Invisible diversity. Are hidden disabilities hiding potential for physics?
Hidden disabilities are typically understood in light of the obstacles they present for students and researchers to succeed in academia. However, the same differences that fuel these conditions can provide a rich source of cognitive diversity to an environment that enables diversity to thrive. Cognitive diversity has great potential to contribute to the scientific output of our field by enhancing our collective problem-solving abilities, innovation, and creativity, among others. This presentation will discuss the advantageous potential that neuro-diversity can bring to our field, and explore the impacts of standardized tests and other barriers to the integration of students and researchers with hidden disabilities from the standpoint of Attention Deficit Hyperactivity Disorder (ADHD).
Speaker: Fernanda Psihas Olmedo (Fermi National Accelerator Laboratory) -
148
Julia language for HEP analysis: faster time to insight and enabling more complex analysis
As the data collection grows larger and computational/statistical techniques become more complex, many physics analysis users are experiencing a "two-language problem"1 without knowing it.
Julia and the ever-growing JuliaHEP2 ecosystem aim to provide end-users the ability to chew through a larger amount of data faster, by being a JIT language from the ground up. And also enable users to do custom machine learning and training because the pure-Julia ecosystem would allow automatic differentiation to propagate freely without foreign-library call barrier.
The poster presenter would talk about:
- Julia and why it's designed precisely for workloads like physics analysis
- How mono language enables effortless parallelization and automatic differentiation
- UnROOT.jl, BAT.jl, pyhf, FHist.jl, etc. and workflow for an end-user analysis in Julia
- Custom training and inference loop based on data before N-tupleized -- enable deeper insight into raw event data, supported by Julia's speed and auto diff ability.Speaker: Jerry Ling (Harvard University) -
149
Longitudinally polarized ZZ scattering at a muon collider
Measuring longitudinally polarized vector boson scattering in, e.g., the $ZZ$ channel is a promising way to investigate the unitarization scheme from the Higgs and possible new physics beyond the Standard Model. However, at the LHC, it demands the end of the HL-LHC lifetime luminosity, 3000$fb^{-1}$, and advanced data analysis technique to reach the discovery threshold due to its small production rates. Instead, there could be great potential at future colliders. We perform a Monte Carlo study and examine the projected sensitivity of longitudinally polarized $ZZ$ scattering at a TeV scale muon collider. We conduct studies at 14TeV and 6TeV muon colliders respectively and find that a 5 standard deviation discovery can be achieved at a 14TeV muon collider, with 3000$fb^{-1}$ of data collected. While a 6TeV muon collider can already surpass HL-LHC, reaching 2 standard deviations with around 4$ab^{-1}$ of data. The effect from lepton isolation and detector granularity is also discussed, which may be more obvious at higher energy muon colliders, as the leptons from longitudinally polarized Z decays tend to be closer.
Speaker: Tianyi Yang (Peking University(CN)) -
150
Low energy calibration and characterization of novel dark matter detectors with a scanning laser device
A major hurdle in searches for sub-GeV particle-like dark matter is demonstrating sufficiently low energy detection thresholds in order to detect recoils from light dark matter particles. Many detector concepts have been proposed to achieve this goal, which often include novel detector target media or sensor technology. A universal challenge in understanding the signals from these new detectors and enabling discovery potential is characterization of detector response near threshold, as the calibration methods available at low energies are very limited. We have developed a cryogenic device for robust calibration of any photon-sensitive detector over the energy range of 0.62-6.89eV. This device can be used to scan over a detector and deliver narrowly-collimated pulses of small numbers of photons in a way that limits parasitic backgrounds, allowing for exploration of a variety of science targets including phonon transport in materials and the effect of quasiparticle poisoning. Design overview and specifications and current status are presented.
Speaker: Kelly Stifter (Fermilab) -
151
Low-Energy Electron-Track Imaging for a Liquid-Argon Time-Projection Chamber using Probabilistic Deep Learning
The GammaTPC is an MeV-scale single-phase liquid-argon time-projection-chamber gamma-ray telescope with a novel dual-scale pixel-based charge-readout system. It promises to enable a significant improvement in sensitivity to MeV-scale gamma rays over previous telescopes. The novel pixel-based charge readout allows for the imaging of the tracks of electrons scattered by Compton interactions of incident gamma rays. The two primary contributors to the accuracy of a Compton telescope are its energy and position resolution. In this work, we are concerned with optimization of the position resolution and also reconstruction of the direction of the electron scattered in a Compton interaction. To this end, we utilize different deterministic and probabilistic deep learning approaches to estimate the position and initial direction of the scattered electron, and to quantify the uncertainty in the predictions. We show that the deep learning models are able to predict precise locations of Compton scatters of MeV-scale gamma rays from realistic pixel based data. Additionally, the predictive uncertainties are used to restrict the specific gamma interactions to be analyzed, leading to improvements in fidelity and reliability of the reconstruction.
Speaker: Micah Buuck (SLAC National Accelerator Laboratory) -
152
Machine-detector interface studies for a multi-TeV muon collider
Circular muon colliders offer the prospect of colliding lepton beams at unprecedented center-of-mass energies. The continuous decay of stored muons poses, however, a significant technological challenge for the collider and detector design. The secondary radiation fields induced by decay electrons and positrons can strongly impede the detector performance and can limit the lifetime of detector components. Muon colliders therefore require an elaborate interaction region design, which integrates a custom detector shielding together with the detector envelope and the final focus system. In this paper, we present design studies for the machine-detector interface and we quantify the resulting beam-induced background for different center-of-mass energies (3 TeV and 10 TeV). Starting from the optics and shielding design developed by the MAP collaboration for 3 TeV, we devise an initial interaction region layout for the 10 TeV collider. In particular, we explore the impact of lattice and shielding design choices on the distribution of secondary particles entering the detector. The obtained results serve as crucial input for detector performance and radiation damage studies.
Speaker: Anton Lechner (CERN) -
153
Metastable anti-branes
Despite their consequential applications, certain aspects of metastable states of anti-branes in warped throats are not yet fully understood. In this poster, I will introduce the Kachru-Pearson-Verlinde (KPV) configuration, a frequently-discussed metastable configuration of anti-D3 branes at the tip of a Klebanov-Strassler throat, and briefly recap the decade-long discussions on its existence. I will present a new perturbative supergravity solution that captures the backreaction of a metastable state of anti-branes in the background of a particular modification of the Klebanov-Strassler throat in a long-wavelength approximation. Our solution, which has no unphysical singularities, describes how non-supersymmetric spherical NS5-branes with dissolved anti-D3 brane charge backreact in a fluxed throat geometry. I'll discuss how this perturbative solution, taken in conjunction with previous results, serves as strong evidence in favour of the existence of the KPV state.
The poster is based on a recent preprint [2112.04514] with Vasilis Niarchos. It is also greatly influenced by previous works [1812.01067] (PRL), [1904.13283] (JHEP), and [1912.04646] (JHEP) with Jay Armas, Vasilis Niarchos, Niels Obers, and Thomas Van Riet.
Speaker: Nam Nguyen (Durham University) -
154
MeV Gamma Ray Signatures from Dark Matter Annihilation and Evaporating Primordial Black Holes in the GRAMS Experiment
The upcoming GRAMS (Gamma-Ray and AntiMatter Survey) experiment aims to provide un- precedented sensitivity to a poorly explored region of the cosmic gamma-ray spectrum from 0.1-100 MeV, often referred to as the “MeV gap”. Utilizing Liquid Argon Time Projection Chamber (LArTPC) technology to detect these MeV gamma rays, GRAMS has the potential to uncover crucial details behind a variety of processes in multi-messenger astrophysics. Various theories on particle interactions beyond the standard model predict that dark matter annihilations may contribute to the cosmic gamma spectrum via monochromatic gamma emissions (spectral lines), the annihilation of decay products, and the radiation of electromagnetically charged final states (FSR). MeV gamma rays may also be emitted from primordial black holes (PBHs) which have gained interest in recent years as being potential candidates for dark matter. By looking for Hawking radiation in the MeV gamma-ray regime, GRAMS can likely probe for ultra-light PBHs, which theoretically may comprise a significant portion of dark matter in the Universe. Here, we will describe the MeV gamma-ray detection concept and the current status of the detector development.
Speaker: Jonathan LeyVa (Northeastern University) -
155
Modeling TXS 0506+056 Neutrino Flares for AMEGO-X
TXS 0506+056 is the first multimessenger blazar, having been detected twice by IceCube during events described as neutrino flares, one of which coincided with a gamma-ray flare. TXS 0506+056 is an unusual blazar independent of the coincident neutrino observations. We develop a one-zone, leptohadronic particle transport model and apply it to the historical broadband SED to establish a baseline for the physical parameters. Then, we look in more detail at the multiwavelength SED simultaneous with each neutrino event. The model is specifically designed to examine the effects of particle acceleration on the observable data through self-consistent implementation of both acceleration and emission processes. Additionally, we compare with other successful models from the literature that suggest divergent physical interpretations to suggest that AMEGO-X is well poised to differentiate between these models through multimessenger collaboration on blazar flares.
Speaker: Kristi Engel (University of Maryland, College Park) -
156
Muon monitor signal to predict NuMI beam parameters and horn current by applying Machine Learning techniques
The neutrino beam quality at the NuMI beamline is determined by observing the incident proton beam parameters and the horn current behaviors. Three arrays of muon monitors located in the downstream of the hadron absorber provide the measurements of the primary beam and horn current quality. We studied the response of muon monitors with the proton beam profile changes and focusing horn current variations.The responses of muon monitors have been used to implement Machine Learning (ML) algorithms to predict the beam parameters by spill-to-spill. In this work we demonstrate a ML application of predicting the beam position horizontal and vertical, beam intensity and horn current with a good prediction accuracy. This work is important for many future applications such as beam and horn current quality assurance and incident detections, neutrino beam systematics studies and neutrino beam quality assurance. Our results demonstrate the capability of developing useful ML applications for future beamlines such as LBNF.
Speaker: Don Athula Wickremasinghe (Fermilab) -
157
Neutrino flavor equilibration and $\nu p$ process nucleosynthesis in core-collapse supernovae
An enduring mystery in nuclear astrophysics pertains to the relatively high observed abundances of the proton-rich isotopes $^{92,94}$Mo and $^{96,98}$Ru. An attractive proposal to solve this problem is called the $\nu p$ process. This process could operate in a core-collapse supernova (CCSN) hot bubble, which is formed by a neutrino-driven matter outflow from the surface of the proto-neutron star after the shock is launched. Under certain conditions, the outflow can be proton-rich, and electron antineutrino captures on protons can create a subdominant neutron population, triggering $(n,\gamma)$ and $(n,p)$ reactions, which combined with $(p,\gamma)$ provide a pathway to make certain proton-rich nuclides considerably beyond the iron peak.
The precise outcome of $\nu p$ process nucleosynthesis depends on the exact physical conditions in the outflow, such as entropy, expansion timescale, electron fraction, and neutrino emission characteristics (luminosities and spectra). Here, we examine the effects of neutrino flavor equilibration near a proto-neutron star on the yields of the $\nu p$ process. Such flavor equilibration may arise, for instance, as a result of fast neutrino flavor conversions near a supernova core.
Speaker: Amol Patwardhan (SLAC) -
158
Neutrino self-interaction: boosting cosmic neutrinos with DSNB
Neutrinos might interact among themselves through forces that have so far remained hidden.
Throughout the history of the Universe, such secret interactions could lead to scatterings between the neutrinos from supernova explosions and the non-relativistic relic neutrinos left over from the Big Bang. Such scatterings can boost the cosmic neutrino background to O(MeV) energies, making it, in principle, observable in experiments searching for the diffuse supernova neutrino background.
Assuming a model-independent four-Fermi interaction, we determine the upscattered cosmic neutrino flux, and derive constraints on such secret interactions from the latest results from Super-Kamiokande. Furthermore, we also study prospects for detection of the boosted flux in future lead-based coherent elastic neutrino-nucleus scattering experiments.Speaker: Anirban Das (SLAC National Accelerator Laboratory) -
159
Operational islands in JT gravity
In this work, we revisit the problem of finding entanglement islands in 2d Jackiw-Teitelboim (JT) gravity. We implement the following adjustments to the traditional setup: (1) we do not explicitly couple to a non-gravitating system, instead we implement only pure absorption into a fiducial detector, (2) we utilize the operationally defined renormalized matter entanglement entropy, as defined by the boundary observer’s wordline. By ‘operational’ we mean in the sense that the observer has access to ‘clocks and rods’ to locate the position of the island. We show that this leads to a unitary Page curve that we explicitly compute, with an island outside of the event horizon. For a macroscopic black hole, this curve nicely follows Hawking's calculation first and then decreases with the Hawking-Bekenstein entropy.
Speaker: Julian De Vuyst (OIST) -
160
Physics Community Needs, Tools, and Resources for Machine Learning
Machine learning (ML) is becoming an increasingly important component of
cutting-edge physics research, but its computational requirements present significant challenges. In this poster, we discuss the needs of the physics
community regarding ML across latency and throughput regimes, the tools and
resources that offer the possibility of addressing these needs, and how these can
be best utilized and accessed in the coming years.Speaker: Elham E Khoda (University of Washington) -
161
PIONEER: Precision measurements of rare pion decays
In the past several years, there have been a number of experimental signals pointing to potential violation of lepton flavor universality. The PIONEER experiment, utilizing the Paul Scherrer Institutes' (PSI) infrastructure for particle physics (CHRISP), seeks to probe such Beyond the Standard Model (BSM) universality violating effects through the measurement of the branching ratio of the charged pion. These branching ratios are extremely sensitive to quantum effects of new particles at very high mass scales, and so can provide a window into physics beyond that which is directly accessible at colliders.
The Standard Model (SM) prediction for the charged pion branching ratio
$R_{e/\mu} \equiv \Gamma(\pi^+\rightarrow e^+\nu(\gamma))/\Gamma(\pi^+\rightarrow \mu^+\nu(\gamma))$ is known to the order of $10^{-4}$. This makes it one of the most precisely calculated hadronic quantities in the SM and is 15 times more precise than the current experimental average. Even with these large uncertainties, the experimental result exhibits a $1\sigma$ tension with universality. In the first phase of the experiment, we intend to match the theoretical uncertainty by measuring $R_{e/\mu}$ to $0.01\%$. This will allow us to test lepton flavor universality at an unprecedented level and probe mass scales up to the PeV range. In the second phase of the experiment, a $0.06\%$ measurement of the branching ratio of pion beta decay, $R_{\pi \beta} \equiv \Gamma(\pi^+\to \pi^0 e^+ \nu (\gamma))/\Gamma(\text{all})$, will provide another window into potential physics beyond the SM by providing a theoretically pristine measurement of ${\left|V_{ud}\right|}$.The experimental design incorporates lessons learned from the previous generation PIENU and PEN/PIBETA experiments at TRIUMF and PSI. In the PIONEER experiment design, an intense pion beam is brought to rest in a segmented, instrumented (active) target (ATAR). The proposed technology for the ATAR is based on low-gain avalanche detectors (LGADs), which can provide precise spatial and temporal resolution for particle tracks and thus separate even very closely spaced decays and decay products. The proposed detector will also include a 3$\pi$ sr, 25 radiation length ($X_0$) electromagnetic calorimeter, which measures the energy of the final state products from $\pi^{+}$ decay. A cylindrical tracker surrounding the ATAR is used to link the locations of pions stopping in the target to showers in the calorimeter. Our design boasts excellent energy and timing resolutions, a greatly enhanced calorimeter depth to reduce leakage, large solid angle coverage, and many more improvements. Each of these aspects is being actively modeled in simulation to ensure we will be able to meet our experimental goals.
Here, we present some theoretical motivations for PIONEER, discuss the experiment design, and show recent results from simulations and a first testing campaign at the PSI PiE5 charged pion beamline.
Speaker: Joshua Labounty (University of Washington) -
162
PIP2-BD: Searches for new physics with a stopped-pion source at the Fermilab accelerator complex
The PIP-II Linac at Fermilab is slated for operation later this decade and can support a MW-class $\mathcal{O}$(1~GeV) proton fixed-target program in addition to the beam required for DUNE. Proton collisions with a fixed target could produce a bright stopped-pion neutrino source. The addition of an accumulator ring allows for a pulsed neutrino source with a high duty factor to suppress backgrounds. The neutrino source supports a program of using coherent elastic neutrino-nucleus scattering (CEvNS) to search for new physics, such as sensitive searches for accelerator-produced light dark matter, active-to-sterile neutrino oscillations, and other BSM physics such as axion-like particles (ALPs). A key feature of the PIP2-BD program is the ability to design the detector hall at Fermilab specifically for HEP physics searches. I will present the PIP-II project and upgrades towards a stopped-pion neutrino source at Fermilab and studies showing the sensitivities of the conceptual PIP2-BD detector, a $\mathcal{O}$(100~ton) liquid argon scintillation detector, to the physics accessible with this source.
Speaker: Jacob Zettlemoyer (Fermilab) -
163
Probes of New Physics with MAGIS-100
The Matter-wave Atomic Gradiometer Interferometric Sensor (MAGIS-100), soon to be constructed at Fermilab, uses three coupled light-pulsed atom interferometers across a 100-meter baseline to probe external potentials as low as $10^{-20}$ eV. This sensitivity enables unparalleled reach into unexplored parameter space for ultralight scalar dark matter that couples to electrons or photons with mass above $10^{-15.5}$ eV, providing significant discovery potential. The sensor is also capable of performing searches for new forces, such as a $B-L$ coupled vector boson, when run in a dual-isotope interferometer mode. In addition to these new physics, MAGIS-100 will also be sensitive to gravitational waves in the “mid-band” region of frequency space (0.1 Hz - 10 Hz) between Advanced LIGO and LISA, and can perform precision tests of quantum mechanics at unprecedented length scales. This detector builds on expertise from the 10-meter prototype at Stanford and capitalizes on the latest advancement in atomic clock technology, and will serve as a pathfinder for a future kilometer-scale sensor. In this poster, I summarize the planned scientific program for the experiment and present projected sensitivities for various physics signals.
Speaker: Dylan Temples (Northwestern University) -
164
Probing axion dark energy using late-time polarized SZ with CMB
Next generation cosmic microwave background (CMB) experiments and galaxy surveys will generate a wealth of new data with unprecedented precision on small scales. Correlations between CMB anisotropies and the galaxy density carry valuable cosmological information about the largest scales, creating novel opportunities for inference. It is possible to foresee a cosmological paradigm shift, in which reconstruction of the gravitational weak-lensing potential, velocity fields and the remote quadrupole field will provide the most precise tests of fundamental physics. The use of the second-order effects in the CMB to extract this information motivate a strong push towards low noise, high resolution frontiers of the upcoming fourth generation CMB experiments. In this colloquium, I will discuss the prospects to use small-scale polarized Sunyaev Zel’dovich (pSZ) effect to probe the axion landscape and show how pSZ can distinguish between axion models where axion serves either as dark energy or as dark matter.
Speaker: Selim Hotinli (Johns Hopkins University) -
165
Probing heavy Majorana neutrino pair production at ILC in a $U(1)_{\rm B-L}$ extension of the Standard Model
We consider a gauged B$-$L (Baryon number minus Lepton number) extension of the Standard Model (SM), which is anomaly free in the presence of three SM singlet Right Handed Neutrinos (RHNs). Associated with the $U(1)_{\rm B-L}$ gauge symmetry breaking, the RHNs acquire Majorana masses and then with the electroweak symmetry breaking, tiny Majorana masses for the SM(-like) neutrinos are naturally generated by the seesaw mechanism. As a result of the seesaw mechanism, the heavy mass eigenstates which are mainly composed of the SM-singlet RHNs obtain suppressed electroweak interactions through small mixings with the SM neutrinos. To investigate the seesaw mechanism, we study the pair production of heavy Majorana neutrinos through the $U(1)_{\rm B-L}$ gauge boson $Z^\prime$ at the 250 GeV and 500 GeV International Linear Collider (ILC). Considering the current and prospective future bounds on the B$-$L model parameters from the search for a resonant $Z^\prime$ boson production at the Large Hadron Collider (LHC), we focus on a ``smoking-gun'' signature of the Majorana nature of the heavy neutrinos: a final state with a pair of same-sign, same-flavor leptons, small missing momentum, and four hadronic jets. We estimate the projected significance of the signature at the ILC.
Speaker: Jurina Nakajima (SOKENDAI/KEK) -
166
Probing ultra-light axions with the 21-cm signal during Cosmic Dawn
Ultra-light axions (ULAs) are a promising and intriguing set of dark-matter candidates. We study the prospects to use forthcoming measurements of 21-cm fluctuations from cosmic dawn to probe ULAs. In this poster, I focus in particular on the velocity acoustic oscillations (VAOs) in the large-scale 21-cm power spectrum, features imprinted by the long-wavelength (k∼0.1 1/Mpc) modulation, by dark-matter--baryon relative velocities, of the small-scale (k∼10−1000 1/Mpc) power required to produce the stars that heat the neutral hydrogen. Damping of small-scale power by ULAs reduces the star-formation rate at cosmic dawn which then leads to a reduced VAO amplitude. Accounting for different assumptions for feedback and foregrounds, I will show that the 21-cm experiments may be sensitive to ULAs with masses up to 10−18eV, two decades of mass higher than current constraints.
