10-11 June 2019
Fermi National Accelerator Laboratory
US/Central timezone
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Contribution List

Displaying 59 contributions out of 59
Type: Oral Session: Monday Afternoon I
SBND is a Liquid Argon Time Projection Chamber (LArTPC) experiment and the near detector in the Short Baseline Neutrino (SBN) program at Fermilab. With a 110 m baseline and a 112 tonne active mass, the detector will observe ~5,000,000 charged current muon neutrino ($\nu_{\mu}$ CC) interactions at energies of <$E_{\nu}$> $\sim$ 650 MeV in its 6.6 $\times 10^{20}$ POT (3 year) exposure. SBND will co ... More
Presented by Rhiannon JONES on 10 Jun 2019 at 3:30 PM
Type: Oral Session: Monday Afternoon II
The Accelerator Neutrino Neutron Interaction Experiment (ANNIE) is a gadolinium-doped water Cherenkov detector located in the Fermilab Booster Neutrino Beam line. Many long-baseline neutrino measurements rely on efficient reconstruction of charged-current quasi-elastic (CCQE) neutrino interactions, whose final-state particles include only the recoiling nucleus, a proton, and an outgoing lepton. O ... More
Presented by Teal PERSHING on 10 Jun 2019 at 5:15 PM
Type: Oral Session: Monday Afternoon II
The Accelerator Neutrino Neutron Interaction Experiment (ANNIE) is a gadolinium-loaded water Cherenkov detector located on the Booster Neutrino Beam at Fermilab. The experiment seeks to better understand neutrino-nucleus interactions by studying the number of final state neutrons produced in charged current interactions. It will be the first experiment testing Large Area Picosecond Photodetectors ... More
Presented by Dr. Emrah TIRAS on 10 Jun 2019 at 5:30 PM
Type: Oral Session: Tuesday Afternoon II
Despite that the Standard Model has been put through many stringent tests, it still can not be the full picture of particle physics. In this short talk, we give an overview of the motivations to go beyond the Standard Model and discuss a few plausible scenarios in its extension.
Presented by Yang GAO on 11 Jun 2019 at 4:30 PM
The LHC is the worlds highest energy proton-proton collider with a center-of-mass energy of 13 TeV. The world's largest machine is currently running at twice its designed luminosity and represents forefront of the energy frontier. The CMS detector is a multipurpose detector that features a 4 Tesla magnet and over a 100 million active channels taking data every 25 ns. It, along with its sister expe ... More
Presented by Cristina Ana MANTILLA SUAREZ on 11 Jun 2019 at 9:00 AM
Type: Oral Session: Monday Afternoon I
MicroBooNE is a short baseline neutrino oscillation experiment based at Fermilab that employs a Liquid Argon Time Projection Chamber (LArTPC) to investigate the excess of low energy events observed by MiniBooNE, study neutrino-argon cross-sections, and perform detector R&D for future LArTPC experiments. The MicroBooNE detector lies along the Booster Neutrino Beamline, which produces neutrinos with ... More
Presented by Polina ABRATENKO on 10 Jun 2019 at 2:45 PM
Presented by Michael WALLBANK on 11 Jun 2019 at 5:45 PM
Type: Oral Session: Tuesday Morning II
The Deep Underground Neutrino Experiment (DUNE) is an international long-baseline neutrino experiment. DUNE will consist of an intense neutrino beam produced at Fermi National Accelerator Laboratory in Batavia, Illinois. The far detector will comprise of four Liquid Argon Time Projection Chambers (LArTPC) holding in total around 40 ktons of fiducial mass and will be placed at the Sanford Undergro ... More
Presented by Mrs. Maura SPANU on 11 Jun 2019 at 12:00 PM
Type: Oral Session: Monday Afternoon II
As the SBN far-detector, the ICARUS T600, a set of liquid argon time-projection chambers (TPC), will operate at shallow depth and therefore be exposed to the full surface flux of cosmic rays. This poses a problematic background to the neutrino oscillation search, especially photons produced by muons passing in close proximity to, but not through, the active volume. A direct way to reject this back ... More
Presented by Mr. Christopher HILGENBERG on 10 Jun 2019 at 4:15 PM
Type: Oral Session: Tuesday Afternoon I
NOvA is a long baseline neutrino experiment based at Fermilab that studies neutrino oscillation parameters via electron neutrino appearance and muon neutrino disappearance. The oscillation measurements compare the Far Detector data to an oscillated prediction which accounts for the Near Detector (ND) data and our understanding of neutrino interactions and cross-sections by using GENIE simulation. ... More
Presented by Maria MARTINEZ-CASALES on 11 Jun 2019 at 3:35 PM
Type: Oral Session: Monday Morning I
The Dark Energy Survey (DES) is a deep, wide-area optical imaging survey in the southern hemisphere. The unprecedented photometry from DES has allowed for exciting science results on topics ranging from cosmology to our Galaxy. I will discuss details of the survey -- which completed its 5.5-year observations in January 2019 -- and highlight some recent science results from the collaboration.