Speaker: Selim Hotinli (Johns Hopkins University) -
167
Prospects for the measurement of ttH production in the opposite-sign dilepton channel at √s = 14 TeV at the High-Luminosity LHC
Prospects for the measurement of top quark-antiquark associated Higgs boson (ttH) production in the HL-LHC era will be presented. The measurement is performed in the opposite sign dilepton channel focusing on the H → bb decay. A novel approach and the projection study for the HL-LHC is explored. The analysis strategy is based on the reconstruction of the Higgs boson invariant mass through the analytical solution of the kinematic equations of the ttH system, employs a neural network for the selection of data and makes use of a data-based method to estimate the main backgrounds.
Speaker: Charis Kleio Koraka (University of Wisconsin Madison (US)) -
168
Quantum Computing Simulation for Collective Neutrino Oscillations
Studies of neutrinos from astrophysical environments such as core-collapse supernovae, neutron star mergers and the early universe provide a large amount of information about various phenomena occurring in them. The description of the flavor oscillation is a crucial aspect for such studies, since the physics of matter under extreme conditions is strongly flavor-dependents (nucleosynthesis, proton/neutron ratio, spectral splits...).
It is well known that the neutrino flavor changes under the effect of 3 contributions: the vacuum oscillation, the interaction with the electrons of the surrounding matter, and the collective oscillations due to interactions between different neutrinos.
This last effect adds a non-linear contribution to the equations of motion, making the exact simulation of such a system inaccessible from any current classical computational resource.Our goal is to describe the real time evolution of a system of many neutrinos by implementing the unitary propagator $U(t) = e^{-iHt}$ using quantum computation and paying attention to the fact that the flavor Hamiltonian $H$, in the presence of neutrino-neutrino term, presents an all-to-all interaction
that makes the implementation of $U(t)$, into a quantum algorithm, strongly dependent on the qubit topology.
In this contribution we present an efficient way to simulate the coherent collective oscillations of a system of $N$ neutrinos motivating the benefits of full-qubit connectivity which allows for more freedom in gate decomposition and a smaller number of quantum gates making simulation on near-term quantum devises more feasible.
We present the results obtained from a real quantum simulation on a trapped-ions based quantum machine for the cases of $N=4$ and $N=8$ neutrinos.Speaker: Valentina Amitrano (University of Trento (Italy)) -
169
Real-time, intelligent data processing for the next-generation of particle imaging detectors
Liquid Argon Time Projection Chamber (LArTPC) particle detectors such as MicroBooNE, SBND, and DUNE produce 3D images of particle interactions using ionization charge collected by anode sensor arrays. One of the physics goals of these experiments is to look for rare and faint signals produced by interactions of beam-produced neutrinos or dark matter particles, or interactions of neutrinos from supernova bursts, or new fundamental physics such as baryon number violation processes. DUNE represents the largest LArTPC detector to be constructed, with millions of readout channels, where data rates can be as large as 5 terabytes per second. To record interactions of interest with 100% live time while meeting data storage and offline processing requirements, it is essential to reduce the data rates by implementing intelligent, real-time data selection techniques so as to preserve those rare signals with high accuracy. Existing LArTPCs such as MicroBooNE or the ProtoDUNE-Single Phase detector and their already collected data sets provide a unique opportunity to demonstrate data selection techniques following the DUNE data-selection strategy, providing an important proof-of-principle for applying such techniques to DUNE and other upcoming LArTPC experiments. This poster will describe the ongoing R&D efforts to also develop and demonstrate more advanced, AI-driven real-time data processing and data selection techniques, using the MicroBooNE and SBND detectors, and discusses real-time data processing challenges and opportunities for the next decade.
Speaker: Dr Daisy Kalra (Columbia University) -
170
Reshaping THz Near-Fields for Efficient Particle Acceleration
Significant developments in accelerator technology will be essential for particle colliders to reach the energies necessary for the next breakthrough in high energy particle physics. THz-frequency structures could provide the gradients needed for next generation particle accelerators with compact, GeV/m-scale devices. One of the most promising THz generation techniques to drive compact structures is optical rectification in lithium niobate using the tilted pulse front method. However, THz accelerator applications using this method are limited by significant losses during transport of THz radiation from the generating nonlinear crystal to the acceleration structure. In addition, the spectral properties of high-field THz sources make it difficult to couple THz radiation into accelerating structures. Constructing an accelerating structure partially out of lithium niobate would allow the integration of THz generation and electron acceleration, and remove the losses due to transport and coupling. In order to design this structure a robust understanding is needed of the THz near-field source properties and how they are affected by changes in the generation setup. We have developed a technique for detailed measurement of the THz near-fields and used it to reconstruct the full temporal 3D THz near-field close to the LN emission face. Analysis of the results from this measurement will inform designs of novel structures for use in THz particle acceleration.
Speaker: Annika Gabriel (SLAC National Accelerator Laboratory) -
171
Search for exotic B decays and low mass dimuon resonances using data scouting at CMS
Enabled by the novel technique of data scouting, CMS reach for low mass resonances has improved significantly. In this poster, we present the first search for a light scalar arising from the decay of a B hadron at CMS along with the search for low mass long lived dark photons that decay to muon pairs. We also provide supplementary material to recast our analysis results to any other model. Using our analysis results, we also show that CMS is competitive with LHCb in the B-regime.
Speaker: Hardik Routray -
172
Search for Neutral Long-lived Particles Decaying in the CMS Endcap Muon Detectors
Many extensions of the standard model (SM) predict the existence of neutral, weakly-coupled particles that have a long lifetime. These long-lived particles (LLPs) often provide striking displaced signatures in detectors, thus escaping the conventional searches for prompt particles and remaining largely unexplored at the LHC.
I will present a first search at the LHC that uses a muon detector as a sampling calorimeter to identify displaced showers produced by decays of LLPs. The search is sensitive to LLPs decaying to final states including hadrons, taus, electrons, or photon, LLP masses as low as a few GeV, and is largely model-independent. The search is enabled by the unique design of CMS endcap muon detectors (EMD), composed of detector planes interleaved with the steel layers of the magnet flux-return yoke. Decays of LLPs in the EMD induce hadronic and electromagnetic showers, giving rise to a high hit multiplicity in localized detector regions that can be efficiently identified with a novel reconstruction technique. The steel flux-return yoke in the CMS detector also provides exceptional shielding from the SM background that dominates existing LLP searches. The search yields competitive sensitivity for proper lifetime from 0.1m to 1000m with the full Run2 dataset recorded at the LHC.
I will present the result of the search, as well as the supplementary materials that allow for reinterpretation of the analysis to any models containing LLPs. I will show the recast and projected sensitivity of this search in a few benchmark models. We show that this new search approach is sensitive to LLPs as light as a few GeV, and can be complementary to proposed and existing dedicated LLP experiments.
Speaker: Christina Wang (California Institute of Technology) -
173
Searching for rare processes in short-baseline neutrino experiments with liquid argon time projection chambers
A number of anomalies have been observed in accelerator-based short-baseline neutrino experiments since the 1990s, including the LSND anomaly and MiniBooNE low energy excess (LEE), motivating follow-up searches for exotic new physics Beyond the Standard Model (BSM). At the same time, the liquid argon time projection chamber (LArTPC) technology offers unprecedented spatial and calorimetric resolution for neutrino scattering in the 100 MeV to a few GeV energy range, and thus is a great platform for precise and sensitive searches for new physics in accelerator-based neutrino beams. MicroBooNE is an 85-tonne active mass LArTPC detector, which finished its neutrino run in 2020, and whose primary physics goal has been the investigation of the MiniBooNE LEE. MicroBooNE released its first results in October 2021, including results from a search for anomalously large single-photon production through neutrino-nucleus neutral current Delta resonance production, followed by Delta radiative decay. Follow-up analyses in MicroBooNE include searches for even rarer single-photon processes such as neutrino-nucleus coherent single-photon production, or BSM processes due to dark sector models predicting neutrino up-scattering and decaying into electron-positron pairs. Such processes can also be searched for with the upcoming Short-Baseline Near Detector (SBND) — a 112-tonne active mass LArTPC located in the same neutrino beamline as MicroBooNE, which will run as part of the Fermilab SBN program beginning in 2023. This poster will review opportunities for precise and sensitive searches for rare and new physics processes with MicroBooNE and SBN.
Speaker: Guanqun Ge (Columbia University) -
174
Searching for Wavelike Dark Matter with SRF Cavities
Haloscopes consisting of a microwave cavity with a high quality factor (Q) connected to low noise electronics have been deployed to directly detect wavelike axions and dark photons. But the dark matter mass is unknown, so haloscopes must be tunable to search through the photon coupling vs. mass parameter space. The scan rate for haloscope experiments is a key figure of merit and is dependent on the cavity’s quality factor. State-of-the-art experiments like ADMX currently use copper cavities with Q~80000. But implementing SRF cavities with Q~10^10 can increase the scan rate by possibly a factor of 10^5.
This poster will describe the principles behind operating a haloscope whose bandwidth is much narrower than the dark matter halo energy distribution. The poster will highlight proof-of-principle measurements that already demonstrate that ultra-high Q cavities have unprecedented sensitivity to dark photon dark matter and current plans to commission a dark photon dark matter search over a wide frequency range. The poster will also describe implications for axion searches and progress toward realizing ultra-high Q cavities under multi-Tesla magnetic fields
Speaker: Raphael Cervantes (University of Washington) -
175
Sensitivity to Decays of Long-Lived Dark Photons at the ILC
Many theories suggest that new particles could have measurably long lifetimes, requiring dedicated search methods not typically used in studies of particles with prompt decays. We present a study on the sensitivity to long-lived dark photon production via dark Higgs decay with the proposed Silicon Detector for the future International Linear Collider (ILC). The ILC is designed to produce a large number of Higgs bosons in an environment cleaner than what is typical of hadron colliders, providing an opportunity to detect low-mass displaced particles and previously unseen Higgs decays to long-lived weakly-interacting particles. This is the first projection for long-lived particle detection at the ILC, and the sensitivity to long-lived dark photons that we have determined can be used as a benchmark for other long-lived searches.
Speaker: Laura Nosler (University of Oregon) -
176
Single photon detectors for dark matter axion searches
Dark matter is the name that we give to the 85% of matter in the universe that interacts via gravity but negligibly with any of the other known forces. One compelling model for dark matter is the axion, as it simultaneously solves the existence of dark matter and the strong CP problem in QCD. Axions may be detectable using haloscopes, which rely on axion-photon coupling in the presence of magnetic field. A major challenge of axion searches at higher frequencies is that the time required becomes increasingly long because of lower signal and increased quantum noise when using a standard haloscope. Building a more sensitive experiment requires eliminating quantum noise, which can be accomplished by detecting single photons. Rydberg atoms are sensitive single photon detectors, and therefore can be used to render the axion search at higher frequencies tractable. This poster presents the progress on the design of the Rydberg atoms for Axions at Yale (RAY) experiment, which aims to find QCD axions at and above 12 GHz.
Speaker: Sumita Ghosh (Yale University) -
177
Space quantum technology and planetary data as probes of dark matter profiles
In this poster, I will present methods using planetary/asteroidal data and space quantum technologies to study fundamental physics.
We first show a proposal using space quantum clocks to study solar-halo ultralight dark matter, motivated by the NASA deep space atomic clock (DSAC) and Parker Solar Probe (PSP).
We then discuss new constraints on fifth forces using asteroidal data. We will show preliminary results of the robust constraints by using the NASA JPL program and asteroid tracking data that are used for planetary defense purposes.
We then discuss model-independent constraints on any dark matter profiles through pure gravity and comment on the implications on cosmic neutrinos.The talk is largely based on https://arxiv.org/abs/2112.07674 and https://arxiv.org/abs/2107.04038, but will also contain completely new results and realistic analysis conducted in collaboration with NASA planetary defense experts.
Speaker: Yu-Dai Tsai (University of California, Irvine) -
178
SQMS axion searches based on $Q_0 \approx 10^{10}$ multimode superconducting cavities
The Physics and Sensing thrust of the Superconducting Quantum Materials and Systems (SQMS) center is developing searches for dark photons, axions and ALPs with the goal of improving upon the current state-of-the-art sensitivity. We are actively working on multiple experiments, including axion haloscopes, DM dark photon searches and light-shining-through-the-wall experiments. All these efforts leverage on Fermilab expertise on ultra-high Q superconducting RF cavities combined with the center research on QIS and quantum technology. This poster focuses on two axion searches that utilize ultra-high Q SRF cavities and their resonant modes to enhance the production and/or detection of axions in the cavity volume. In addition, multi-mode and single mode non-linearity measurements are being carried out as part of an experimental feasibility study to gain insight on the behavior of the ultra-high Q resonators and the RF system in the regime relevant for axion searches.
Speaker: Bianca Giaccone -
179
Stasis in an Expanding Universe: A Recipe for Stable Mixed-Component Cosmological Eras
One signature of an expanding universe is the time-variation of the cosmological abundances of its different components. For example, a radiation-dominated universe inevitably gives way to a matter-dominated universe, and critical moments such as matter-radiation equality are fleeting. In this talk, I shall demonstrate that this lore is not always correct. In particular, I shall show how a form of "stasis" can arise wherein the relative cosmological abundances of the different components remain unchanged over extended cosmological epochs, even as the universe expands. Moreover, I shall also demonstrate that such situations are not fine-tuned, but are in fact global attractors within certain cosmological frameworks, with the universe naturally evolving towards such long-lasting periods of stasis for a wide variety of initial conditions. I shall also discuss some of the implications of a stasis epoch for the evolution of primordial density perturbations and the growth of structure, for dark-matter production, and even for the age of the universe.
Speaker: Brooks Thomas (Lafayette College) -
180
Stau study at the ILC and its implication for the muon g-2 anomaly
Once all the sleptons as well as the Bino are observed at the ILC, the Bino contribution to the muon anomalous magnetic dipole moment (muon $g−2$) in supersymmetric (SUSY) models can be reconstructed. Motivated by the recently confirmed muon $g−2$ anomaly, we examine the reconstruction accuracy at the ILC with $\sqrt{s}$ = 500 GeV. For this purpose, measurements of stau parameters are important. We quantitatively study the determination of the mass and mixing parameters of the staus at the ILC. Furthermore, we discuss the implication of the stau study to the reconstruction of the SUSY contribution to the muon $g−2$. At the benchmark point of our choice, we find that the SUSY contribution to the muon $g−2$ can be determined with a precision of $\sim 1\%$ at the ILC.
Speaker: Dr Shin-ichi Kawada (KEK) -
181
Studies of GaN-based avalanche diodes as a primary cell for a solid-state photomultiplier
Silicon photomultipliers (SiPMs) are now widely used in high-energy physics. They are popular because of their small size, their capability to detect single-photons, their insensitivity to magnetic fields, and their low radioactivity. It is, however, challenging to achieve high photon detection efficiencies in the UV and VUV. A feature very much desired in liquid Argon and Xenon detectors. Achieving good UV sensitivity is an inherent problem with any silicon-based photon detector. Compound III-V semiconductors like GaN or AlGaN, on the other hand, exhibit good UV sensitivity. Also, their spectral response can be tuned to meet the needs of a specific application. Is it thus feasible to build a GaN or AlGaN photon detector that uses the SiPM concept? To find out, we develop GaN and AlGaN photodiodes and test the electrical and optical characteristics of single cells operated in Geigermode. In this poster, I present our structures and their Geigermode characteristics.
Speaker: Nepomuk Otte (Georgia Institute of Technology) -
182
Studies of tau neutrino appearance at the DUNE Near Detector complex
The DUNE experiment will use the new LBNF (Long-Baseline Neutrino Facility) neutrino beam sampled at the Near Detector complex (DUNE ND), 574 m downstream of the production target, and at the Far Detector complex, 1300 km away at the SURF laboratory at a depth of about 1.5 km. The highly capable multi-component Near Detector complex, with a LAr TPC (Liquid Argon Time Projection Chamber) as its primary detector, enables DUNE to probe new physics beyond the Standard Model, including the possibility of short-baseline tau neutrino appearance mediated by sterile neutrino oscillations. Tau neutrino detection is particularly challenging due to the high energy production threshold of the tau lepton and its very short lifetime. However, the excellent spatial resolution of the Near Detector LAr TPC and the large statistics expected (particularly using the high-energy beam configuration) for the LBNF beam provide a unique opportunity to probe these exotic signatures. In this poster, we will present a study of DUNE's projected sensitivities to short-baseline tau neutrino appearance using the DUNE ND and discuss how the sensitivities are enhanced when combining the ND-LAr TPC with downstream components serving as magnetized muon spectrometers, including ND GAr or ND-GAr-Lite, and the SAND detector.
Speaker: Soamasina Herilala Razafinime -
183
Study of Electroweak Phase Transition in Exotic Higgs Decays at the CEPC
A strong first-order electroweak phase transition (SFOEWPT) is expected within BSM scenarios and can be induced by light new particles weakly coupled to the Higgs. At the future Circular Electron Positron Collider (CEPC), 1 million events of Higgs boson associated with a Z boson will be collected in a very clean environment and the sensitivity to probe the SFOEWPT for new scalar masses can be down to ~10GeV. In this poster we will present the search for exotic decays of the Higgs bosons into a pair of spin-zero particles using the simulated e+e- collision data with a luminosity of 5000/fb at sqrt(s)= 240 GeV. The expected sensitivity is significantly better than that can be achieved at the HL-LHC.
Speaker: Ke Li (University of Washington) -
184
Superconducting Nanowire Single Photon Detectors for sub-GeV Dark Matter Detection
Elucidating the fundamental nature of dark matter (DM) is one of the open questions in particle physics today. The growing interest in new sub-GeV DM models has led to many proposals for experiments that can effectively probe this unexplored parameter space. Due to their low energy thresholds and low intrinsic dark count rates, superconducting nanowire single photon detectors (SNSPDs) can be effective in low-mass DM detection.
One novel detector architecture sensitive to MeV-scale DM via electron recoils uses n-type GaAs as a scintillating target and large-area SNSPDs as sensors to read out scintillation photons.
We highlight recent optical excitation experiments on nanogram-scale targets with 1 mm2 SNSPD arrays, and the development of an energy-tagged x-ray excitation source for future characterization experiments. The plan to scale this experiment to larger target volumes is driving the development of SNSPDs with cm2-scale active areas using novel multiplexing techniques and nanofabrication processes.Speaker: Jamie Luskin (Jet Propulsion Laboratory / University of Maryland College Park) -
185
Superconducting Nanowire Single Photon Detectors for sub-GeV Dark Matter Searches
Elucidating the fundamental nature of dark matter (DM) is one of the open questions in particle physics today. The growing interest in new sub-GeV DM models has led to many proposals for experiments that can effectively probe this unexplored parameter space. Due to their low energy thresholds and low intrinsic dark count rates, superconducting nanowire single photon detectors (SNSPDs) can be effective in low-mass DM detection.
One novel detector architecture sensitive to MeV-scale DM via electron recoils uses n-type GaAs as a scintillating target and large-area SNSPDs as sensors to read out scintillation photons.
We highlight recent advances in detector technology including mm2 active areas and scalable nanofabrication using photolithography. We present optical excitation experiments on nanogram-scale targets with 1 mm2 SNSPD arrays, and the development of an energy-tagged x-ray excitation source for future characterization experiments. The plan to scale this experiment to larger target volumes is driving the development of SNSPDs with cm2-scale active areas using novel multiplexing techniques and nanofabrication processes.Speaker: Jamie Luskin (JPL/Caltech/UMD) -
186
Testing Lorentz and CPT symmetries in High Energy Collisions
In this work, we consider the strong sector of the minimal and the non-minimal
Standard Model Extension in order to compute the cross section for Drell Yan and deep inelastic scattering processes. We use this framework to test Lorentz and CPT symmetries with real data, collected at colliders such as LHC and Hera, and simulated data for the future US-based electron-ion collider [1].[1] V. Alan Kostelecký, Enrico Lunghi, Nathan Sherrill, A.R. Vieira, JHEP 04 (2020) 143.
Speaker: Prof. Alexandre Vieira (Universidade Federal do Triângulo Mineiro) -
187
The Cherenkov Telescope Array (CTA): Prospects for Fundamental Physics and Cosmology with Very-High-Energy Gamma Rays
The Cherenkov Telescope Array is designed to improve the sensitivity to 20 GeV – 300 TeV gamma rays by a factor of 5 – 20 compared to current instruments. It will provide the unprecedented capability to probe extreme astrophysical environments, explore fundamental physics, and search for dark matter (DM) signatures. In particular, the CTA DM sensitivity will reach the thermal relic cross-section for DM masses above ~200 GeV, and extend to DM masses above ~1 TeV, which are inaccessible to other existing or upcoming experiments. Observations of extragalactic gamma rays enable tests of Lorentz invariance and measurements of the extragalactic background light, cosmological parameters, intergalactic magnetic fields, axion-like particles, and primordial black holes. CTA is an international project that has profited from strong U.S. participation in technology development in the form of a novel dual-mirror Schwarzschild-Couder Telescope and in science planning. The U.S. support for CTA construction, if provided, will enhance the science reach of the observatory and ensure U.S. access to this transformational facility and the discoveries it will enable.
Speaker: Qi Feng (SAO) -
188
The Cosmic-Ray Positron Excess: Status of the Pulsar Explanation
Pulsars - spinning neutron stars that are magnetized – are likely the leading source which could explain the large excess in the observed positron flux present in data measurements from the AMS-01, HEAT, and PAMELA collaborations. While first thought to be from a source of annihilating dark matter, there have since been more compelling observations - via experiments such as HAWC - of TeV halos associated with pulsars especially young ones within a few kiloparsecs of Earth. These halos indicate that such pulsars inject significant fluxes of very high-energy electron-positrons pairs into the interstellar medium (ISM), thereby likely providing the dominant contribution to the cosmic-ray positron flux. This poster highlights the important updates on the constraints of local pulsar populations which further support the pulsar explanation to resolving the positron excess, through building upon previous work done by Hooper, Linden, and collaborators. Using the cosmic-ray positron fraction as measured by the AMS-02 Collaboration and applying reasonable model parameters, a good agreement can be obtained with the measured positron fraction up to energies of roughly ∼ 300 GeV. At higher energies, the positron fraction is dominated by a small number of pulsars, making it difficult to reliably predict the shape of the expected positron fraction. The low-energy positron spectrum supports the conclusion that pulsars typically transfer approximately ∼ 5 − 20% of their total spindown power in efficiency into the production of very high-energy electron-positron pairs, producing a spectrum of such particles with a hard spectral index of ∼ 1.5 − 1.7. Such pulsars typically spindown on a timescale on the order of ten thousand years. The best fits were obtained for models in which the radio and gamma-ray beams from pulsars are detectable to 28% and 62% of surrounding observers, respectively.
Speaker: Olivia Bitter (Fermilab/UChicago) -
189
The Deep Junction LGAD: Concept and Progess
Achieving granularity below the 1 mm scale while maintaining high efficiency, precise timing, and good spatial resolution is a goal of continued R&D on silicon diode Low Gain Avalanche Detectors (LGAD). The deep junction LGAD (DJ-LGAD) approach, proposed by the SCIPP ultrafast sensor R&D group, is to make use of the diode junction to create avalanche-generating fields within the sensor, and then to bury the junction underneath several microns of n+ material to keep surface fields low, and allow for conventional pixelization techniques. In this talk, we will present updates relating to the DJ-LGAD design and fabrication.
Speaker: Yuzhan Zhao (University of California, Santa Cruz, SCIPP) -
190
The LUX-ZEPLIN (LZ) Experiment: Searching for direct evidence of dark matter
Astronomical observations have indicated a considerable amount of dark matter in our universe, but nobody has been able to directly observe any dark matter yet. LZ is an experiment looking for dark matter particles, in particular Weakly Interacting Massive Particles (WIMPs) among other candidates. LZ is located at the Sanford Underground Research Facility in Lead, South Dakota, and it uses a dual-phase time projection chamber containing 7 tonnes of liquid xenon and 5.6-tonne fiducial mass, aided by an LXe "skin" detector and liquid scintillator-based outer detector to veto events inconsistent with dark matter. In this poster, we will give an overview of the LZ experiment.
Speaker: Yue Wang (UC Berkeley) -
191
The Snowball Chamber: Supercooled Water for Dark Matter, Neutrinos, and General Particle Detection
The snowball chamber is analogous to the bubble and cloud chambers in that it relies on a phase transition, but it is new to high-energy particle physics. The concept of the snowball chamber relies on supercooled water (or a noble element, for scintillation for energy reconstruction), which can remain metastable for long time periods in a sufficiently clean and smooth container (on the level of the critical radius for nucleation). The results gleaned from the first prototype setup (20 grams) will be reviewed, as well as plans for the future, with an eye to future deployment of a larger (kg-scale) device underground for direct detection of dark matter WIMPs, with a special focus on low-mass (GeV-scale) WIMPs, capitalizing on the presence of H, which could potentially also lead to world-leading sensitivity to spin-dependent-proton interactions for O(1 GeV/c^2)-mass WIMPs and CEvNS. Supercooled water also has the potential advantage of a sub-keV energy threshold for nuclear recoils, but this remains an atmospheric chemistry prediction that must be verified by careful measurements.
Speaker: Prof. Matthew Szydagis (UAlbany SUNY) -
192
The Southern Wide-field Gamma-Ray Observatory (SWGO)
The Southern Wide-field Gamma-ray Observatory (SWGO) Collaboration is currently engaged in design and prototyping work towards the realization of this future gamma-ray facility in the Southern Hemisphere. SWGO be a next-generation, wide-field-of-view, survey instrument sensitive to gamma rays from ~100 GeV to hundreds of TeV. Its science topics are numerous and diverse, including probing physics beyond the Standard Model, monitoring the transient sky at very-high energies, unveiling Galactic and extragalactic particle accelerators, and the characterization of the cosmic-ray flux. Due to its location and large field of view, SWGO will be complementary to other current and planned gamma-ray observatories such as HAWC, LHAASO, and CTA.
Speaker: Kristi Engel (University of Maryland, College Park) -
193
The Trinity UHE Neutrino Observatory
The detection of astrophysical neutrinos with IceCube has renewed the interest in opening the neutrino window at even higher energies. Trinity is a proposed system of air-shower imaging telescopes to detect Earth-skimming tau neutrinos. The observatory will have 18 novel wide field-of-view telescopes distributed at three different sites on mountain tops in its final configuration. With its high sensitivity between PeV and 10 EeV, Trinity will fill the gap between IceCube and proposed radio UHE-neutrino instruments. In this poster, I discuss Trinity's concept, design, and sensitivity to diffuse and point sources, highlighting synergies with future radio and in-ice optical observatories. I will close by discussing the Trinity demonstrator we are constructing and planning to deploy in Fall 2022 on Frisco Peak, Utah.
Speaker: Nepomuk Otte (Georgia Institute of Technology) -
194
Toward CUPID-1T
Current experiments to search for broken lepton-number symmetry through the observation of neutrinoless double-beta decay ($0\nu\beta\beta$) provide the most stringent limits on the Majorana nature of neutrinos and the effective Majorana neutrino mass ($m_\beta\beta$). The next-generation experiments will focus on sensitivity to the $0\nu\beta\beta$ half-life of $\mathcal{O}(10^{27}-10^{28}$years$)$ and $m_{\beta\beta}{\sim}15$meV, which would provide complete coverage of the so-called Inverted Ordering region of the neutrino mass parameter space.
With reasonably achievable advancements in sensor technology and background reduction, new, future calorimetric experiments at the 1-ton scale can increase the sensitivity by at least another order of magnitude, exploring the large fraction of the parameter space that corresponds to the neutrino mass Normal Ordering. In addition, a detector of such magnitude would also be sensitive to a number of interesting particle physics searches: this poster will also discuss searches for solar and supernova neutrinos, light dark matter and new scalar bosons, and tests of symmetry.Speaker: Danielle Speller (Johns Hopkins University) -
195
Towards an Interpretable Data-driven Trigger System for High-throughput Physics Facilities
Data-intensive science is increasingly reliant on real-time processing capabilities and machine learning workflows, in order to filter and analyze the extreme volume and complexity of the data being collected. This is especially true at the energy and intensity frontiers of particle physics, for physics facilities such as the Large Hadron Collider (LHC).
The sophisticated trigger systems at the LHC are crucial for selecting relevant physics processes. However, the design, implementation, and usage of the trigger algorithms are resource-intensive and can include significant blind spots. The configuration of the trigger algorithms is manually designed based on domain knowledge (involving $\sim100$ data filters).
We propose a new data-driven approach for designing and optimizing high-throughput data filtering and trigger systems at the LHC. The main purpose is to replace the current hand-designed trigger system with a data-driven trigger system with a minimal run-time cost, to account for non-local inefficiencies in the existing trigger menu and construct a cost-effective data filtering and trigger model that does not compromise physics coverage. This approach involves novel machine learning algorithms that are cost-effective, interpretable, tailored to (sequential) optimization, and can be implemented efficiently in hardware. An early demonstration of this approach is currently being prototyped using the Xilinx Versal ACAP (adaptive compute acceleration platform) board.
This model will be ideally used to expand to a self-driving and continuous learning triggering system, based on novel active learning algorithms for exploring new phenomena and inferring the underlying physics.Speaker: Cecilia Tosciri (University of Chicago) -
196
Transforming U.S. Particle Physics Education
The pursuit of knowledge in particle physics requires constant learning. As new tools become available, new theories are developed, and physicists search for new answers with ever-evolving methods. However, it is the case that formal educational systems serve as the primary training grounds for particle physicists. Graduate school (and undergraduate school to a lesser extent) is where researchers learn most of the technical skills required for research, develop scientific problem-solving abilities, learn how to establish themselves in their field, and begin developing their career. It is unfortunate, then, that the skills gained by physicists during their formal education are often mismatched with the skills actually required for a successful career in physics. We performed a survey of the U.S. particle physics community to determine the missing elements of graduate and undergraduate education and to gauge how to bridge these gaps. Our poster will present the results of this survey. We also recommend several specific community actions to improve the quality of particle physics education; the "community" here refers to physics departments, national labs, professional societies, funding agencies, and individual physicists.
Speaker: Vetri Velan (University of California, Berkeley) -
197
U.S. Participation in the next-generation gamma-ray facility, the Cherenkov Telescope Array Observatory
The Cherenkov Telescope Array Observatory (CTAO) will be the major next-generation facility for observations of very high-energy (VHE) gamma-ray sources, having sensitivity for energies 20 GeV - 300 TeV. Funding has now been secured and construction is beginning for the "Alpha Configuration," consisting of observatories in the Atacama Desert (Chile) in the southern hemisphere and at La Palma (Spain) in the north. The Alpha Configuration will achieve sensitivity as much as an order of magnitude better than existing instruments. The Astro2020 Decadal Survey has recommended U.S. participation in CTAO as part of the Multi-Messenger Program for the 2020s, and in particular recommends support for the addition of ten Schwarzschild-Couder Telescopes (SCTs), which would be an enhancement to the southern array. An international consortium of CTA members, led by the U.S., has developed and prototyped the 9.7-m-aperture SCT, which uses a novel design incorporating a secondary mirror to achieve superior performance over the core 100 GeV - 10 TeV energy region of CTAO. CTAO will be the first open observatory in the VHE band, accepting proposals from and executing observations for any scientist from a country contributing financially to its construction and operation; U.S. participation in CTAO would unlock this access for all scientists based in the U.S. This presentation will survey the design and science capabilities of CTAO, as well as how these would be augmented with the addition of Schwarzschild-Couder Telescopes to the array.
Speaker: Lab Saha (Center for Astrophysics, Harvard and Smithsonian) -
198
Updated Results from HAYSTAC's Quantum-Enhanced Search for Dark Matter Axions
The HAYSTAC Collaboration is currently searching for axion cold dark matter with the use of a resonant microwave cavity. Because both the mass of the axion and its coupling strength are largely unknown, a key figure of merit for a haloscope is the rate at which it can scan this vast parameter space. Recent progress in developing squeezed state receivers have allowed HAYSTAC to reduce noise levels below the standard quantum limit, resulting in a factor of two scan rate enhancement as first demonstrated in the search over the combined axion mass window of 16.96-17.12$\mu$eV and 17.14-17.28 $\mu$eV. This quantum enhanced search was continued between July and September 2021, extending the scanned region to axions with masses between 18.45-18.69$\mu$eV. Here I will show the status of HAYSTAC with emphasis on the most recent data taking phase that includes improvements to the data acquisition routine which have reduced dead time by a factor of two, further improving the scan rate of the experiment.
Speaker: Michael Jewell (Yale) -
199
A3D3 Postbaccalaureate Fellowship Program
The Accelerated AI Algorithms for Data-Driven Discovery (A3D3) Institute funded by the National Science Foundation (NSF), under the Harnessing the Data Revolution (HDR) program, recently launched a postbaccalaureate research fellowship this year aimed to increase participation in research from traditionally underrepresented groups in STEM, such as African American/Black, Chicano/Latino, Native American/Alaska Native, Native Hawaiin/Pacific Islander, and Filipino students.
A3D3 is a multi-disciplinary and geographically distributed entity with the primary mission to lead a paradigm shift in the application of real-time artificial intelligence (AI) at scale to advance scientific knowledge and accelerate discovery in particle physics, astrophysics, biology, and neuroscience. The Institute team reflects a collaborative effort of Principal Investigators from Caltech, Duke University, MIT, Purdue University, University of California San Diego, University of Illinois at Urbana-Champaign, University of Minnesota, University of Washington, and University of Wisconsin-Madison.
We will describe the A3D3 postbac program, including its goals, structure, advertisement, application process, selection process (including equity, diversity, and inclusion considerations), planned professional development activities, and future improvements. While the program is just starting, we hope to share our experiences with the community to enable others to create similar programs.
Speaker: Javier Duarte (University of California San Diego)
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Social: Reception & Poster Session 211 South Ballroom (HUB)
211 South Ballroom
HUB
https://washington.zoom.us/j/98883066364?pwd=UjVOajdLMFpMQWVibUtsR010T1AzUT09
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Accelerator Frontier: AF6 and AF1 Internal (TBD) 238 (MGH)
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19EConveners: Cameron Geddes (LBNL), Zhirong Huang (SLAC National Accelerator Laboratory) -
Accelerator Frontier: Several AFx Internal (ARDAP, Intl R&D) 254 (MGH)
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19FConveners: Frank Zimmermann (CERN), Mark Palmer (Brookhaven National Laboratory), Tor Raubenheimer (SLAC)- 200
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High Energy & High Luminosity CollidersSpeaker: Emanuela Barzi (Fermilab)
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Community Engagement Frontier: Frontier Discussion 231 (MGH)
231
MGH
21D- 205
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Discussion about the CEF plenary
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Feedback on TG Reports
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Feedback on Frontier Report
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Computational Frontier: CompF3 Machine Learning (20F) 238 (HUB)
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HUB
20F-
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IntroductionSpeakers: Daniel Whiteson (UC Irvine), Kazuhiro Terao (SLAC National Accelerator Laboratory), Phiala Shanahan (Massachusetts Institute of Technology)
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First-principles theory calculations and detector simulationsSpeakers: Ian Moult (MIT), Ian Moult (Lawrence Berkeley Laboratory)
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Data analysisSpeaker: Javier Duarte (University of California San Diego)
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Detector and Accelerator Design and OperationsSpeaker: Auralee Edelen (SLAC)
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Community Tools, Standards, Resources and Management.Speaker: Philip Harris (MIT)
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Discussion
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Cosmic Frontier: CF5 Discussion 337 (HUB)
337
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18HConveners: Clarence Chang (Argonne National Lab), Deirdre Shoemaker (University of Texas at Austin), Laura Newburgh (Yale University) -
Cross frontier sessions: Dark Matter Complementarity (CF-EF-RF-TF CF1 CF2 CF3 CF7) 220 (Kane Hall)
220
Kane Hall
20LA panel during the 22j session discussing the intersections of the AF and EF frontiers
Conveners: Caterina Doglioni (Lund University), Flip Tanedo (UC Riversider), Natalia Toro (SLAC National Accelerator Laboratory), Stefania Gori (UC Santa Cruz)-
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IntroductionSpeakers: Caterina Doglioni (Lund University), Flip Tanedo (UC Riversider), Natalia Toro (SLAC National Accelerator Laboratory), Stefania Gori (UC Santa Cruz)
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Light DM from Rare Processes & Precision FrontierSpeaker: Natalia Toro (SLAC National Accelerator Laboratory)
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Particle DM from Cosmic FrontierSpeakers: Bjoern Penning (University of Michigan), Hugh Lippincott (UCSB)
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DM in cosmic probes from Cosmic FrontierSpeakers: Alex Drlica-Wagner (Fermilab), HAI-BO YU (UNIVERSITY OF CALIFORNIA, RIVERSIDE)
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Particle DM from Energy FrontierSpeaker: Suchita Kulkarni
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10:05
Coffee break
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Dark Matter perspective from the Theory FrontierSpeaker: Julia (Jessie) Shelton (Harvard Physics)
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Introduction to panelSpeaker: Caterina Doglioni (Lund University)
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Panel discussion
Discussion of topics and questions submitted prior to the session, can be found in this google document
Speakers: Alex Drlica-Wagner (Fermilab), Doojin Kim (University of Arizona), HAI-BO YU (UNIVERSITY OF CALIFORNIA, RIVERSIDE), Hugh Lippincott (UCSB), Julia (Jessie) Shelton (Harvard Physics), Lindley Winslow (MIT), Natalia Toro (SLAC National Accelerator Laboratory), Suchita Kulkarni, Suchita Kulkarni, Susan Gardner (U Kentucky)
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Cross frontier sessions: TF-EF Energy Frontier Theory 175 (JHN)
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JHN
19JA panel during the 22j session discussing the intersections of the AF and EF frontiers
Conveners: Ayres Freitas (University of Pittsburgh), Ethan Neil (University of Colorado, Boulder), Jesse Thaler (MIT), Laura Reina (Florida State University), Nathaniel Craig (UC Santa Barbara), Radja Boughezal (Argonne National Laboratory), Shufang Su (University of Arizona), Zhen Liu (University of Minnesota)-
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Where are we going? (panel discussion)
Direction to explore BSM physics.
What are the Dream/Nightmare cases for new physics, and what is the need for Energy Frontier machines?
Questions from the audience.Speakers: Jesse Thaler (MIT), Laura Reina (Florida State University), Michelangelo Mangano (CERN), Tao Han (University of Pittsburgh) -
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Novel observables and new ideas for possible explorationsSpeakers: Doojin Kim (University of Arizona), Joshua Isaacson, Tilman Plehn (University of Heidelberg)
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a) Kinematic Variables and Feature Engineering for Particle PhenomenologySpeaker: Doojin Kim (University of Arizona)
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c) Machine Learning for LHC SimulationsSpeaker: Tilman Plehn (University of Heidelberg)
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d) Discussion
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10:10
Coffee Break
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Precision physics for future collidersSpeakers: Andreas Kronfeld (Fermilab), Gherardo Vita (SLAC), Huey-Wen Lin (MSU), Samuel Abreu (UCLouvain)
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a) Precision calculation for e+e- colliders: future directionsSpeaker: Samuel Abreu (UCLouvain)
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b) Precision calculations for hadron colliders: future directionsSpeaker: Gherardo Vita (SLAC)
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c) Lattice for precision studies at the energy frontier
(alphas, mb, ...)
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d) Lattice for precision studies at the energy frontier
PDF
Speaker: Huey-Wen Lin (MSU) -
e) Discussion
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Instrumentation Frontier: IF10 242 (MGH)
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23EConveners: Prof. Albrecht Karle (University of Wisconsin/WIPAC), Amy Connolly (OSU)-
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IntroductionSpeaker: Prof. Albrecht Karle (University of Wisconsin/WIPAC)
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Radio detection of neutrinos using ice as target, and detectors in iceSpeaker: Dr Brian Clark (Michigan State University )
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Radio instrumentation for neutrino detectors using iceSpeaker: Dr Cosmin Deaconu (University of Chicago/KICP)
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Radar detection of neutrinos in the iceSpeaker: Prof. Steven Prohira (University of Kansas)
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Air shower detection of earth-skimming neutrinosSpeaker: Prof. Nepomuk Otte
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Coffee break
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KID detectors
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Radio air shower detectionSpeaker: Prof. Sijbrand de Jong (Radboud University)
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IceCube UpgradeSpeaker: Dr Mike DuVernois (University of Wisconsin/WIPAC)
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IceCube-Gen2 Optical, techical with km3net and P1 in contextSpeaker: Prof. Carsten Rott (University of Utah)
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Panel, round tableSpeaker: Prof. Albrecht Karle (University of Wisconsin/WIPAC)
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Instrumentation Frontier: IF3 288 (MGH)
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23FConveners: Artur Apresyan (Fermilab), Steven Worm, Tony Affolder (UCSC- SCIPP)-
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IntroductionSpeakers: Artur Apresyan (Fermilab), Steven Worm, Tony Affolder (UCSC- SCIPP)
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4D-tracking detectorsSpeaker: Ariel Schwartzman (SLAC National Accelerator Laboratory)
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3D integrationSpeaker: Simone Mazza (UC Santa Cruz)
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Coffee Break
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248
Discussion and IF03 recommendations
-
241
-
Instrumentation Frontier: IF4 284 (MGH)
284
MGH
30VConveners: Allison Deiana, Darin Acosta (Rice University), Wesley Ketchum (Fermi National Accelerator Laboratory)-
249
IntroductionSpeakers: Allison Deiana, Darin Acosta (Rice University), Wesley Ketchum (Fermi National Accelerator Laboratory)
-
250
Readout TechnologiesSpeaker: Alexander Paramonov (Argonne National Laboratory)
-
251
Innovations in TDAQSpeakers: Catrin Bernius (SLAC National Accelerator Laboratory (US)), David Miller (University of Chicago), Rainer Bartoldus (SLAC)
-
09:10
Break
-
252
Perspective and outlook for hardware-based track triggersSpeaker: Kristian Hahn (Northwestern Univ.)