Presented by Nora SHIPP on 10 Jun 2019 at 9:10 AM
Type: Oral Session: Tuesday Morning II
A brief talk on the updates and technical details of DUNE in a concentrated format.
Presented by Richard DIURBA on 11 Jun 2019 at 11:45 AM
Type: Oral Session: Monday Morning II
A large dynamical-range diagnostics (LDRD) design at Jefferson Lab will be used at the FAST-IOTA injector to measure the transverse distribution of halo associated with a high-charge electron beam. One important aspect of this work is to explore the halo distribution when the beam has significant angular momentum (i.e. is magnetized). The beam distribution is measured by recording radiation produc ... More
Presented by Mr. Christopher MARSHALL on 10 Jun 2019 at 11:30 AM
Type: Oral Session: Tuesday Afternoon II
The Mu2e experiment at Fermilab will search for the charged-lepton flavour violating neutrino-less conversion of a negative muon into an electron in the field of an aluminum nucleus. The Mu2e detector is composed of a tracker and an electromagnetic calorimeter and an external veto for cosmic rays. The calorimeter plays an important role in providing excellent particle identification capabilitie ... More
Presented by Dr. Raffaella DONGHIA on 11 Jun 2019 at 5:30 PM
Type: Oral Session: Monday Morning I
Charge Coupled Devices and MKIDs are pixelated imaging sensors used for astronomy. FNAL in involved in the development of instruments using these sensors. I will describe the development of a novel micro-mirror array projector for the characterization of these imaging sensors. The CCD require tight control of the light intensity and the exposure time, and the micromirror array allow to also contro ... More
Presented by Brody OLESON on 10 Jun 2019 at 9:55 AM
Type: Oral Session: Monday Morning II
E1039/SpinQuest is the first transversally-polarized Drell-Yan experiment at Fermilab. SpinQuest data-taking is anticipated to begin this coming fall 2019. In SpinQuest, a transversely-polarized NH3 or ND3 target is employed with the unpolarized 120-GeV extracted proton beam from Fermilab Main Injector to obtain various measurements of transverse single spin asymmetries in J/psi, psi’, lambda, d ... More
Presented by Dr. Chun-Min JEN on 10 Jun 2019 at 12:00 PM
Type: Oral Session: Monday Afternoon II
Elastic neutrino-electron scattering provides an important tool for normalizing neutrino flux in modern experiments. This process is subject to large radiative corrections. We determine the Fermi effective theory performing the one-loop matching to the Standard model at the electroweak scale with subsequent running down to GeV scale. Based on this theory, we analytically evaluate virtual correcti ... More
Presented by Oleksandr TOMALAK on 10 Jun 2019 at 4:45 PM
Presented by Dr. Deepika JENA on 11 Jun 2019 at 2:00 PM
Type: Oral Session: Monday Afternoon II
We propose a low-cost and movable setup to probe minicharged particles (or milli-charged particles) using high-intensity proton fixed-target facilities. This proposal, FerMINI, consists of a milliQan-type detector, requiring multi-coincident (nominally, triple-coincident) scintillation signatures within a small time window, located downstream of the proton target of a neutrino experiment. During t ... More
Presented by Dr. Yu-Dai TSAI on 10 Jun 2019 at 6:00 PM
Type: Oral Session: Monday Morning II
The SpinQuest collaboration will measure the sea quark Sivers asymmetry using Drell-Yan production from the 120 GeV proton beam of the Fermilab Main Injector incident on transversely polarized proton and deuteron targets. Measuring a nonzero Sivers asymmetry would provide strong evidence for nonzero orbital angular momentum of sea quarks. The use of both polarized hydrogen and deuterium targets wi ... More