-
253
A fast method for particle trackingSpeaker: Ashutosh Kotwal (Duke University)
-
254
Track-Based Triggers for Exotic SignaturesSpeaker: Tova Holmes (University of Tennessee)
-
255
Discussion
- 256
-
257
Fast ML and Anomaly Driven Trigger Discussion
-
258
Guided discussion on TDAQ needs
-
249
-
Instrumentation Frontier: IF6 248 (MGH)
248
MGH
23CConveners: Andy White (U. texas at Arlington), Minfang Yeh (Brookhaven National Laboratory), Rachel Yohay (Florida State University)-
259
Recap of the process (Calorimetry talks, LOIs, White Papers, Summary)
The IF06 session will consist of a short introductory talk followed by a discussion period - for each of the four main calorimetry subject areas (Precise Timing, Dual-Readout, Particle Flow, and Materials)
Speakers: Andy White (U. texas at Arlington), Minfang Yeh (Brookhaven National Laboratory), Rachel Yohay (Florida State University) -
260
Precise timing
Summary of main points/highlights from WP/Summary
Critical issues, challenges, questions (10 min)
followed by discussion.Speaker: Frank Simon (Max-Planck-Institute for Physics) -
261
Particle Flow
Summary of main points/highlights from WP/Summary
Critical issues, challenges, questions (10min) Katja Kruger
"High granularity MAPS ECal" Jim Brau
followed by discussion.Speakers: James Brau (Univ. of Oregon), Dr Katja Kruger (DESY) -
262
Break
-
263
Dual-Readout
Summary of main points/highlights from WP/Summary
Critical issues, challenges, questions (10 min)
followed by discussionSpeaker: Sarah Eno (U. Maryland) -
264
Materials for Calorimetry
Summary of main points/highlights from WP/Summary
Critical issues, challenges, questions
followed by discussionSpeaker: Renyuan Zhu (Caltech) -
265
General discussionSpeakers: Andy White (U. texas at Arlington), Minfang Yeh (Brookhaven National Laboratory), Rachel Yohay (Florida State University)
-
259
-
Neutrino Physics Frontier: DUNE P5 Strategy (Oscillation Physics) 120 (Kane Hall)
120
Kane Hall
20NConvener: Elizabeth Worcester (BNL)-
266
DUNE Oscillation AnalysisSpeakers: Callum Wilkinson, Callum Wilkinson (Lawrence Berkeley National Laboratory)
-
267
Neutrino Interactions and the DUNE Oscillation AnalysisSpeaker: Kevin McFarland (University of Rochester)
- 268
-
269
Oscillation Physics Global ContextSpeaker: Sanjib Kumar Agarwalla (Institute of Physics, Bhubaneswar)
-
09:52
Coffee Break
-
266
-
Rare Processes and Precision Frontier: RF1 Discussions 111 (JHN)
111
JHN
20C-
270
Weak decays of b and c quarks: summarySpeakers: Angelo Di Canto (BNL), Stefan Meinel (University of Arizona)
-
271
Discussion
-
270
-
Underground Facilities Frontier: UF2 - Underground Facilities for Cosmic Frontier 307 (HUB)
307
HUB
19BConvener: Scott Hertel (UMass Amherst)-
272
UF2 TopicalSpeaker: Scott Hertel (UMass Amherst)
-
272
-
Cosmic Frontier: CF6 Discussion 337 (HUB)
337
HUB
18OConveners: Brenna Flaugher (Fermilab), David Schlegel (Lawrence Berkeley National Lab), Vivian Miranda (Stony Brook University) -
Accelerator Frontier: AF3 307 (HUB)
307
HUB
37B -
Computational Frontier: CompF4 Storage and Processing Resource Areas 238 (HUB)
238
HUB
20UConveners: Wahid Bhimji (NERSC, Berkeley Lab), Dr Meifeng Lin (Brookhaven National Laboratory), Frank Wuerthwein (UCSD)-
273
IntroductionSpeakers: Meifeng Lin (BNL), Wahid Bhimji (NERSC, Berkeley Lab)
- 274
-
275
AI hardwareSpeakers: Javier Duarte (University of California San Diego), Nhan Tran (FNAL)
-
276
StorageSpeakers: Bo Jayatilaka (Fermilab), Carlos Maltzahn, Peter van Gemmeren (ANL)
-
277
Analysis FacilitiesSpeakers: Gordon Watts (University of Washington), Mark Neubauer (University of Illinois Urbana-Champaign), Oksana Shadura (University of Nebraska Lincoln (US))
- 278
-
279
NetworkingSpeakers: Chin Guok (ESnet), Eli Dart (ESnet / LBNL), Shawn McKee (Univ. of Michigan)
-
280
Overall Findings and RecommendationsSpeakers: Meifeng Lin (BNL), Wahid Bhimji (NERSC, Berkeley Lab)
-
281
Discussion
-
273
-
Cosmic Frontier: CF7 Discussion 337 (HUB)
337
HUB
18RConveners: Bangalore Sathyaprakash (Penn State University), Ke Fang (University of Wisconsin-Madison), Kirsten Tollefson (Michigan State University), Kristi Engel (University of Maryland, College Park), Luis Anchordoqui (City University of New York, Lehman College), Rana Adhikari (Caltech), Tiffany Lewis (NASA Goddard) -
Cross frontier sessions: UF-NF-RF Facilities for measurements of 0nbb and neutrinos from natural sources 241 (MGH)
241
MGH
19AA panel during the 22j session discussing the intersections of the AF and EF frontiers
Convener: Jeter Hall (SNOLAB)-
282
Ton-Scale 0nBB Overvew & Future LS ExperimentsSpeaker: Joshua Klein (University of Pennsylvania)
-
283
Beyond Ton Scale 0nBB and Future Xe ExperimentsSpeaker: Richard Saldanha (Pacific Northwest National Laboratory)
-
284
Future Natural-Source Neutrino ExperimentsSpeaker: Zara Bagdasarian (University of California Berkeley)
-
285
Future Bolometer ExperimentsSpeaker: Karsten Heeger (Yale University)
-
286
Panel DiscussionSpeakers: Jeter Hall (SNOLAB), Joshua Klein (University of Pennsylvania), Karsten Heeger (Yale University), Patrick Decowski (Nikhef / University of Amsterdam), Richard Saldanha (Pacific Northwest National Laboratory), Zara Bagdasarian (University of California Berkeley)
-
282
-
Neutrino Physics Frontier: DUNE P5 Strategy (Low Energy and BSM Physics) 120 (Kane Hall)
120
Kane Hall
20XConvener: Patrick Huber (Virginia Tech)-
10:00
Coffee Break
- 287
-
288
BSM Context and MotivationSpeaker: Pilar Coloma (Instituto de Fisica Teorica UAM/CSIC)
-
289
Beyond 3-Flavor Oscillations in DUNESpeaker: Alexandre Sousa (University of Cincinnati)
-
290
Direct BSM Detection in DUNESpeakers: Jaehoon Yu (University of Texas at Arlington), Jaehoon Yu
-
10:00
-
Rare Processes and Precision Frontier: RF2 Discussions 111 (JHN)
111
JHN
20S-
291
Prospects in kaon decay physics
(remote)
Speaker: Hajime Nanjo (Osaka University) -
292
Prospects in charged pion decay physics
(in person)
Speaker: David Hertzog (University of Washington) -
293
Prospects on theory inputs for the first-row CKM unitarity tests
(remote)
Speaker: Chien Yeah Seng (HISKP, Universität Bonn) -
294
Lattice QCD input for the first-row CKM unitarity tests
(in person)
Speaker: Luchang Jin (BNL) -
295
Prospects in eta decays at JEFSpeaker: Liping Gan (University North Carolina Wilmington)
-
296
Studying eta decays at REDTOP
(in person)
Speaker: Corrado Gatto (INFN and Northern Illinois University)
-
291
-
Cosmic Frontier: CF4 CF5 CF6 CF7 Dark Energy Complementarity 337 (HUB)
337
HUB
20W -
US funding Agency Meetings: FOA/DOE General Meeting 120 (Kane Hall)
120
Kane Hall
36A-
297
Perspective from DOE - upcoming FOA'sSpeaker: William Kilgore (U.S. Department of Energy)
-
297
-
Afternoon Plenary: Panel: Careers and Training the Next Generations 130 (Kane Hall)
130
Kane Hall
19SConveners: Petra Merkel (Fermi National Accelerator Laboratory), Sridhara Dasu (University of Wisconsin), Steven Lund (USPAS / MSU / FRIB)-
298
Obstacles and Solutions to Careers in HEPSpeaker: Sudhir Malik (University of Puerto Rico Mayaguez)
-
299
Careers and training in accelerator physicsSpeaker: Steven Lund (USPAS / MSU / FRIB)
-
300
Career and Training Panel DiscussionSpeakers: Farah Fahim (FERMILAB), Giordon Stark, Jeremy Love (Department of Energy), Rachel Yohay (Florida State University), Robert Bernstein (Fermilab), Steven Lund (USPAS / MSU / FRIB), Tim Tait (UC Irvine)
-
298
-
Afternoon Plenary: Cosmic Frontier: Paths to Discovery 120 (Kane Hall)
120
Kane Hall
30WConveners: Aaron Chou (Fermi National Accelerator Laboratory), Marcelle Soares-Santos (Fermilab), Tim Tait (UC Irvine)- 301
-
302
The Path to Dark Energy and Cosmic AccelerationSpeaker: Prof. Kyle Dawson (University of Utah)
-
303
The Path to Cosmic Probes of Dark MatterSpeaker: Prof. Risa Wechsler (Stanford / SLAC)
-
Afternoon Plenary: Energy Frontier: Lepton Colliders 130 (Kane Hall)
130
Kane Hall
30DConveners: Alessandro Tricoli (BNL), Laura Reina (Florida State University), Meenakshi Narain (Brown University), Steve Gourlay (LBNL), Tor Raubenheimer (SLAC), Vladimir Shiltsev (FNAL)- 304
-
305
Lepton colliders - e+e- Collider Forum presentationSpeaker: Sridhara Dasu (University of Wisconsin)
-
306
Lepton Coliders - mu+mu- Colider Forum presentationSpeaker: Diktys Stratakis (Fermi National Accelerator Laboratory)
-
307
Questions and discussionSpeakers: Derun Li (LBNL), Diktys Stratakis (Fermi National Accelerator Laboratory), Emilio Nanni (SLAC National Accelerator Laboratory), Fabio Maltoni, Fabio Maltoni (Universite' catholique de Louvain), John Power (Argonne National Lab), Kevin Black, Maria Chamizo Llatas (Brookhaven National Laboratory), Patrick Meade (Stony Brook), Sergo Jindariani (FNAL), Sridhara Dasu (University of Wisconsin), Stefan Wagner (CBPF), Stephen Wagner (University of Colorado, Boulder), Ulrich Heintz (Brown University)
-
17:00
Coffee 225 and Lobby (Kane Hall)
225 and Lobby
Kane Hall
-
Afternoon Plenary: HEP Community Engagement: Is the HEP Community going to take responsibility for Engagement (or not)? 130 (Kane Hall)
130
Kane Hall
19VConveners: Breese Quinn (University of Mississippi), Ketevi Adikle Assamagan (Brookhaven National Laboratory)-
308
Community Engagement Frontier IntroductionSpeaker: Ketevi Adikle Assamagan (Brookhaven National Laboratory)
-
309
Selected Key CEF Recommendations (49 min: ~7 min per Topical Group)
-
a) Community marginalization and need improvement (CEF03)Speaker: Mu-Chun Chen (University of California, Irvine)
-
b) Empowering marginalized communities through education (CEF04)Speaker: Sudhir Malik (University of Puerto Rico Mayaguez)
-
c) Structural changes for effective engagements toward marginalized communities (CEF05)Speaker: Donald Lincoln (Fermilab)
-
d) DEI impact on career pipelines, development and retention (CEF02)Speaker: Julie Hogan (Bethel University)
-
e) DEI in HEP-industry dynamics (CEF01)Speaker: Farah Fahim (FERMILAB)
-
f) Policy implementations to improve DEI (CEF06)Speaker: Louise Suter (FNAL)
-
g) DEI and Societal and environmental impactsSpeaker: Ken Bloom (University of Nebraska-Lincoln)
-
-
310
Options for Implementing CEF RecommendationsSpeaker: Breese Quinn (University of Mississippi)
-
311
Questions and discussion
A panel will consist of all speakers
Speakers: Breese Quinn (University of Mississippi), Ketevi Adikle Assamagan (Brookhaven National Laboratory)
-
308
-
Social: Industry Networking 211 South Ballroom (HUB)
211 South Ballroom
HUB
https://washington.zoom.us/j/98883066364?pwd=UjVOajdLMFpMQWVibUtsR010T1AzUT09
Conveners: Amber Roepe, Jan Strube (PNNL), Jan Strube (Pacific Northwest National Laboratory), Karri DiPetrillo (Fermilab), Tova Holmes (University of Tennessee)
-
-
-
Accelerator Frontier: AF6 Report (2 hrs) and AF-Summary-I (2 hrs) 102 (JHN)
102
JHN
19CConveners: Cameron Geddes (LBNL), Mark Hogan (SLAC), Pietro Musumeci (UCLA), Steve Gourlay (LBNL), Tor Raubenheimer (SLAC), Vladimir Shiltsev (FNAL) -
Computational Frontier: CompF1 Experimental Algorithm Parallelization 248 (MGH)
248
MGH
20E-
312
Portability: A Necessary Approach for Future Scientific SoftwareSpeaker: Meghna Bhattacharya
-
313
Future architectures and challenges for experimental algorithmsSpeaker: Salman Habib (Argonne National Laboratory)
-
314
Overview of CompF1 reportSpeakers: Giuseppe Cerati (Fermi National Accelerator Laboratory), Giuseppe Cerati (Fermilab), Katrin Heitmann (Argonne National Laboratory), Walter Hopkins (Argonne National Laboratory)
-
08:45
Coffee
-
315
Discussion of the Report and Recommendations
-
316
Summary of report enhancementsSpeakers: Giuseppe Cerati (Fermi National Accelerator Laboratory), Giuseppe Cerati (Fermilab), Katrin Heitmann (Argonne National Laboratory), Walter Hopkins (Argonne National Laboratory)
-
312
-
Cosmic Frontier: Report Discussion 120 (Kane Hall)
120
Kane Hall
23Q-
317
CF1 Report DiscussionSpeakers: Hugh Lippincott (UCSB), Jodi Cooley (SMU), Tien-Tien Yu (University of Oregon), Tracy Slatyer (MIT)
-
318
CF2 Report DiscussionSpeakers: Gray Rybka (University of Washington), Joerg Jaeckel, Lindley Winslow (MIT)
-
319
CF3 Report DiscussionSpeakers: Alex Drlica-Wagner (Fermilab), Chanda Prescod-Weinstein (University of New Hampshire), HAI-BO YU (UNIVERSITY OF CALIFORNIA, RIVERSIDE)
-
09:30
Coffee / Informal Discussion
-
320
CF4 Report DiscussionSpeakers: Anze Slosar (BNL), James Annis (Fermilab), Jeffrey Newman (University of Pittsburgh and PITT-PACC)
-
321
CF5 Report DiscussionSpeakers: Clarence Chang (Argonne National Lab), Deirdre Shoemaker (University of Texas at Austin), Laura Newburgh (Yale University)
-
322
CF6 Report DiscussionSpeakers: Brenna Flaugher (Fermilab), David Schlegel (Lawrence Berkeley National Lab), Vivian Miranda (Stony Brook University)
-
323
CF7 Report DiscussionSpeakers: Bangalore Sathyaprakash (Penn State University), Ke Fang (University of Wisconsin-Madison), Kirsten Tollefson (Michigan State University), Kristi Engel (University of Maryland, College Park), Luis Anchordoqui (City University of New York, Lehman College), Rana Adhikari (Caltech), Tiffany Lewis (NASA Goddard)
-
317
-
Cross frontier sessions: AF-NF AF2-AF5-NF9 Booster Replacement Options 231 (MGH)
231
MGH
30EA panel during the 22j session discussing the intersections of the AF and EF frontiers
Conveners: Alysia Marino (University of Colorado), J. Pedro Ochoa (University of California at Irvine), Laura Fields (Fermilab)-
324
Introduction to Booster Replacement SessionSpeaker: Alysia Marino (University of Colorado)
-
325
Summary of Wolrdwide CapabilitiesSpeaker: Robert Zwaska (Fermilab)
- 326
- 327
-
328
Cost Effective Upgrade AproachSpeaker: Sergei Nagaitsev (Fermilab/U.Chicago)
- 329
-
330
coffee break
-
331
Physics Opportunities with Booster Replacement OptionsSpeaker: Matthew Toups (FNAL)
-
332
DUNE Physics with 2.4 MW UpgradeSpeaker: Chris Marshall (University of Rochester)
-
333
LBNF Target Station UpgradesSpeaker: Patrick Hurh (FNAL)
-
334
R&D for target materialsSpeaker: Frederique Pellemoine (Fermilab -AD - TSD - TRD)
-
335
Discussion
-
324
-
Cross frontier sessions: Quantum Science & Technology (QST) Instrumentation (IF) & Underground Facilities (UF) 111 (JHN)
111
JHN
22FA panel during the 22j session discussing the intersections of the AF and EF frontiers
Convener: John Orrell (Pacific Northwest National Laboratory)-
336
Short introductionSpeaker: John Orrell (Pacific Northwest National Laboratory)
-
337
Low-background quantum sensing at Fermilab's underground facilitySpeaker: Daniel Bowring (Fermilab)
-
338
R&D Needs for Studying the Effects of Radiation on Superconducting Quantum DevicesSpeaker: Ben Loer (Pacific Northwest National Laboratory)
-
339
Discussion - Underground infrastructure needs for QST/QISSpeaker: John Orrell (Pacific Northwest National Laboratory)
-
336
-
Energy Frontier: BSM II 220 (Kane Hall)
220
Kane Hall
19OConveners: Simone Pagan Griso (Lawrence Berkeley National Laboratory), Tulika Bose (University of Wisconsin-Madison), Zhen Liu (University of Minnesota)-
340
IntroductionSpeakers: Simone Pagan Griso (Lawrence Berkeley National Laboratory), Tulika Bose (University of Wisconsin-Madison), Zhen Liu (University of Minnesota)
-
341
New Bosons and Heavy Resonances
10' after the talk is reserved for Q&A
Speaker: Robert Harris (Fermilab) -
342
New Fermions
10' after the talk is reserved for Q&A
Speaker: Julie Hogan (Bethel University) -
343
LLPs: overview of main results in the reportSpeaker: Juliette Alimena (CERN)
-
344
LLPs: interplay with instrumentation frontierSpeakers: Cristián Peña (Fermi National Accelerator Laboratory), Cristián Peña (Fermi National Accelerator Laboratory)
-
345
LLPs: common discussion
-
346
Panel: strengthen the main messages of the EF BSM report -- feedback from communitySpeakers: Dean Robinson (LBL), Stephane Willocq (University of Massachusetts), Suchita Kulkarni, Tova Holmes (University of Tennessee)
-
340
-
Energy Frontier: EWK I 130 (Kane Hall)
130
Kane Hall
19NConveners: Alberto Belloni, Ayres Freitas (University of Pittsburgh)-
347
Longitudinally polarized ZZ scattering at the Muon Collider
3' after the talk is reserved for Q&A
Speaker: Tianyi Yang (Peking Univ.) -
348
Vector Boson Scattering processes: Status and prospects
3’ after the talk is reserved for Q&A
Speaker: Michele Gallinaro (LIP Lisbon) -
349
Electroweak Fragmentations/Parton Showers at high energies
5’ after the talk is reserved for Q&A
Speaker: Keping Xie (University of Pittsburgh) -
350
Anomalous quartic gauge couplings at a muon collider
5’ after the talk is reserved for Q&A
Speaker: Elham E Khoda (University of Washington) -
351
Sensitivity to longitudinal vector boson scattering in W±W±jj at future hadron colliders
3’ after the talk is reserved for Q&A
Speaker: Luka Nedic (Oxford U.) -
352
Analysis of Higgs production in the VBF-VH channel at the LHC
3’ after the talk is reserved for Q&A
Speaker: Chaitanya Paranjape (IIT Dhanbad) -
353
EW restoration in at the LHC and beyond
3’ after the talk is reserved for Q&A
Speaker: Ian Lewis (University of Kansas) -
354
Coffee Break
-
355
Precision electroweak physics at the LHeC and FCC-eh
3’ after the talk is reserved for Q&A
Speaker: Daniel Britzger (MPI Munich) -
356
Precise electroweak measurements at ILC
5’ after the talk is reserved for Q&A
Speaker: Taikan Suehara (Kyushu University) -
357
Enabling precision EW measurements at high energy e+e- colliders with in situ center-of-mass energy measurements
5’ after the talk is reserved for Q&A
Speaker: Graham Wilson (University of Kansas) -
358
Measuring the tau polarisation at ILC
5’ after the talk is reserved for Q&A
Speaker: Keita Yumino (SOKENDAI) -
359
Electroweak physics at the Belle II/SuperKEKB beam polarization upgrade
5’ after the talk is reserved for Q&A
Speaker: John Michael Roney (University of Victoria)
-
347
-
Energy Frontier: Top I 210 (Kane Hall)
210
Kane Hall
19MConveners: Doreen Wackeroth (University at Buffalo, SUNY), Reinhard Schwienhorst (Michigan State University)-
360
Status and outlook for top quark coupling measurements
10' after the talk is reserved for Q&A
Speaker: Gauthier Durieux (CERN) -
361
Top cross-section measurements
10' after the talk is reserved for Q&A
Speaker: Regina Demina (University of Rochester) -
362
Top-pair and single top production at hadron colliders
10' after the talk is reserved for Q&A
Speaker: Nikolaos Kidonakis (Kennesaw State University) -
363
Coffee Break
-
364
Top quark mass at lepton colliders
10' after the talk is reserved for Q&A
Speaker: Frank Simon (Max-Planck-Institute for Physics) -
365
Overview of spin correlation and FCNC in top
10' after the talk is reserved for Q&A
Speaker: Amandeep Singh Bakshi (Purdue University) -
366
Discussion of Vision for top quark physics and heavy flavor productionSpeakers: Doreen Wackeroth (University at Buffalo, SUNY), Reinhard Schwienhorst (Michigan State University)
-
360
-
Instrumentation Frontier: Discussing the Report with the Community 175 (JHN)
175
JHN
30FConveners: Jinlong Zhang (ANL), Petra Merkel (Fermi National Accelerator Laboratory), Phillip Barbeau (Duke University)-
367
IF Introduction
short introduction of overall IF report
Speaker: Phillip Barbeau (Duke University) -
368
Key points from IF01 - Quantum SensorsSpeakers: Kent Irwin (Stanford University and SLAC), Reina Maruyama (Yale University), Tom Cecil (Argonne), matt pyle (University of California Berkeley)
-
369
Key points from IF02 - Photon DetectorsSpeakers: Carlos Escobar (FERMILAB), Christopher Rogan, Juan Estrada Vigil (FNAL)
-
370
Key points from IF03 - Solid State Detectors and TrackingSpeakers: Artur Apresyan (Fermilab), Steven Worm, Tony Affolder (UCSC- SCIPP)
-
371
Key points from IF04 - Trigger and DAQSpeakers: Allison Deiana, Darin Acosta (Rice University), Wesley Ketchum (Fermi National Accelerator Laboratory)
-
372
Key points from IF05 - Micro Pattern Gas Detectors (MPGDs)Speakers: Bernd Surrow (Temple University), Maxim Titov (CEA Saclay), Sven Vahsen (University of Hawaii)
-
373
Key points from IF06 - CalorimetrySpeakers: Andy White (U. texas at Arlington), Minfang Yeh (Brookhaven National Laboratory), Rachel Yohay (Florida State University)
-
374
Key points from IF07 - Electronics/ASICsSpeakers: Gabriella Carini (Brookhaven National Laboratory), John Parsons (Columbia University (US)), Mitch Newcomer (U.Penn)
-
375
Key points from IF08 - Noble ElementsSpeakers: Carl Dahl (Northwestern University), Eric Dahl (Northwestern University / Fermilab), Jennifer Raaf (Fermilab), Roxanne Guenette, Roxanne Guenette (University of Manchester)
-
376
Key points from IF09 - Cross Cutting and Systems IntegrationSpeakers: Ian Shipsey (Oxford), Ian Shipsey (Oxford), James Fast (PNNL), Maurice Garcia-Sciveres (Lawrence Berkeley National Laboratory), Maurice Garcia-Sciveres (LBNL), Mauricio Garcia-Sciveres
-
377
Key points from IF10 - Radio DetectionSpeakers: Albrecht Karle (University of Wisconsin ), Amy Connolly (OSU)
-
09:45
Coffee break
-
378
IF report discussion and input from the community
https://docs.google.com/document/d/1rg3495-phcrHYj5PzSwSBHrbEtIdWuZZpd5REMPEvq0/edit
Speakers: Jinlong Zhang (ANL), Petra Merkel (Fermi National Accelerator Laboratory), Phillip Barbeau (Duke University)
-
367
-
Neutrino Physics Frontier: DUNE P5 Strategy (Expanded Physics Scope in Phase II) 110 (Kane Hall)
110
Kane Hall
20YConvener: Kate Scholberg (Duke University)- 379
-
380
Neutrinoless Double Beta DecaySpeaker: Julieta Gruszko
-
381
Low(er) Energy PhysicsSpeaker: David Caratelli (UC Santa Barbara)
-
382
Tau neutrino appearanceSpeakers: Mary Bishai (Brookhaven National Laboratory), Mary Bishai
-
09:52
Coffee break
-
Rare Processes and Precision Frontier: RF6 3 Big Idea + 1 Experimental Summary White Papers 337 (HUB)
337
HUB
20B- 383
- 384
- 385
- 386
-
387
Discussion on the RF6 reportSpeakers: Mike Williams (MIT), Stefania Gori (UC Santa Cruz)
-
Theory Frontier: Astro-particle physics & cosmology (TF9); Theory of neutrino physics (TF11) 214 (HUB)
214
HUB
18CConveners: Andre de Gouvea (Northwestern University), Daniel Green (UCSD)-
388
Fundamental Physics from Cosmic SurveysSpeaker: Benjamin Wallisch (Institute of Advanced Study & University of California San Diego)
- 389
-
390
Dark Matter and Dark Sectors: from Theory to Discovery in the LabSpeaker: Masha Baryakhtar (New York University)
-
391
Dark Matter and Dark Sectors: from Theory to Discovery in the SkySpeaker: Joshua Foster (University of Michigan)
-
09:40
Coffee Break
-
392
Neutrino Theory and Particle PhysicsSpeaker: Prof. Lisa Everett (UW Madison)
- 393
-
394
Neutrino Theory and Astrophysics & CosmologySpeaker: Evan Grohs (North Carolina State University)
-
388
-
Computational Frontier: CompF6 Quantum Computing 248 (MGH)
248
MGH
20T-
395
IntroductionSpeakers: Gabriel Perdue (Fermilab), Martin Savage (Institute For Nuclear Theory), Travis Humble (Oak Ridge National Laboratory)
- 396
- 397
- 398
- 399
-
400
Computing Needs for Quantum MaterialsSpeaker: Sinéad Griffin (Lawrence Berkeley National Lab)
-
11:00
Break
-
401
Quantum NetworksSpeaker: Nicholas Peters (Oak Ridge National Laboratory)
-
402
Quantum Computing for Data AnalysisSpeaker: Andrea Delgado (Oak RIdge National Laboratory)
-
403
Computing Systems and SoftwareSpeaker: Dr Kathleen Hamilton (Oak Ridge National Laboratory)
-
11:40
Schedule Slack and Discussion
-
395
-
Cross frontier sessions: RF-EF Long Lived Particles 220 (Kane Hall)
220
Kane Hall
30GA panel during the 22j session discussing the intersections of the AF and EF frontiers
Conveners: Mike Williams (MIT), Simone Pagan Griso (Lawrence Berkeley National Laboratory), Stefania Gori (UC Santa Cruz), Tulika Bose (University of Wisconsin-Madison), Zhen Liu (University of Minnesota)-
10:00
Coffee Break
-
404
Models for long-lived particles at high-energy and high-intensity experiments
5' after the talk is reserved for Q&A
Speaker: Simon Knapen (Lawrence Berkeley National Lab and UC Berkeley) -
405
Searches for long-lived particles at high-energy and high-intensity experiments
5' after the talk is reserved for Q&A
Speaker: Brian Batell (University of Pittsburgh) -
406
Forward Physics Facility for HL-LHC
5' after the talk is reserved for Q&A
Speaker: Jonathan Feng (UC Irvine) -
407
Discussion on common RF6-EF09 message for snowmass
-
10:00
-
Neutrino Physics Frontier: DUNE P5 Strategy (Phase II Detector R&D) 110 (Kane Hall)
110
Kane Hall
20OConvener: Elizabeth Worcester (BNL)-
10:00
Coffee Break
-
408
DUNE ContextSpeaker: Sergio Bertolucci (University of Bologna)
- 409
- 410
- 411
-
412
Photo-ionizing LArSpeaker: Fernanda Psihas Olmedo (Fermi National Accelerator Laboratory)
-
413
TheiaSpeakers: Gabriel Orebi Gann (UC Berkeley / LBNL), Gabriel Orebi Gann (University of California at Berkeley/LBNL)
-
10:00
-
Rare Processes and Precision Frontier: RF7 Exp And Theory Overview - Hadron Spectroscopy 337 (HUB)
337
HUB
20R-
414
Welcome and Summary of RF7 activities
(in person)
Speaker: Tomasz Skwarnicki (Syracuse University) -
415
Future of Hadron Spectroscopy at LHC
(remote)
Speaker: Matt Durham (Los Alamos National Lab) -
416
Future of Hadron Spectroscopy at Belle II
(in person)
Speaker: Jake Bennett (The University of Mississippi) -
417
Future of Hadron Spectroscopy at BESIII and Super Tau-Charm Factory
(remote)
Speaker: N Huesken -
418
Future of Hadron Spectroscopy at Photoproduction Experiments
(remote)
Speaker: Sean Dobbs (FSU) -
419
Amplitude Analyses in Hadron Spectroscopy
(remote)
Speaker: ARKAITZ RODAS (College of William & Mary) -
420
Hadron Spectroscopy with Lattice QCD
(remote)
Speaker: M Padmanath (Graz U.) -
421
Future of Phenomenology of Hadron Spectroscopy
(in person)
Speaker: Richard Lebed (Arizona State University)
-
414
-
Underground Facilities Frontier: UF5 - Synergistic Underground Science & Facilities 111 (JHN)
111
JHN
18BConvener: John Orrell (Pacific Northwest National Laboratory)-
422
Overview of Synergistic Underground ResearchSpeaker: John Orrell (Pacific Northwest National Laboratory)
-
423
Opportunities for Synergistic Research Presentations (10' each)
-
424
Open discussion: Key messages or additions for Synergistic Underground ResearchSpeaker: John Orrell (Pacific Northwest National Laboratory)
-
422
-
Social: LIGO Hanford Observatory live virtual tour Zoom
Zoom
https://washington.zoom.us/j/98883066364?pwd=UjVOajdLMFpMQWVibUtsR010T1AzUT09
Convener: Joey Key (University of Washington Bothell)-
425
LIGO Hanford Observatory virtual tourSpeaker: Joey Key (University of Washington Bothell)
-
425
-
US funding Agency Meetings: NSF General Meeting 210 (Kane Hall)
210
Kane Hall
36B-
426
The NSFSpeaker: James Shank (NSF)
-
426
-
Afternoon Plenary: Neutrino Frontier Connections, Progress, and Plans 210 (Kane Hall)
210
Kane Hall
20BBConveners: Elizabeth Worcester (BNL), Kate Scholberg (Duke University), Patrick Huber (Virginia Tech)-
427
Neutrino Frontier Connections
Neutrino Frontier physics topics with especially strong connections to other frontiers and/or non-HEP funding sources
-
a) 0nbb and neutrino massSpeaker: Joseph Formaggio Formaggio (MIT)
-
b) Neutrino interactionsSpeaker: Kendall Mahn (Michigan State University)
-
c) Beams and instrumentationSpeakers: Joshua Klein (University of Pennsylvania), Joshua Klein
-
-
428
Neutrino Frontier Connections, Progress, and Plans
Panel discussion on neutrino frontier projects, including timelines, costs, future planning, balance of program with introductory project overview presentation
-
a) OverviewSpeaker: Joseph Lykken (Fermilab)
-
b) Panel/FAQs with invited panelists
Panelists: Sergio Bertolucci, Joe Lykken, Reina Maruyama, Lia Merminga, Jason Newby, J. Pedor Ochoa, Ron Ray
Speakers: J. Pedro Ochoa (University of California at Irvine), Jason Newby (Oak Ridge National Laboratory), Joseph Lykken (Fermilab), Lia Merminga (FNAL), Reina Maruyama (Yale University), Ronald Ray (Fermilab), Sergio Bertolucci (University of Bologna)
-
-
427
-
Afternoon Plenary: Rare Proceses and Precision measurement and AMO 220 (Kane Hall)
220
Kane Hall
30HConveners: Alexey Petrov (Wayne State University), Marina Artuso (syracuse university), Robert Bernstein (Fermilab)-
429
Understanding Dark Matter and Dark Sectors at RP Frontier
(45 min)
Speaker: Stefania Gori (UCSC)Speaker: Stefania Gori (UC Santa Cruz) -
430
Roundtable: EDMs, atomic parity violation, and gravity signatures and synergies with the AMO physics programSpeakers: Marianna Safronova (University of Delaware), Nick Hutzler (Caltech), On Kim (Institute for Basic Science, Center for Axion and Precision Physics Research), Tanmoy Bhattacharya (Los Alamos National Laboratory)
-
429
-
Afternoon Plenary: Detector Technologies for the Next Decades 220 (Kane Hall)
220
Kane Hall
30IConveners: Jinlong Zhang (ANL), Petra Merkel (Fermi National Accelerator Laboratory), Phillip Barbeau (Duke University)-
431
Advancing detector instrumentation over the next decadesSpeaker: James Fast (Jefferson Lab)
-
432
Detector needs for future collider experimentsSpeaker: Andy White (U. texas at Arlington)
-
433
Detector needs for future cosmic experimentsSpeaker: Reina Maruyama (Yale University)
-
434
Detector needs for future neutrino and intensity experimentsSpeaker: Wesley Ketchum (Fermi National Accelerator Laboratory)
-
435
Questions and discussion
-
431
-
17:00
Coffee Lobby (Kane Hall)
Lobby
Kane Hall
-
Social: Adam Riess Public Lecture 130 (Kane Hall)
130
Kane Hall
https://washington.zoom.us/j/98883066364?pwd=UjVOajdLMFpMQWVibUtsR010T1AzUT09
-
-
-
Accelerator Frontier: AF5 Report (1.5 hrs), AF1 Report (1.5 hrs) and AF-Summary-II (1 hrs) 130 (Kane Hall)
130
Kane Hall
24LConveners: Eric Prebys, Steve Gourlay (LBNL), Tor Raubenheimer (SLAC), Vladimir Shiltsev (FNAL)- 436
-
437
EDMSpeaker: Richard Talman (Laboratory of Elementary Particle Physics, Cornell University)
-
438
Discussion
-
439
AF1: Education, Outreach & Diversity in Accelerator Science & EngSpeaker: Steven Lund (USPAS / MSU / FRIB)
-
440
AF1: Beam Physics and Accelerator Education Summary ReportSpeaker: Mei Bai (SLAC)
-
441
Particle Accelerator ModelingSpeaker: Jean-Luc Vay (Lawrence Berkeley National Laboratory)
-
Accelerator Frontier: Internal AF7 (2 hrs) 175 (JHN)
175
JHN
24KConveners: Emilio Nanni (SLAC National Accelerator Laboratory), GianLuca Sabbi (LBNL)-
442
AF7 Report DiscussionSpeakers: Emilio Nanni (SLAC National Accelerator Laboratory), Hans Weise (DESY), Sergey Belomestnykh (Fermilab)
-
443
AF7 Community InputSpeakers: Ganapati Myneni (JLab), Jim Norem (-), Xueying Lu (Northern Illinois Univ / Argonne National Laboratory)
-
444
US Magnet Development Program Status and PlansSpeaker: Soren Prestemon (Lawrence Berkeley National Laboratory)
- 445
-
446
Leading-Edge technology And Feasibility-directed (LEAF) ProgramSpeaker: Giorgio Apollinari (Fermilab)
-
447
Next generation technology for low-cost Nb3Sn accelerator magnetsSpeaker: Giorgio Ambrosio (FNAL APS-TD/MSD)
-
442
-
Cosmic Frontier: Parallel 220 (Kane Hall)
220
Kane Hall
24M-
448
CF Report DiscussionSpeakers: Aaron Chou (Fermi National Accelerator Laboratory), Tim Tait (UC Irvine), Marcelle Soares-Santos (Fermilab)
-
10:00
Coffee & Free Discussion
-
449
Panel: Astroparticle Physics Synergies with Particle PhysicsSpeakers: Albrecht Karle (University of Wisconsin/WIPAC), Bangalore Sathyaprakesh, Erin O'Sullivan (Uppsala University), J. Patrick Harding (Los Alamos National Laboratory), John Krizmanic , Jorg Horandel, Regina Caputo , Tom Shutt (SLAC)
-
448
-
Cross frontier sessions: EF-CompF Big Experiments 110 (Kane Hall)
110
Kane Hall
18XA panel during the 22j session discussing the intersections of the AF and EF frontiers
Conveners: Mike Williams (MIT), Oliver Gutsche (Fermi National Accelerator Laboratory), Peter Onyisi (University of Texas at Austin)-
450
DUNE
Feedback from DUNE
Speaker: Heidi Schellman (Oregon state) - 451
-
452
CMS
Feedback from CMS
Speaker: JAMES LETTS (UCSD) -
453
LHCb
Feedback from LHCb
Speaker: Vladimir Gligorov -
454
CMB-S4
Feedback from CMB-S4
Speaker: Julian Borrill (Berkeley Lab & UC Berkeley) -
455
LSST
Feedback from LSST
Speaker: Leanne GUY (AURA/LSST) -
456
LSST-DESC
Feedback from LSST Dark Energy Science Collaboration (DESC)
Speakers: Heather Kelly, Jim Chiang -
457
Belle II
Feedback from Belle II
Speaker: Jake Bennett (The University of Mississippi) -
458
T2K
Feedback from T2K
Speakers: Patrick Dunne (Imperial College London), Sophie King -
459
NOvA
Feedback from NOvA
Speaker: Gavin S. Davies (Indiana University) -
460
SBN
Feedback from SBN
Speaker: Wesley Ketchum (Fermi National Accelerator Laboratory) -
461
Discussion
-
450
-
Cross frontier sessions: IF-RF-EF Fast timing requirements and technology developments for future experiments 337 (HUB)
337
HUB
21JA panel during the 22j session discussing the intersections of the AF and EF frontiers
Conveners: Marina Artuso (syracuse university), Tony Affolder (UCSC- SCIPP)-
462
Notes for Session
-
463
Fast Timing Requirements for Hadron and e+e- Colliders
15 min presentation + 5 min discussion
Speaker: Tommaso Tabarelli de Fatis (Università di Milano Bicocca and INFN (Milan. Italy)) -
464
Fast Timing Requirements for Muon Colliders
15 presentation + 5 min discussion
Speaker: Lawrence Lee (University of Tennessee, Knoxville) -
465
Fast Timing Requirements for Rare Processes and Precision Measurements
15 min presentations + 5 min discussion
Speaker: Matthew Rudolph (Syracuse University) -
466
Technology developments for fast timing (Trackers)
15 min presentation + 5 min discussion
Speaker: Simone Mazza (UC Santa Cruz) -
467
Technology developments for fast timing (Calorimetry)
15 meeting presentation + 5 min discussion
Speaker: Frank Simon (Max-Planck-Institute for Physics) -
468
Fast Timing Usings in the Electron-Ion ColliderSpeaker: Ye Zhenyu (University of Illinois at Chicago)
-
10:00
Coffee Break
- 469
-
470
Use Case: Long Lived Particle SearchSpeakers: Cristián Peña (Fermi National Accelerator Laboratory), Cristián Peña (Fermi National Accelerator Laboratory), Cristián Peña (Fermilab)
-
471
Discussion
Are the similar/common requirements from the different frontiers?
Are the technology development path likely to meet experimental goals?
Do the use cases (calorimetry, tracking, PID,...) result in convergent or divergent design/optimizations?
What are the most challenging problems and how can we address them?