Presented by Joshua HOSKINS on 10 Jun 2019 at 11:45 AM
Type: Oral Session: Monday Morning I
This project was realized primarily to test and improve the spatial tracking resolution of the ANL (Argonne National Laboratory) telescope consisting of the ATLAS IBL silicon pixel sensors and FE-I4 chips by making use of the test beam at Fermilab. In this paper, we will discuss the overall performance of the modules and how it can be improved. We will also discuss efforts made to improve the spat ... More
Presented by Spoorthi NAGASAMUDRAM on 10 Jun 2019 at 10:25 AM
Type: Oral Session: Monday Afternoon II
Liquid Argon Time Projection Chambers (LArTPCs) are currently being used extensively for neutrino physics due to their excellent capabilities in performing particle identification, and precise 3D and calorimetric energy reconstruction. The Liquid Argon In A Test Beam (LArIAT) experiment was located at the Test Beam Facility where it was exposed to a known charged particle beam. The capability of ... More
Presented by Vincent BASQUE on 10 Jun 2019 at 4:30 PM
Type: Oral Session: Tuesday Morning I
In this talk I summarize the current status of the field in lattice QCD. My goal will be to provide an accessible overview. I will emphasize work done at Fermilab and work affecting Fermilab experiments.
Presented by William JAY on 11 Jun 2019 at 9:30 AM
Type: Oral Session: Tuesday Morning I
The CMS Muon group has proposed the use of Gas Electron Multiplier (GEM) technology to maintain an efficient and reliable operation during the High Luminosity phase of the LHC (HL-LHC). This is particularly important to study many physics processes with muons in the final state. The CMS GEM chambers will cover eta region 1.6 to 2.2 of the endcap. We report on the GE1/1 layout and their performance ... More
Presented by Mr. Aashaq SHAH on 11 Jun 2019 at 10:00 AM
Type: Oral Session: Monday Afternoon II
Based in the NuMI beamline at Fermi National Laboratory, the on-axis MINERvA experiment is focused on reaching precision measurements of neutrino and antineutrino interactions in diverse nuclei materials for energies up to 50 GeV. The results support the current and future oscillation experiments as well as to provide information about the structure of nuclei. A look at the latest results from the ... More
Presented by Ms. Barbara YAEGGY on 10 Jun 2019 at 5:00 PM
Type: Oral Session: Monday Morning I
Dark matter halos are the fundamental building blocks of cosmic large-scale structure. Improving our theoretical understanding of their structure, evolution and formation is an essential step towards understanding how galaxies form, which in turn will allow us to fully exploit the large amount of data from future galaxy surveys. I will present a machine learning approach which aims to provide new ... More
Presented by Ms. Luisa LUCIE-SMITH on 10 Jun 2019 at 10:10 AM
Type: Oral Session: Tuesday Morning II
The Deep Underground Neutrino Experiment (DUNE) is a leading-edge experiment for neutrino science and proton decay studies. The single-phase liquid argon prototype detector at CERN is a crucial milestone for the DUNE that will inform the construction and operation of the far detector modules. In this talk, I will present the current status of reconstructing Michel electrons from cosmic-ray muons i ... More
Presented by Dr. Aleena RAFIQUE on 11 Jun 2019 at 12:15 PM
Type: Oral Session: Monday Afternoon I
MicroBooNE is one of three liquid argon time projection chambers (LArTPCs) making up the Short-Baseline Neutrino Program at FNAL. Located on the Booster Neutrino Beamline, MicroBooNE has been collecting data since October 2015 to determine the source of the low-energy electromagnetic event excess previously reported by MiniBooNE and LSND. In addition to its signature analysis, MicroBooNE is employ ... More