-
462
-
Cross frontier sessions: Long Baseline Neutrinos and Underground Facilities (UF) for the Neutrino Frontier (NF) 231 (MGH)
231
MGH
18QA panel during the 22j session discussing the intersections of the AF and EF frontiers
-
472
Hyper-Kamiokande Project, the next generation nucleon decay and neutrino experimentSpeaker: Dr Masato Shiozawa
- 473
-
474
DUNE/SURFSpeaker: Jaret Heise (Sanford Underground Research Facility)
-
472
-
Cross frontier sessions: RF-EF-TF RF1 Flavor anomalies and exotics at colliders 241 (MGH)
241
MGH
22AA panel during the 22j session discussing the intersections of the AF and EF frontiers
-
475
current status (and prospects) of flavor anomalies (20'+10')Speaker: Rafael Silva Coutinho (Syracuse University)
-
476
BSM models (20'+10')Speaker: Wolfgang Altmannshofer (UC Santa Cruz)
-
477
high-energy searches at present and future colliders (20'+10')Speaker: Cari Cesarotti (Harvard University)
-
478
Discussion on flavor anomalies in Snowmass reports and main message
-
475
-
Energy Frontier: EWK II 210 (Kane Hall)
210
Kane Hall
21PConveners: Alberto Belloni, Ayres Freitas (University of Pittsburgh)-
479
Higgs/EW Fit at (HL-)LHC & muon colliders
5’ after the talk is reserved for Q&A
Speaker: Jorge de Blas (University of Granada) -
480
Higgs/EW Fit at future e+e- colliders
5’ after the talk is reserved for Q&A
Speaker: Michael Peskin (SLAC) -
481
SMEFT Fit for top-quark sector
5’ after the talk is reserved for Q&A
Speaker: Victor Miralles (IFIC-UV) -
482
SMEFT fit for 4-fermion & CP-violating interactions
5’ after the talk is reserved for Q&A
Speaker: Yong Du (ITP CAS) -
483
General discussion on global fits for Snowmass
-
484
Coffee break
-
485
Discussion of EWK report
-
479
-
Instrumentation Frontier: IF7 307 (HUB)
307
HUB
24GConveners: Gabriella Carini (Brookhaven National Laboratory), John Parsons (Columbia University (US)), Mitch Newcomer (U.Penn)-
486
IF 07 OverviewSpeakers: Gabriella Carini (Brookhaven National Laboratory), John Parsons (Columbia University (US)), Mitch Newcomer (U.Penn)
- 487
- 488
- 489
-
490
Optical LinksSpeakers: Alexander Paramonov (Argonne National Laboratory), Alexander Paramonov (Argonne National Laboratory)
-
10:00
Break
- 491
- 492
- 493
-
494
Roundtable
-
486
-
Neutrino Physics Frontier: Blue Sky/Very Long Term ideas 254 (MGH)
254
MGH
21MConveners: Kate Scholberg (Duke University), Louis Strigari (Texas A&M University), Raimund Strauss (Technical University Munich, Germany)-
495
Low-threshold detectorsSpeaker: Sunil Golwala (California Institute of Technology)
- 496
-
497
Directional neutrino and dark matter detectionSpeaker: Sven Vahsen (University of Hawaii)
-
498
Ultra-high energy neutrinosSpeaker: Angela Olinto (The University of Chicago)
- 499
-
500
Panel discussionSpeakers: Ben Monreal, Elisabetta Baracchini , Katherine Freese
-
09:50
Coffee Break
-
495
-
Theory Frontier: Effective field theory (TF02); Lattice gauge theory (TF05) 111 (JHN)
111
JHN
18DConveners: Ethan Neil (University of Colorado, Boulder), Zohreh Davoudi (University of Maryland)-
501
EFTs for Dark Matter PhenomenologySpeaker: Zhengkang Zhang (UC Berkeley)
-
502
Naturalness in Effective Field TheorySpeaker: Nathaniel Craig (UC Santa Barbara)
-
503
UV Constraints on IR PhysicsSpeaker: Prof. Claudia De Rham (Imperial College London)
-
09:45
Coffee Break
-
504
Lattice Gauge Theory for HEP: OverviewSpeaker: Zohreh Davoudi (University of Maryland)
- 505
-
506
Nucleons and nuclei for BSM searches and neutrino physicsSpeaker: Michael Wagman (Fermilab)
- 507
-
508
Lattice for BSM explorationSpeaker: Ethan Neil (University of Colorado, Boulder)
- 509
-
501
-
Computational Frontier: CompF7 Reinterpretation and long-term preservation of data and code 231 (MGH)
231
MGH
20DConvener: Stephen Bailey (Lawrence Berkeley National Lab)-
510
Overview of CompF7 Report
Overview of the CompF7 "Reinterpretation and Long-Term Preservation of Data and Code" report and recommendations.
See #compf07-preservation slack for location of live notes for this session.
Speaker: Stephen Bailey (Lawrence Berkeley National Lab) -
511
CompF7 White Paper: Data and Analysis Preservation, Recasting, and Reinterpretation
Comments from authors of contributed white paper
https://arxiv.org/abs/2203.10057Speaker: Matthew Feickert -
512
CompF7 White Paper: Analysis Description Language: A DSL for HEP Analysis
Comments from authors of https://arxiv.org/abs/2203.09886
Speaker: Sezen Sekmen -
513
CompF7 White Paper: Data Preservation for Cosmology
Comments from authors of https://arxiv.org/abs/2203.08113
Speaker: Stephen Bailey (Lawrence Berkeley National Lab) -
514
CompF7 Discussion
See #compf07-preservation slack for location of live notes for this session.
-
510
-
Cross frontier sessions: RF-EF-AF RF5 to discuss CLFV and heavy states 284 (MGH)
284
MGH
24OA panel during the 22j session discussing the intersections of the AF and EF frontiers
-
515
Theoretical Overview
Time includes at least 5' dedicated to Q&A
Speaker: Wolfgang Altmannshofer (UC Santa Cruz) -
516
CLFV in heavy state decays at colliders
Excluding Heavy-Quarks decays.
Time includes at least 5' dedicated to Q&ASpeaker: Mogens Dam (Niels Bohr Institute, Copenhagen University) -
517
CLFV in heavy quark decays - interplay between LFV and LFUV
Time includes at least 5' dedicated to Q&A
Speaker: Peter Stangl (University of Bern) -
518
Discussion on common message
-
515
-
Energy Frontier: Dark Matter Discussion 110 (Kane Hall)
110
Kane Hall
21N-
519
Minimal WIMP
15' after the talk reserved for Q&A
Speaker: Zhen Liu (University of Minnesota) -
520
Invisible Higgs
15' after the talk are reserved for Q&A
Speaker: Diallo BOYE (Brookhaven National Laboratory) -
521
Simplified models of BSM DM mediation
15' after the talk is reserved for Q&A
Speaker: Katherine Pachal (TRIUMF) -
522
Beyond WIMP DM modelsSpeakers: Suchita Kulkarni, Suchita Kulkarni
-
519
-
Neutrino Physics Frontier: Experimental Neutrino Anomalies 254 (MGH)
254
MGH
35AConveners: Alexandre Sousa (University of Cincinnati), Bryce Littlejohn (Illinois Institute of Technology), Georgia Karagiorgi (Columbia University), Pedro Machado (Fermilab)-
10:00
Coffee Break
-
523
Overview: Neutrino Experimental AnomaliesSpeakers: Alexandre Sousa (University of Cincinnati), Bryce Littlejohn (Illinois Institute of Technology), Georgia Karagiorgi (Columbia University), Pedro Machado (Fermilab)
-
524
Experimental Status: Atmospheric/Accelerator DIF and DARSpeaker: Mark Ross-Lonergan
-
525
Experimental Status: Radioactive Sources and Reactors over the Past 10 YearsSpeaker: Pranava Teja Surukuchi (Yale University)
-
526
Recent Theory Progress and Interpretation(s)Speaker: Matheus Hostert (Perimeter Institute)
-
527
Panel: Path to Resolution through Neutrino Experiments and Beyond
Moderators: Alex Sousa, Georgia Karagiorgi, Bryce Littlejohn, Pedro Machado
Panelists:
Carlos Arguelles
Milind Diwan
Karsten Heeger
Kevin Kelly
Marilena LoVerde
Alysia Marino
Walter Pettus
Dave Schmitz
Kate Scholberg
Josh Spitz
Bob Svoboda
Zahra Tabrizi
Matt Toups
Michael WallbankFocus 1: Path to resolution in this decade
Focus 2: Future program beyond the upcoming P5 periodFormat: 45 minutes for community-contributed questions followed by 15 minutes for live questions from the audience (in person and zoom)
Speakers: Alysia Marino (University of Colorado), Carlos Argüelles Delgado (Harvard University), David Schmitz (University of Chicago), Georgia Karagiorgi (Columbia University), Joshua Spitz (University of Michigan), Karsten Heeger (Yale University), Kate Scholberg (Duke University), Kevin Kelly (CERN), Marilena Loverde (University of Washington), Matthew Toups (FNAL), Michael Wallbank (University of Cincinnati), Milind Diwan (BNL), Robert Svoboda (UC Davis), Walter Pettus (Indiana University), Zahra Tabrizi (Northwestern University)
-
10:00
-
Birds of a Feather: Mental Health, Invisible Disabilities, and Neurodiversity 210 (Kane Hall)
210
Kane Hall
36EOther meetings that make use of the fact we are all in one place!
Conveners: Biswaranjan Behera (Colorado State University), Yu-Dai Tsai (University of California, Irvine)-
528
Intro to The Mental Health Lunch + Q&A
I will give a 20 minutes intro to the lunch, including the goals, the schedule, and the topics.
It will be followed by a brief Q&A sessionSpeaker: Yu-Dai Tsai (University of California, Irvine) -
529
My Personal Experience
Hitoshi will share his stories regarding mental health.
Speaker: Hitoshi Murayama (University of California, Berkeley & IPMU, University of Tokyo) -
530
Discussions: How to Normalize Mental Health Discussions
We will have a 20-minute monitored discussion. The topics can include
-
co-learningthe with LGBTQIA community about opening up on mental health issues
-
How to utilize resources, including HR, lab/school supports, etc.
-
Intersectionality: gender, racial, cultural discussions
Speakers: Biswaranjan Behera (Colorado State University), Yu-Dai Tsai (University of California, Irvine) -
-
531
Discussion: Support Invisible Disabilities & Neurodiversity
-
Conflict resolution for neuro-diverse people
-
Compile a list of negative phrases; transitioning from these descriptions & hidden discrimination
-
How to increase the representation of invisible disability and neuro-diversity
-
How to better value neuro-diverse excellence
Speakers: Yu-Dai Tsai (University of California, Irvine), Biswaranjan Behera (Colorado State University) -
-
528
-
US funding Agency Meetings: DOE PM: Cosmic frontier 110 (Kane Hall)
110
Kane Hall
36C-
532
DOE: Cosmic frontierSpeaker: Kathy Turner (DOE Office of High Energy Physics)
-
532
-
US funding Agency Meetings: NSF Special PI Meeting 130 (Kane Hall)
130
Kane Hall
36D- 533
-
534
Discussion
-
Afternoon Plenary: Rare Prcesses and Precision Measurements 130 (Kane Hall)
130
Kane Hall
21UConveners: Alexey Petrov (Wayne State University), Marina Artuso (syracuse university), Robert Bernstein (Fermilab)-
535
How far the SM can go: examples from the RP FrontierSpeaker: Prof. Phillip Urquijo (Uiversity of Melbourne)
-
536
Search for New Physics: the questions we can address with leptons and quarksSpeaker: Vincenzo Cirigliano (Los Alamos National Laboratory)
-
535
-
Afternoon Plenary: Beams, Accelerator R&D and Future Facilities: Accelerator Frontier Vision 130 (Kane Hall)
130
Kane Hall
30IConveners: Steve Gourlay (LBNL), Tor Raubenheimer (SLAC), Vladimir Shiltsev (FNAL)-
537
An accelerator R&D plan for the next 10 yearsSpeaker: Vladimir Shiltsev (FNAL)
-
538
Discussion/PanelSpeakers: Steve Gourlay (LBNL), Tor Raubenheimer (SLAC)
-
537
-
17:00
Coffee 225 and Lobby (Kane Hall)
225 and Lobby
Kane Hall
-
Social: Physics VR 225 - Walker Ames (Kane Hall)
225 - Walker Ames
Kane Hall
https://washington.zoom.us/j/98883066364?pwd=UjVOajdLMFpMQWVibUtsR010T1AzUT09
-
Afternoon Plenary: Cosmic Probes of Fundamental Physics 130 (Kane Hall)
130
Kane Hall
23WConveners: Aaron Chou (Fermilab), Marcelle Soares-Santos (Fermilab), Tim Tait (UC Irvine)- 539
-
540
Cosmic AccelerationSpeaker: Marcelle Soares-Santos (Fermilab)
-
541
Panel Discussion: Cosmic Opportunities for Fundamental PhysicsSpeakers: Andrew Sonnenschein (Fermilab), Prof. Chanda Prescod-Weinstein (University of New Hampshire), Jeffrey Newman (University of Pittsburgh and PITT-PACC), John Carlstrom (University of Chicago), Ke Fang (University of Wisconsin-Madison), Maria Elena Monzani (SLAC National Accelerator Laboratory), Marilena Loverde (Stony Brook University), Stefan Ballmer (Syracuse University)
-
Social: Physics Slam 130 (Kane Hall)
130
Kane Hall
https://washington.zoom.us/j/98883066364?pwd=UjVOajdLMFpMQWVibUtsR010T1AzUT09
-
542
Physics Slam
-
542
-
-
-
Accelerator Frontier: AF-wide: AF2 Report (2 hrs) and AF7-Targets and Sources Report (2 hrs) 130 (Kane Hall)
130
Kane Hall
24JConveners: Charlotte Barbier (ORNL), Frederique Pellemoine (Fermilab -AD - TSD - TRD), Robert Zwaska (Fermilab), Yine Sun (Argonne National Lab.)-
543
AF2 Report and Worldwide Capability TablesSpeaker: Robert Zwaska (Fermilab)
-
544
AF2 Report DiscussionSpeaker: Robert Zwaska (Fermilab)
-
09:40
Coffee Break
-
545
AF7 Targets Report and DiscussionSpeakers: Charlotte Barbier (ORNL), Frederique Pellemoine (Fermilab -AD - TSD - TRD), Yine Sun (Argonne National Lab.)
-
546
AF7 Sources Report and DiscussionSpeakers: Charlotte Barbier (ORNL), Frederique Pellemoine (Fermilab -AD - TSD - TRD), Yine Sun (Argonne National Lab.)
-
543
-
Accelerator Frontier: AF4 Internal (TBD) 214 (HUB)
214
HUB
24IConvener: Mark Palmer (Brookhaven National Laboratory)-
547
AF4+AF6 Discussion on AF4 ReportSpeaker: Mark Palmer (Brookhaven National Laboratory)
-
548
AF4 + Collider R&D Program DiscussionSpeakers: Alexander Valishev (Fermilab), Mark Palmer (Brookhaven National Laboratory), Nadia Pastrone (INFN-Torino), Pushpalatha Bhat (Fermilab), Sergei Nagaitsev (Fermilab/U.Chicago)
-
549
Collider in SeaSpeaker: Peter McIntyre (Texas A&M University)
-
547
-
Accelerator Frontier: CCC: AF3 Internal - eeForum 332 (HUB)
332
HUB
24HConveners: Caterina Vernieri (SLAC), Emilio Nanni (SLAC National Accelerator Laboratory), Mei Bai (SLAC)-
550
C3 in the context of EFSpeaker: Meenakshi Narain (Brown University)
- 551
- 552
- 553
-
554
Background SimulationsSpeaker: Lindsey Gray (Fermi National Accelerator Laboratory)
- 555
-
556
Beam Dump ExperimentsSpeaker: Douglas Tuckler (UC Santa Cruz and Fermi National Accelerator Laboratory)
-
557
Muon ExperimentsSpeaker: Dylan Rankin (Massachusetts Institute of Technology)
-
558
C3 in the Context of AF3/4Speaker: Angeles Faus-Golfe
- 559
-
560
BDS/FFSpeaker: Glen White (SLAC National Accelerator Lab)
- 561
-
562
C3 Demonstration R&D PlanSpeaker: Faya Wang
-
563
C3 in the Context of AF7Speaker: Sergey Belomestnykh (Fermilab)
-
564
Survey of Ongoing and Near-Term R&DSpeakers: Ankur Dhar (SLAC National Accelerator Lab), Emilio Nanni (SLAC National Accelerator Laboratory), Evgenya Simakov (LANL), Faya Wang, James Rosenzweig (UCLA), Martin Breidenbach (SLAC), Tor Raubenheimer (SLAC), Zenghai Li (SLAC)
-
550
-
Computational Frontier: Report Discussion 220 (Kane Hall)
220
Kane Hall
30KConveners: Benjamin Nachman (LBNL), Daniel Elvira (Fermilab), Steven Gottlieb (Indiana Univ.)-
565
IntroductionSpeakers: Benjamin Nachman (LBNL), Daniel Elvira (Fermilab), Steven Gottlieb (Indiana Univ.)
-
566
Experimental Algorithms ParallelizationSpeakers: Giuseppe Cerati (Fermi National Accelerator Laboratory), Katrin Heitmann (Argonne National Laboratory), Walter Hopkins (Argonne National Laboratory)
-
567
Theoretical Calculations and SimulationSpeakers: Kevin Pedro (Fermilab), Peter Boyle (Brookhaven National Laboratory), ji qiang (LBNL)
-
568
Machine LearningSpeakers: Daniel Whiteson (UC Irvine), Kazuhiro Terao, Phiala Shanahan (Massachusetts Institute of Technology)
-
569
Storage and processing resource accessSpeakers: Frank Wuerthwein (UCSD), Meifeng Lin (Brookhaven National Laboratory), Wahid Bhimji (NERSC, Berkeley Lab)
-
570
End user analysisSpeakers: Amy Roberts (CU Denver), Gavin Davies (University of Mississippi), Peter Onyisi (University of Texas at Austin)
-
571
Quantum computingSpeakers: Gabriel Perdue (Fermilab), Martin Savage (Institute For Nuclear Theory), Travis Humble (Oak Ridge National Laboratory)
-
572
Reinterpretation and long-term preservation of data and codeSpeakers: Kyle Cranmer (NYU), Matias Carrasco Kind (NCSA/University of Illinois), Stephen Bailey (Lawrence Berkeley National Lab)
-
573
Overall Computing Frontier reportSpeakers: Benjamin Nachman (LBNL), Daniel Elvira (Fermilab), Steven Gottlieb (Indiana Univ.)
-
574
Discussion
-
565
-
Cross frontier sessions: AF/EF 337 (HUB)
337
HUB
22GA panel during the 22j session discussing the intersections of the AF and EF frontiers
Conveners: GianLuca Sabbi (LBNL), Vladimir Shiltsev (FNAL)-
575
AF7m reportSpeakers: Alexander Zlobin (Fermilab), GianLuca Sabbi (LBNL)
-
576
Discussion
-
575
-
Cross frontier sessions: NF-CF Neutrino mass scale with beta decay kinematics, double beta decay, and cosmology 307 (HUB)
307
HUB
22CA panel during the 22j session discussing the intersections of the AF and EF frontiers
-
577
Inferring neutrino mass from beta-decay kinematicsSpeakers: Christine Claessens, Christine Claessens (JGU Mainz)
-
578
Inferring neutrino mass from cosmological probesSpeaker: Eleonora Di Valentino (University of Sheffield)
-
579
Inferring neutrino mass from neutrinoless double beta decaySpeaker: Jason Detwiler
-
580
Discovery scenarios among three neutrino-mass probesSpeaker: Massimiliano Lattanzi (INFN Ferrara)
-
09:50
Break
-
581
Model dependence in cosmological probesSpeaker: Steen Hannestad (University of Aarhus)
-
582
Model dependence in neutrinoless double-beta decay probesSpeaker: Andre de Gouvea (Northwestern University)
-
583
Further DiscussionSpeakers: Diana Parno (Carnegie Mellon University), Luis Anchordoqui (City University of New York, Lehman College), Luis Anchordoqui (University of Wisconsin Milwaukee)
-
577
-
Cross frontier sessions: NF-EF Cross-cutting issues 238 (MGH)
238
MGH
22HA panel during the 22j session discussing the intersections of the AF and EF frontiers
Convener: Andre de Gouvea (Northwestern University)- 584
- 585
-
586
Neutrinos and Muon CollidersSpeaker: Chris Rogers (Rutherford Lab)
-
Energy Frontier: BSM IV 102 (JHN)
102
JHN
23N-
587
Discussion of BSM Report and Conclusion Writing
Unstructured informal discussion on BSM report with EF08 and EF09 conveners. Everyone welcome to stop by and ask questions, express opinions and help to strengthen the main message of the report.
Speakers: Simone Pagan Griso (Lawrence Berkeley National Laboratory), Tulika Bose (University of Wisconsin-Madison), Zhen Liu (University of Minnesota)
-
587
-
Instrumentation Frontier: IF5 238 (HUB)
238
HUB
23DConveners: Bernd Surrow (Temple University), Maxim Titov (CEA Saclay), Sven Vahsen (University of Hawaii)-
588
MPGDs: Recent advances, current R&D, and the European StrategySpeaker: Klaus Dehmelt (Stony Brook University)
-
08:20
Q/A
-
589
MPGDs for nuclear physics experiments and a proposed MPGD center of excellenceSpeaker: Matt Posik (Temple University)
-
08:50
Q/A
-
590
MPGDs for Recoil imaging for DM, neutrino, and BSM physicsSpeaker: Ciaran O'Hare (University of Sydney)
-
09:20
Q/A
-
591
MPGDs for TPCs at future lepton collidersSpeaker: Alain Bellerive (Carleton University)
-
09:50
Q/A
- 592
-
10:20
Q/A
- 593
-
10:50
Q/A
-
594
US-based MPGD User facility (Video presentation)Speaker: Kondo Gnanvo
-
11:20
Q/A
-
595
MPGD SummarySpeakers: Maxim Titov (CEA Saclay), Sven Vahsen (University of Hawaii)
-
588
-
Instrumentation Frontier: IF8 288 (MGH)
288
MGH
24FConveners: Carl Dahl (Northwestern University), Eric Dahl (Northwestern University / Fermilab), Jennifer Raaf (Fermilab), Roxanne Guenette (University of Manchester), Roxanne Guenette-
596
Review of IF08 Topical Group Report
-
597
BREAK
-
598
Further discussion and community input to IF08 TG Report
-
596
-
Instrumentation Frontier: IF9 284 (MGH)
284
MGH
24EConveners: Ian Shipsey (Oxford), James Fast (PNNL), Maurice Garcia-Sciveres (LBNL)-
599
Report on the ECFA Detector R&D RoadmapSpeaker: Ian Shipsey (Oxford)
-
600
Review of IF9 Report & BREAK from 10:00Speakers: Ian Shipsey (Oxford), James Fast (PNNL), Maurice Garcia-Sciveres (LBNL)
-
601
Community Input to Final Report
-
599
-
Neutrino Physics Frontier: Optimizing Among Funding Agencies 254 (MGH)
254
MGH
21LConveners: Julieta Gruszko, Kate Scholberg (Duke University), Steven Gardiner (Fermilab)-
602
Neutrino Frontier Inter-Agency Discussion
-
602
-
Rare Processes and Precision Frontier: RF3 Discussions 231 (MGH)
231
MGH
21B-
603
IntroductionSpeakers: Peter Winter (Argonne National Laboratory), Thomas Blum (University of Connecticut)
-
604
Precision Studies of Spacetime Symmetries and Gravitational Physics
(remote)
Speaker: Ralf Lehnert -
605
Prospects for precise predictions of aμ in the Standard Model
(in person)
Speaker: Aida El-Khadra (University of Illinois at Urbana-Champaign) -
606
EDMs and the search for new physics
(in person)
Speaker: Tanmoy Bhattacharya (Los Alamos National Laboratory) -
607
The storage ring proton EDM at 10^(−29) 𝑒⋅cm
(in person)
Speaker: On Kim (Institute for Basic Science, Center for Axion and Precision Physics Research) - 608
-
609
Q & A
-
603
-
Theory Frontier: TF04: Theory of Scattering Amplitudes 175 (JHN)
175
JHN
35CConveners: Jaroslav Trnka (UC Davies), Zvi Bern (UCLA)- 610
-
611
Amplitudes and Fundamental Physics (Zoom)Speaker: Prof. Henriette Elvang (University of Michigan)
-
612
Amplitudes and Precision at Hadron CollidersSpeaker: Fernando Febres Cordero (FSU)
-
613
Amplitudes and Gravitational WavesSpeaker: Dr Enrico Herrmann (UCLA)
-
Theory Frontier: Theory techniques for precision physics (TF06); Collider phenomenology (TF07) 111 (JHN)
111
JHN
18FConveners: Radja Boughezal (Argonne National Laboratory), Shufang Su (University of Arizona)-
614
Precision Theory for HEP: OverviewSpeaker: Radja Boughezal (Argonne National Laboratory)
-
615
Theoretical Developments in SMEFT Beyond Dim-6Speaker: Frank Petriello (Northwestern University)
- 616
-
617
Precision measurements and field theory: a virtuous cycleSpeaker: Dr Isabel Garcia Garcia (KITP)
-
09:45
Coffee Break
- 618
-
619
New Observables for Precision Colllider PhysicsSpeaker: Ian Moult (Lawrence Berkeley Laboratory)
-
620
Calculational Challenges for High-Energy CollidersSpeaker: Fabio Maltoni (Universite' catholique de Louvain)
- 621
-
622
Discussion of TF07 Report Executive SummarySpeaker: Shufang Su (University of Arizona)
-
614
-
Energy Frontier: BSM V 102 (JHN)
102
JHN
31A-
623
Discussion of BSM Report and Conclusion Writing (continued)
Unstructured informal discussion on BSM report with EF08 and EF09 conveners. Everyone welcome to stop by and ask questions, express opinions and help to strengthen the main message of the report.
Speakers: Elliot Lipeles (University of Pennsylvania), James Hirschauer (Fermi National Accelerator Laboratory), Nausheen Shah (Wayne State University)
-
623
-
Computational Frontier: Industry Session 220 (Kane Hall)
220
Kane Hall
30LConveners: Peter Boyle (Brookhaven National Laboratory), Steven Gottlieb (Indiana Univ.)- 624
- 625
-
626
Andrew Putnam, MicrosoftSpeaker: Andrew Putnam
- 627
-
Cross frontier sessions: EF-AF combined EF/AF reports discussion 022 (JHN)
022
JHN
21VA panel during the 22j session discussing the intersections of the AF and EF frontiers
Conveners: Dmitri Denisov (Fermilab), Tor Raubenheimer (SLAC)-
628
Energy Frontier report summarySpeaker: Alessandro Tricoli (BNL)
-
629
Accelerator Frontier report summarySpeaker: Vladimir Shiltsev (FNAL)
-
630
Discussion of EF and AF reportsSpeaker: Dmitri Denisov (Fermilab)
-
628
-
Cross frontier sessions: RF-EF-TF RF7-EF6-EF7 hadrons as production probes; production mechanisms probing the internal structure of exotic hadrons 248 (MGH)
248
MGH
23AA panel during the 22j session discussing the intersections of the AF and EF frontiers
-
Cross frontier sessions: TF-CompF QIS 337 (HUB)
337
HUB
21ZA panel during the 22j session discussing the intersections of the AF and EF frontiers
-
631
Session ChairsSpeakers: Christian Bauer (LBNL), Gabriel Perdue (Fermilab), Nathaniel Craig (UC Santa Barbara)
- 632
- 633
- 634
-
635
Quantum Computing: ApplicationsSpeakers: Martin Savage (INT), Zohreh Davoudi (University of Maryland)
-
631
-
Rare Processes and Precision Frontier: RF5 Discussions 231 (MGH)
231
MGH
21R- 636
-
637
CLFV theory overviewSpeaker: Julian Heeck (University of Virginia)
- 638
- 639
-
640
Muonium - antimuonium experimentsSpeaker: Daniel Kaplan (Illinois Institute of Technology)
-
641
CLFV in tau decaysSpeaker: Swagato Banerjee (University of Louisville)
-
Underground Facilities Frontier: UF1 - Underground Facilities for Neutrinos 242 (MGH)
242
MGH
22QConveners: Danielle Speller (Johns Hopkins University), Patrick Decowski (Nikhef / University of Amsterdam), Timothy Bolton (Kansas State University)-
642
UF1 highlights and key points of the topical reportSpeaker: Danielle Speller (Johns Hopkins University)
-
643
Open for feedback & discussionSpeaker: Timothy Bolton (Kansas State University)
-
642
-
Community Engagement Frontier: Early Career panel (session is Q&A on non-HEP/industry jobs) 220 (Kane Hall)
220
Kane Hall
36HConveners: Julie Hogan (Bethel University), Sudhir Malik (University of Puerto Rico Mayaguez) -
US funding Agency Meetings: DOE PM: Energy 130 (Kane Hall)
130
Kane Hall
36F-
644
DOE: Energy FrontierSpeaker: Abid Patwa (U.S. Department of Energy)
-
644
-
US funding Agency Meetings: DOE PM: Theory 175 (JHN)
175
JHN
36G- 645
-
Afternoon Plenary: Advancing Research at Underground Facilities (UF) 130 (Kane Hall)
130
Kane Hall
22VConveners: Laura Baudis (University of Zurich), Jeter Hall (SNOLAB), Kevin Lesko (LBNL), John Orrell (Pacific Northwest National Laboratory)-
646
Underground needs for Neutrino & Cosmic Frontier scienceSpeaker: Scott Hertel (UMass Amherst)
-
647
Supporting infrastructure and synergistic researchSpeaker: Alvine Kamaha (UCLA)
-
648
A strategy for underground facilities and researchSpeaker: John Orrell (Pacific Northwest National Laboratory)
-
649
Questions and discussion
-
646
-
Afternoon Plenary: Theory Frontier: A Vision for the Future 130 (Kane Hall)
130
Kane Hall
30MConveners: Aida El-Khadra (University of Illinois at Urbana-Champaign), Csaba Csaki (Cornell University), Nathaniel Craig (UC Santa Barbara)-
650
Recent developments and future vision for formal theorySpeaker: Shamit Kachru (Stanford University)
-
651
Recent developments and future vision for particle theorySpeaker: Jesse Thaler (MIT)
-
650
-
17:00
Coffee 225 and Lobby (Kane Hall)
225 and Lobby
Kane Hall
-
Afternoon Plenary: Big Picture Neutrino Science 130 (Kane Hall)
130
Kane Hall
22WConveners: Elizabeth Worcester (BNL), Kate Scholberg (Duke University), Patrick Huber (Virginia Tech)-
652
Oscillation Physics: Three flavors and BeyondSpeaker: Mark Messier (Indiana University)
- 653
- 654
-
655
Questions and discussion
-
652
-
Social: Conference Dinner 211 South Ballroom (HUB)
211 South Ballroom
HUB
https://washington.zoom.us/j/98883066364?pwd=UjVOajdLMFpMQWVibUtsR010T1AzUT09
-
-
-
Accelerator Frontier: AF-wide: AF7-RF Report ( 2hrs) and AF7-Magnets Report (2 hrs) 110 (Kane Hall)
110
Kane Hall
24CConveners: Alexander Zlobin (Fermilab), Emilio Nanni (SLAC National Accelerator Laboratory), GianLuca Sabbi (LBNL), Sergey Belomestnykh (Fermilab)-
656
AF7 RF ReportSpeakers: Emilio Nanni (SLAC National Accelerator Laboratory), Sergey Belomestnykh (Fermilab)
-
657
Magnet reportSpeakers: Alexander Zlobin (Fermilab), GianLuca Sabbi (LBNL), Susana Izquierdo Bermudez (CERN)
-
658
Discussion
-
656
-
Accelerator Frontier: AF3 Report (1hr) and AF4 Internal (1 hr) 120 (Kane Hall)
120
Kane Hall
18MConveners: Frank Zimmermann (CERN), Georg Hoffstaetter (Cornell University), Mark Palmer (Brookhaven National Laboratory)- 659
-
Cross frontier sessions: IF-NF Instrumentation for Neutrino Experiments 026 (JHN)
026
JHN
21GA panel during the 22j session discussing the intersections of the AF and EF frontiers
- 660
-
661
Radio Detection TechniquesSpeaker: Albrecht Karle (University of Wisconsin-Madison)
-
662
Dichroic Approaches to Photon DetectionSpeaker: Samuel Naugle (University of Pennsylvania)
- 663
- 664
-
665
New Materials for Neutrino DetectionSpeaker: Minfang Yeh (Brookhaven National Laboratory)
-
Cross frontier sessions: IF-UF Cross-cutting Facilities 022 (JHN)
022
JHN
21FA panel during the 22j session discussing the intersections of the AF and EF frontiers
-
Cross frontier sessions: TF-CF Cosmic Frontier Theory 220 (Kane Hall)
220
Kane Hall
19KA panel during the 22j session discussing the intersections of the AF and EF frontiers
Conveners: Prof. Daniel Green (UCSD), Flip Tanedo (UC Riversider), Tracy Slatyer (MIT)- 666
-
667
Cosmic probes of dark matter physicsSpeaker: Chanda Prescod-Weinstein (University of New Hampshire)
- 668
-
669
Opportunities at the Intersection of Theory and ObservationsSpeaker: Benjamin Wallisch (Institute of Advanced Study & University of California San Diego)
-
10:00
Coffee break
-
670
Panel discussion: Theory and the Cosmic FrontierSpeakers: Hitoshi Murayama (University of California, Berkeley & IPMU, University of Tokyo), Joel Meyers (Southern Methodist University), Lindsey Bleem (Argonne National Laboratory), Masha Baryakhtar (New York University), Patrick Fox (Fermilab)
-
Energy Frontier: Discussion and Summaries 130 (Kane Hall)
130
Kane Hall
24NConveners: Alessandro Tricoli (BNL), Laura Reina (Florida State University), Meenakshi Narain (Brown University)-
671
Energy Frontier OverviewSpeaker: Meenakshi Narain (Brown University)
-
672
Physics at the HL-LHC with ATLAS and CMS
5’ after the talk is reserved for Q&A
Speaker: Jennet Dickinson (Fermilab) -
673
Higgs Report
5’ after the talk is reserved for Q&A
Speakers: Caterina Vernieri (SLAC), Isobel Ojalvo (Princeton University (US)), Patrick Meade (Stony Brook University), Sally Dawson (Brookhaven National Laboratoy) -
674
Top Quark Report
5’ after the talk is reserved for Q&A
Speakers: Doreen Wackeroth (University at Buffalo, SUNY), Reinhard Schwienhorst (Michigan State University) -
675
Electroweak Report
5’ after the talk is reserved for Q&A
Speakers: Alberto Belloni, Ayres Freitas (University of Pittsburgh), Junping Tian (University of Tokyo) -
676
Strong Interactions Report
5’ after the talk is reserved for Q&A
Speakers: Christophe Royon, Huey-Wen Lin (MSU), Michael Begel (Brookhaven National Lab), Michael Schmitt (Northwestern University), Pavel Nadolsky (Southern Methodist University), Stefan Hoeche (Fermilab) -
677
Coffee Break
-
678
BSM Report
10’ after the talk is reserved for Q&A
Speakers: Caterina Doglioni (Lund University), Elliot Lipeles (University of Pennsylvania), James Hirschauer (Fermi National Accelerator Laboratory), Liantao Wang (University of Chicago), Nausheen Shah (Wayne State University), Simone Pagan Griso (Lawrence Berkeley National Laboratory), Tulika Bose (University of Wisconsin-Madison), Zhen Liu (University of Minnesota) -
679
Discussion of Energy Frontier Report VisionSpeaker: Laura Reina (Florida State University)
-
671
-
Neutrino Physics Frontier: BSM/Dark Sectors & Reactor Neutrinos (Early Career Presentations) 254 (MGH)
254
MGH
20IConveners: Jacob Zettlemoyer (Fermilab), Julieta Gruszko-
680
First Results from MicroBooNE's Low Energy Excess Search and Constraints on eV-Scale Sterile Neutrino OscillationsSpeaker: Jay Hyun Jo (Yale University)
-
681
New bounds on axion-like particles from MicroBooNESpeakers: Salvador Urrea (Instituto de Física Corpuscular(IFIC) Valencia), Salvador Urrea Gonzalez (IFIC (UV))
-
682
Prospects for Dark Sector Searches at the Deep Underground Neutrino ExperimentSpeaker: Wooyoung Jang (University of Texas at Arlington)
-
683
Searching for dark matter with COHERENT at the Spallation Neutron SourceSpeaker: Daniel Pershey
-
684
Searches for New Physics at an Upgraded Fermilab Accelerator Complex: PIP2-BD and SBN-BDSpeaker: Jacob Zettlemoyer (Fermilab)
-
685
Bounds on Right Handed Neutrino Parameters from Observable LeptogenesisSpeaker: Stefan Sandner (IFIC UV / CSIC)
-
10:12
Break
-
686
Forthcoming Science from the PROSPECT-I Data SetSpeaker: Diego Venegas Vargas (University of Tennessee-Knoxville)
-
687
The design and expanded physics reach of the PROSPECT-II detector upgradeSpeaker: Felicia Sutanto (University of Michigan)
-
688
CONFLUX – A standard framework for reactor neutrino flux calculationSpeaker: XIANYI ZHANG (Lawrence Livermore National Laboratory)
-
689
JUNO: Physics Prospects and StatusSpeaker: Roberto Carlos Mandujano (University of California-Irvine)
-
680
-
Neutrino Physics Frontier: DUNE & Neutrino Interactions (Early Career Presentations) 241 (MGH)
241
MGH
20KConveners: Jacob Zettlemoyer (Fermilab), Steven Gardiner (Fermilab), Vishvas Pandey (University of Florida)-
690
A Gaseous Argon-Based Near Detector to Enhance the Physics Capabilities of DUNESpeaker: Tanaz Mohayai (Fermilab)
-
691
The Modular LArTPC – Design and Prototype for the DUNE NDSpeaker: Zoya Vallari (Caltech)
-
692
Sensitivity to Heavy Neutral Leptons with the SAND detector at the DUNE ND complexSpeaker: zahra ghorbanimoghaddam (INFN Genova)
-
693
Studies of tau neutrino appearance at the DUNE Near Detector complexSpeaker: Soamasina Herilala Razafinime
-
694
Probing active-sterile neutrino mixing in LED and 3+1 scenarios with DUNESpeaker: David Vanegas Forero (Universidad de Medellín)
-
695
BSM Targets at a Target-less DUNESpeaker: Zahra Tabrizi (Northwestern University)
-
10:12
Break
-
696
The NOvA Test Beam ProgramSpeaker: Michael Wallbank (University of Cincinnati)
- 697
-
698
Prospects for DUNE Measurements of Deep Inelastic Charged-Current Tau Neutrino InteractionsSpeaker: Barbara Yaeggy (University of Cincinnati)
-
699
Bubble Chamber Detectors with Light Nuclear Targets for Neutrino ScatteringSpeaker: Bryan Ramson
-
690
-
Rare Processes and Precision Frontier: All-Frontier Discussions 102 (JHN)
102
JHN
23Y -
Theory Frontier: BSM Model Building (TF08); Quantum Information Science (TF10) 210 (Kane Hall)
210
Kane Hall
18EConveners: Graham Kribs (Fermilab/U Oregon), simon catterall (syracuse university)-
700
Model Building Into the FutureSpeaker: Hitoshi Murayama (University of California, Berkeley & IPMU, University of Tokyo)
- 701
- 702
-
09:45
Coffee Break
- 703
- 704
- 705
-
700
-
Theory Frontier: String theory, quantum gravity, black holes (TF01); CFT and formal QFT (TF03) 238 (MGH)
238
MGH
18GConveners: Nathaniel Craig (UC Santa Barbara), Shamit Kachru (Stanford University)-
706
Particle Physics and String TheorySpeaker: Mirjam Cvetic (University of Pennsylvania)
-
707
Black Holes and Quantum GravitySpeaker: Prof. Xi Dong (UC Santa Barbara)
-
708
Some New Ideas in QFT and Condensed Matter PhysicsSpeaker: Prof. John McGreevy (UC San Diego)
-
09:45
Coffee Break
- 709
- 710
- 711
-
706
-
Cross frontier sessions: NF-CF-IF Talks+Panel 026 (JHN)
026
JHN
22JA panel during the 22j session discussing the intersections of the AF and EF frontiers
-
09:55
Cofffee Break
- 712
-
713
mKIDs and Quantum Sensors for DM and Neutrino PhysicsSpeaker: Marco Vignati (Sapienza U and INFN)
-
714
Low-threshold cryogenic detectors for neutrino physicsSpeaker: Rupak Mahapatra (Texas A&M University)
- 715
-
716
NF+IF+CF PanelSpeakers: Albrecht Karle (University of Wisconsin ), Cristiano Galbiati, Hugh Lippincott (UCSB), Julieta Gruszko, Mayly Sanchez (Iowa State University), Noah Kurinsky, Tanner Kaptanoglu (University of California, Berkeley)
-
09:55
-
Computational Frontier: Small Experiments 111 (JHN)
111
JHN
21E-
717
Welcome and IntroductionSpeakers: Benjamin Nachman (LBNL), Erica Snider (Fermilab)
-
718
Brief overview of white paper
https://arxiv.org/abs/2203.07645
Speaker: Maria Elena Monzani (SLAC National Accelerator Laboratory) -
719
CompF report overviewSpeakers: Benjamin Nachman (LBNL), Daniel Elvira (Fermilab), Steven Gottlieb (Indiana Univ.)
-
720
Discussion
-
717
-
Cross frontier sessions: NF-TF Neutrino theory network 175 (JHN)
175
JHN
22KA panel during the 22j session discussing the intersections of the AF and EF frontiers
- 721
- 722
-
723
Word from the DOE, Personal Experiences, Discussion
-
Instrumentation Frontier: Finalizing the Report with Community Input 075 (JHN)
075
JHN
30NConveners: Jinlong Zhang (ANL), Petra Merkel (Fermi National Accelerator Laboratory), Phillip Barbeau (Duke University)-
724
Detectors for e+e- collidersSpeakers: Ulrich Heintz, Ulrich Heintz (Brown University)
- 725
-
726
Roundtable with Topical Groups
Go over the feedback each group got on their report.
Go over new input from XF meetings and other information from community.
-
724
-
Underground Facilities Frontier: UF4 - Supporting Capabilities for Underground Research 022 (JHN)
022
JHN
21CConvener: Brianna Mount (Black Hills State University)-
727
UF4 - Supporting Capabilities for Underground Research
Presentation and live editing of the Supporting Capabilities for Underground Research (UF4) Topical Report.
Speaker: Brianna Mount (Black Hills State University)
-
727
-
Birds of a Feather: Communicating HEP to the public and the gov’t 110 (Kane Hall)
110
Kane Hall
36IOther meetings that make use of the fact we are all in one place!
-
728
Communicating HEP to the Public and GovernmentSpeakers: Kathryn Jepsen (Symmetry Magazine), Louise Suter (FNAL), Rob Fine, Rob Fine (University of Rochester)
-
728
-
Birds of a Feather: Townhall: International Benchmarking (HEPAP subpanel) 130 (Kane Hall)
130
Kane Hall
Other meetings that make use of the fact we are all in one place!
Conveners: Bonnie Fleming (Yale University), Patricia McBride (Fermilab)-
729
Townhall: International Benchmarking (HEPAP subpanel)
Members of the HEPAP Subpanel will be present to lead a short discussion of the panel's charge and to listen to your input.
Speakers: Bonnie Fleming (Yale University), Patricia McBride (Fermilab)
-
729
-
Afternoon Plenary: Physics on the Energy Frontier 130 (Kane Hall)
130
Kane Hall
21WConveners: Alessandro Tricoli (BNL), Laura Reina (Florida State University), Meenakshi Narain (Brown University)-
730
Energy Frontier Vision OverviewSpeaker: Alessandro Tricoli (BNL)
-
731
The Physics case for Higgs Factories - When and WhySpeaker: Sally Dawson (Brookhaven National Laboratoy)
-
732
The Physics case for Energy Frontier Multi-TeV colliders - When and WhySpeaker: Simone Pagan Griso (Lawrence Berkeley National Laboratory)
-
733
Questions and discussion
-
730
-
Afternoon Plenary: The Future of Computing for HEP 130 (Kane Hall)
130
Kane Hall
30OConveners: Benjamin Nachman (LBNL), Daniel Elvira (Fermilab), Steven Gottlieb (Indiana Univ.)-
734
IntroductionSpeakers: Benjamin Nachman (LBNL), Daniel Elvira (Fermilab), Steven Gottlieb (Indiana Univ.)
- 735
-
736
Questions/Discussion
-
737
Computing challenges and R&D to bridge the resource/need gap in the next 10-15 yearsSpeaker: Ken Bloom (University of Nebraska-Lincoln)
-
738
Questions/Discussion
-
739
Collaborative initiatives across experiment boundariesSpeaker: Elizabeth Sexton-Kennedy (FNAL)
-
740
Questions/Discussion
-
734
-
17:00
Coffee 225 and Lobby (Kane Hall)
225 and Lobby
Kane Hall
-
Afternoon Plenary: HEP/Quantum Science and Technology (QST) Intersections 130 (Kane Hall)
130
Kane Hall
23XConveners: Maria Spiropulu, Martin Savage (INT)-
741
HEP/QST Landscape
The landscape of QST/HEP intersections across academic/research institutions, including national and international laboratories and industry.
Speaker: Joseph Lykken (Fermilab) -
742
HEP & the language of entanglement
Quantum entanglement advancing HEP theory, experiment, and computation. Examples drawn from black holes and radiation.
Speaker: Geoffrey Penington (IAS/Princeton) -
743
National Quantum Initiative (NQI): 2018 - now
The status of the National Quantum Initiative launched by the DOE and other federal agencies in 2018.
Speaker: Paul Dabbar -
744
Panel Discussion
The panel will debate the status and envision the future of QST/HEP intersections and highlight the integration of quantum science and technology developments with the HEP apparatus, including building a quantum-ready workforce.
Topics that will be discussed include: 1) Codesign quantum experiments to advance and be advanced by the HEP mission as exemplified by the ongoing dark sector searches as well as other quantum gravity type of probes in AMO experiments in collaboration with HEP/QIS theorists. 2) The role of NQI centers and QC testbeds including SQMS for example, in advancing the HEP mission on fundamental physics while at the same time advancing Quantum Information Science and Technology systems at large. Status and achievements to-date, challenges and prospects as well as capability building. 3) The integration of Quantum Computing (hardware, software, hybrid architectures) into the laboratory, academic, research computing ecosystem. 4) Status and progress of quantum operating systems and architectures, and the growing partnerships between tech companies and researchers in HEP toward advancing the fundamental physics mission. How the HEP user-based scientific community can help tech companies by providing benchmarking and users of the quantum computing infrastructure. 5) Status and future of Quantum Simulations in HEP, the role and applications of AI/QML in HEP and HEP theoretical or experimental challenges and research that can advance quantum computing and QML tools.
Speakers: Aaron Chou (Fermilab), Anna Grassellino (Fermilab), Chiristian Bauer (LBNL), Krysta Svore (Microsoft), Monika Schleier-Smith (Stanford), Paul Dabbar (Columbia & BQT), Ravi Naik (Berkeley/LBNL), Shinjae Yoo (BNL), Travis Humble (Oak Ridge National Laboratory) -
745
Closing Remarks
The role and impact of fundamental science, specifically HEP, on the present and future quantum ecosystem.
Speaker: Carl Williams
-
741
-
Social: Colliderscope: Live music featuring oscilloscopes! Blue Moon Tavern
Blue Moon Tavern
712 NE 45th St, Seattle, WA 98105 50Bhttps://washington.zoom.us/j/98883066364?pwd=UjVOajdLMFpMQWVibUtsR010T1AzUT09
-
746
Colliderscope: Live music featuring oscilloscopes!Speaker: Lawrence Lee (University of Tennessee, Knoxville)
-
746
-
-
-
Accelerator Frontier: Future Colliders R&D Program Initiative 220 (Kane Hall)
220
Kane Hall
30PConveners: Pushpalatha Bhat (Fermilab), Sergei Nagaitsev (Fermilab/U.Chicago)-
747
National Accelerator R&D Program on Future CollidersSpeaker: Pushpa Bhat
-
748
GARD Thrusts/scope and Roadmaps (ABP, AAC, RF, MDP)
ABP (Sergei Nagaitsev), AAC (Mark Hogan), RF (Sergey Belomestnykh), MDP (Steve Gourlay) + discussion
Speakers: Sergei Nagaitsev (Fermilab/U.Chicago), Mark Hogan (SLAC), Sergey Belomestnykh (Fermilab), Steve Gourlay (LBNL) -
749
Examples of topics for Future Colliders R&D Program
ILC (Andy Lankford), FCC (Tor Raubenheimer), MC (Mark Palmer), C3/HELEN (Emilio Nanni), AAC (Cameron Geddes) +discussion
Speakers: Andrew Lankford (UC Irvine), Tor Raubenheimer (SLAC), Mark Palmer (Brookhaven National Laboratory), Emilio Nanni (SLAC National Accelerator Laboratory), Cameron Geddes (LBNL) -
750
International Efforts in Collider R&D
CERN/FCC (Frank Zimmermann), Japan/ILC (Shoji Asai), China/CepC (Xinchou Lou), INFN/MC (Nadia Pastrone)
+ discussion (15')Speakers: Frank Zimmermann (CERN), Shoji Asai (U. Tokyo), Xinchou LOU (University of Texas at Dallas/IHEP), Nadia Pastrone (INFN-Torino)
-
747
-
Cross frontier sessions: NF-CF-TF high energy and ultrahigh energy astrophysical neutrino 102 (JHN)
102
JHN
22NA panel during the 22j session discussing the intersections of the AF and EF frontiers
-
751
High-Energy and Ultra-High-Energy Neutrinos WhitepaperSpeaker: Mauricio Bustamante (Niels Bohr Institute, University of Copenhagen)
- 752
-
753
Tau Neutrinos in the next decade white paperSpeaker: Peter Denton (Brookhaven National Laboratory)
-
754
Forward physics facility and high energy neutrinosSpeaker: INA SARCEVIC (UNIVERSITY OF ARIZONA)
- 755
-
756
Main messages roundtableSpeakers: Erin O'Sullivan (Uppsala University), Ke Fang (University of Wisconsin-Madison)
-
751
-
Cross frontier sessions: RF-NF RF5 to discuss CLFV and neutrinos - mu2e and facilities 254 (MGH)
254
MGH
24AA panel during the 22j session discussing the intersections of the AF and EF frontiers
- 757
- 758
-
759
LFU and CLFVSpeaker: Chris Polly (Fermilab)
-
760
The ABCs of NSI: Probes of BSM Neutrino InteractionsSpeaker: Ian Shoemaker (Virginia Tech)
-
Instrumentation Frontier: Informal Writing 075 (JHN)
075
JHN
24DConveners: Jinlong Zhang (ANL), Petra Merkel (Fermi National Accelerator Laboratory), Phillip Barbeau (Duke University)-
761
work on report
-
761
-
Neutrino Physics Frontier: Beyond neutrino mass physics reach of precision beta-decay experiments 238 (MGH)
238
MGH
21KConveners: Bryce Littlejohn (Illinois Institute of Technology), Diana Parno (Carnegie Mellon University), Ian Shoemaker (Virginia Tech)-
762
Experimental overview of precision beta-decay measurementsSpeaker: Kyle Leach (Colorado School of Mines)
- 763
-
764
Overview of sterile-neutrino sensitivity in beta-spectrum measurementsSpeaker: Pranava Teja Surukuchi (Yale University)
-
765
Further discussion
-
762
-
Neutrino Physics Frontier: Community Engagement Success Stories 026 (JHN)
026
JHN
22IConvener: Elizabeth Worcester (BNL)-
766
SURF Outreach and Community RelationsSpeaker: Mike Headley (SDSTA - SURF)
- 767
- 768
- 769
- 770
-
771
Discussion
-
766
-
Neutrino Physics Frontier: New Opportunities in Neutrinos (Early Career Presentations) 022 (JHN)
022
JHN
20HConveners: Jacob Zettlemoyer (Fermilab), Tanaz Mohayai (Fermilab)-
772
Low-energy neutrino physics at TheiaSpeaker: Zara Bagdasarian (University of California Berkeley)
- 773
-
774
Accelerator Neutrino Oscillation Experiments: This Generation and NextSpeaker: Kevin Wood (Lawrence Berkeley National Laboratory)
-
775
Physics at the MeV-Scale in LArTPCsSpeaker: William Foreman (Illinois Institute of Technology)
-
776
Low Energy Physics Program of DUNESpeaker: Thiago Sogo Bezerra (University of Sussex)
-
777
Doped Liquid Argon TPCs as a Neutrinoless Double Beta Decay PlatformSpeaker: Fernanda Psihas Olmedo (Fermi National Accelerator Laboratory)
-
772
-
Neutrino Physics Frontier: The Future is Now (Early Career Presentations) 175 (JHN)
175
JHN
20JConveners: Jacob Zettlemoyer (Fermilab), Samuel Hedges (Duke University)-
778
Mobile Antineutrino Demonstrator projectSpeaker: Olga Kyzylova (Virginia Tech)
-
779
Design of novel plastic scintillator technologies for neutrino detection at LLNLSpeaker: Cristian Roca (LLNL)
-
780
EOS: A tonne-scale testbed for hybrid neutrino detectorsSpeaker: Tanner Kaptanoglu (University of California, Berkeley)
-
781
Enhanced Particle Identification in Water-based Liquid ScintillatorSpeaker: Tomi Akindele (Lawrence Livermore National Laboratory)
-
782
CUPID, CUPID-1T, and the DEMETER demonstratorSpeaker: Erin Hansen
-
778
-
Theory Frontier: Discussion and frontier reports 110 (Kane Hall)
110
Kane Hall
19PConveners: Aida El-Khadra (University of Illinois at Urbana-Champaign), Csaba Csaki (Cornell University), Nathaniel Craig (UC Santa Barbara) -
Underground Facilities Frontier: UF6 - Underground Facilities Gaps & Needs 242 (MGH)
242
MGH
23B -
Birds of a Feather: COVID Roundtable (lessons (to be) learned) 210 (Kane Hall)
210
Kane Hall
36JOther meetings that make use of the fact we are all in one place!
- 783
-
Afternoon Plenary: Snowmass Early Career 130 (Kane Hall)
130
Kane Hall
24SConveners: Garvita Agarwal, Jacob Zettlemoyer (Fermilab)- 784
-
785
SEC Survey: Introduction and MethodsSpeaker: Erin Conley (Duke University)
- 786
-
787
SEC Survey: Physics Outlook FindingsSpeaker: Joshua Barrow
-
788
Early Career Organizations in HEPSpeaker: Fernanda Psihas Olmedo (Fermi National Accelerator Laboratory)
-
Afternoon Plenary: CPAD: Careers and Collaborations in Detector Instrumentation 120 (Kane Hall)
120
Kane Hall
30RConveners: Karsten Heeger (Yale University), Petra Merkel (Fermi National Accelerator Laboratory)-
789
Development and production of high-performance water based liquid scintillators for particle physics experimentsSpeaker: Minfang Yeh (Brookhaven National Laboratory)
-
790
Development of novel low-cost, large-area lithium-drifted silicon detectorsSpeaker: Kerstin Perez (Massachusetts Institute of Technology)
-
791
MKID Development for Measurement of the Cosmic Microwave BackgroundSpeaker: Karia Dibert (University of Chicago)
-
792
Development of Deep Junction Low Gain Avalanche Diodes for high Granularity Timing DetectorsSpeaker: Yuzhan Zhao (University of California, Santa Cruz, SCIPP)
-
793
Panel on workforce development, collaboration with industry and cross cutting technologies with outside HEPSpeakers: Dan Dwyer (LBNL), Gabriella Carini (Brookhaven National Laboratory), Helmut Marsiske (Office of High Energy Physics, U.S. Department of Energy), Ian Shipsey (Oxford), Marina Artuso (syracuse university), Reina Maruyama (Yale University)
-
789
-
Afternoon Plenary: Communicating Science to Everyone 130 (Kane Hall)
130
Kane Hall
30QConvener: Kathryn Jepsen (Symmetry Magazine)-
794
Introduction
-
795
Remarks by Dr. Lucianne Walkowicz
Dr. Lucianne Walkowicz is an astronomer who has organized Ask a Scientist events on public transportation in New York City and Chicago and theme events such as A Night in the Afrofuture at Adler Planetarium in Chicago. (participating virtually)
-
796
Remarks by Dr. Jessica Esquivel
Dr. Jessica Esquivel is a Fermilab physicist who has organized events such as Wakandacon, an Afrofuturist comic convention in Chicago. (participating in person)
-
797
Remarks by Dr. Xinnan Du
Dr. Xinnan Du is an outreach & engagement manager at KIPAC, who had organized bilingual virtual events for students and their parents around UC Riverside. (participating in person)
-
798
Renarks by Dr. Desire Whitmore
Dr. Whitmore is a spectroscopist and staff physics educator who has organized events in partnership with Latinx organizations and who helps run a program for transgender youth at the Explortatorium science museum in San Francisco. (participating virtually)
-
799
Panel Discussion
-
794
-
17:00
Coffee 225 and Lobby (Kane Hall)
225 and Lobby
Kane Hall
-
Afternoon Plenary: DOE Multiprogram Laboratories: their HEP programs and intersections with other disciplines”. 120 (Kane Hall)
120
Kane Hall
24UConvener: Chris Quigg (Fermilab)- 800
- 801
- 802
-
803
Report from Lawrence Berkeley National LaboratorySpeakers: Natalie Roe, Natalie Roe (Lawrence Berkeley National Lab)
- 804
-
805
Perspective of DOE Nuclear PhysicsSpeaker: Paul Sorensen (Department of Energy)
-
806
Discussion
-
-
-
Physics Highlights from the Frontiers 130 (Kane Hall)
130
Kane Hall
25Bdescription here
Convener: Marcela Carena (Fermilab)-
807
Frontier Summaries and Panel Discussion: Science Highlights
In this discussion, each of the Frontiers gives a summary of the physics highlights / Big ideas, which defines their vision for 2025-2035 and 10 years after 2035. These physics highlights will followed by a summary on experiments proposed to investigate them and their proposed timelines (timelines=R&D, construction and data collection). Each Frontier will also comment on the mapping of their science on the current P5 science drivers drivers. The collective physics highlights from all Frontiers may reaffirm the P5 science drivers or a need to extend them.
- 808
- 809
- 810
- 811
-
812
Rare Processes and Precision Measurements FrontierSpeaker: Marina Artuso (syracuse university)
-
813
Theory FrontierSpeaker: Aida El-Khadra (University of Illinois at Urbana-Champaign)
-
814
Questions and discussion
-
807
-
09:45
Coffee Break
-
Enabling the Physics Goals: Enabling Science
Frontiers: AF, CEF, COMPF, IF, TF, UF
Title: Enabling the Physics Goals
Abstract: Each Frontier describes briefly a) their goals and priorities; b) critical R&D or infrastructure needed during 2025-2035 to support and enable the physics vision discussed during panel on physics highlights and how they may benefit from targeted funding; and c) R&D or infrastructure needs to support the proposed physics measurements in 2035+ and may be developed by next P5. Each Frontier will comment on the related P5 science drivers and also if any of their goals do not map on the P5 science drivers.-
815
IntroductionSpeakers: Ian Shipsey (Purdue University), Ian Shipsey (Oxford), Ian Shipsey (Oxford)
- 816
- 817
- 818
-
819
Inrstrumentation FrontierSpeaker: Petra Merkel (Fermi National Accelerator Laboratory)
- 820
- 821
-
822
Questions and discussion
-
815
-
Social: Conference Picture Red Square
Red Square
50Chttps://washington.zoom.us/j/98883066364?pwd=UjVOajdLMFpMQWVibUtsR010T1AzUT09
-
Birds of a Feather: Early-Career Feedback 130 (Kane Hall)
130
Kane Hall
Other meetings that make use of the fact we are all in one place!
Conveners: Breese Quinn (University of Mississippi), Fernanda Psihas Olmedo (Fermi National Accelerator Laboratory), Rob Fine (University of Rochester), Rob Fine-
823
Early Career FeedbackSpeakers: Breese Quinn (University of Mississippi), Fernanda Psihas Olmedo (Fermi National Accelerator Laboratory), Julia Gonski (Columbia University), Rob Fine (University of Rochester), Rob Fine
-
823
-
Physics Highlights from the Frontiers: Poster Session Awards!!!!!
description here
Convener: Jason Detwiler- 824
-
Physics Highlights from the Frontiers: Intersections between Particle Physics and Associated Fields 130 (Kane Hall)
130
Kane Hall
25Cdescription here
Conveners: Glennys Farrar (NYU), Priscilla Cushman (University of Minnesota), Yury Kolomensky (LBNL)-
825
Intersections with AstrophysicsSpeaker: Will Farr (Stony Brook / CCA)
-
826
Intersections with Nuclear PhysicsSpeaker: David Hertzog
-
827
Intersections with BES: material science, atomic and molecular structure, new technology toolsSpeaker: Peter Denes (LBNL)
-
825
-
15:30
Coffee 225 and Lobby (Kane Hall)
225 and Lobby
Kane Hall
-
Physics Highlights from the Frontiers: National & International Laboratory Plans 130 (Kane Hall)
130
Kane Hall
30Tdescription here
-
828
IntroductionSpeaker: Jonathan Bagger (Johns Hopkins University)
-
829
CERN PerspectiveSpeakers: Fabiola Gianotti (CERN), Fabiola Gianotti (CERN)
-
830
Fermilab PerspectiveSpeakers: Lia Merminga (TRIUMF), Lia Merminga (FNAL)
- 831
-
832
KEK PerspectiveSpeakers: Masa Yamauchi (KEK), Masanori Yamauchi (KEK), Masanori Yamauchi (KEK)
-
833
Questions and discussion
-
828
-
Physics Highlights from the Frontiers: Examples of International and National Status and Plans 130 (Kane Hall)
130
Kane Hall
30Udescription here
-
834
View from the CERN CouncilSpeaker: Eliezer Rabinovici (Hebrew University)
-
835
Particle Physics in Latin AmericaSpeaker: Fernando Quevedo
- 836
-
837
View from ICFASpeaker: Stuart Henderson (Thomas Jefferson National Accelerator Facility)
-
838
HEP in AfricaSpeaker: Ketevi Adikle Assamagan (Brookhaven National Laboratory)
- 839
-
840
Questions and discussion
-
834
-
Social: Mariner's Baseball Night Mariner's Baseball Stadium
Mariner's Baseball Stadium
50Ahttps://washington.zoom.us/j/98883066364?pwd=UjVOajdLMFpMQWVibUtsR010T1AzUT09
-
-
-
Physics Highlights from the Frontiers: Summary, Part 2 130 (Kane Hall)
130
Kane Hall
26Bdescription here
-
841
International Benchmarking SubpanelSpeakers: Bonnie Fleming (Yale University), Patricia McBride (Fermilab)
-
842
National Academy Study (EPP2020) - Elementary Particle Physics: Progress and PromiseSpeakers: Maria Spiropulu (California Institute of Technology), Maria Spiropulu, Maria Spiropulu (California Institute of Technology), Maria Spiropulu (California Institute of Technology), Maria Spiropulu (California Institute of Technology)
-
843
Large Experiments/Facilities and the proposed timelines
-
a) Energy FrontierSpeaker: Meenakshi Narain (Brown University)
-
b) Cosmic FrontierSpeaker: Marcelle Soares-Santos (Fermilab)
-
c) Neutrino FrontierSpeaker: Stephen Brice (FNAL)
-
d) Rare Prcesses and Precision Measurements FrontierSpeaker: Alexey Petrov (Wayne State University)
-
e) Accelerator FrontierSpeakers: Tor Raubenheimer (SLAC), Tor Raubenheimer (SLAC)
-
g) Questions and discussion
-
-
844
Message from DOE Office of Science etc.
-
10:05
Coffee Break
-
845
Mid and Small scale Experiments/Facilities and the proposed timelines
-
a) Cosmic FrontierSpeakers: Aaron Chou (Fermi National Accelerator Laboratory), Aaron Chou (Fermilab)
-
b) Neutrino FrontierSpeaker: Mayly Sanchez (Iowa State University)
-
c) Rare Processes and Precision MeasurementsSpeaker: Robert Bernstein (Fermilab)
-
f) Instrumentation FrontierSpeakers: Jinlong Zhang (ANL), Jinlong Zhang (ANL)
-
-
846
Community Summer Study and Workshop SynthesisSpeakers: Priscilla Cushman (University of Minnesota), Priscilla Cushman (University of Minnesota)
- 847
-
848
Remarks and Thanks from DPF Chair and the UW OrganizersSpeakers: Gordon Watts (University of Washington), Joel Butler (Fermilab)
-
841
-