Presented by Ms. Katrina MILLER on 10 Jun 2019 at 2:00 PM
Type: Oral Session: Tuesday Afternoon II
The discovery of neutrino oscillation manifests the violation of lepton number conservation. It further indicates Charged Lepton Flavor Violation (CLFV) is not explicitly forbidden in the Standard Model (SM), although it is dynamically suppressed which remain unobserved. Many well-motivated physics models predict rates for CLFV processes that are within a few orders of magnitude of the current exp ... More
Presented by Yujing SUN on 11 Jun 2019 at 5:15 PM
Type: Oral Session: Tuesday Afternoon II
The Muon $g-2$ Experiment (E989) is measuring the magnetic anomaly, $a_\mu$, of the muon to 140 parts per billion (ppb) to resolve the outstanding discrepancy between the value predicted by the Standard Model and the best measurement to date. The magnetic anomaly receives contributions from loops of any particle type in the muon-photon vertex, so a discrepancy between theory and experiment is a st ... More
Presented by Jason HEMPSTEAD on 11 Jun 2019 at 4:45 PM
Type: Oral Session: Tuesday Afternoon I
The long-baseline neutrino oscillation experiment named NOvA is comprised of two detectors utilizing liquid scintillator tracking calorimeters. Both are positioned 14 mrad off-axis with respect to the NuMI beam with the near detector being at Fermilab. The far detector, at 14 kton, can be found approximately 810 km away in Ash River, Minnesota. The main physics goals of NOvA include, but are not l ... More
Presented by Miranda ELKINS on 11 Jun 2019 at 2:20 PM
Type: Oral Session: Tuesday Afternoon I
NOvA continues as one of the leading long-baseline neutrino experiments, thanks to Fermilab's powerful 700 kW NuMI beam, which provides NOvA with a beam of predominantly muon neutrinos or antineutrinos. NOvA studies neutrino oscillations using two detectors, both constructed from plastic extrusions filled with liquid scintillator, placed 810 km apart and both slightly off-axis from the beam c ... More
Presented by Dr. Ashley BACK on 11 Jun 2019 at 3:05 PM
Type: Oral Session: Tuesday Afternoon I
NOvA is a long-baseline neutrino experiment with two functionally identical liquid scintillator detectors 809 km apart, off-axis from the NuMI beam. The main goal of this experiment is to determine the mass hierarchy and precise measurement of several neutrino oscillation parameters. To measure these parameters precisely we need to have a correct estimate of the neutrino and antineutrino compositi ... More
Presented by Mr. abhilash DOMBARA on 11 Jun 2019 at 3:20 PM
Type: Oral Session: Tuesday Afternoon I
Deep learning has aided the NOvA experiment in selection of NuMI beam neutrino events. Low statistics makes enhancements in signal efficiency especially critical to the success of the NOvA analysis. Use of convolutional neural networks (CNNs) for event and particle identification has led to significant gains in signal efficiency for neutrino event selection while also reducing the complexity of th ... More
Presented by Grant NIKSERESHT on 11 Jun 2019 at 2:50 PM
Type: Oral Session: Monday Afternoon I
I will discuss the current state of neutrino theory work, specifically focusing on how we interface with interpretations of current experiments and predictions for upcoming experiments. I will discuss ideas that Fermilab theorists are currently exploring regarding the experimental neutrino program at Fermilab, from the SBN experiments to DUNE.
Presented by Kevin KELLY on 10 Jun 2019 at 1:45 PM
Type: Oral Session: Tuesday Afternoon I
Muon monitors are a very important diagnostic tool for the NOvA experiment at Fermilab. With the MINOS experiment decommissioned, MM are the only detectors to indicate and help mitigate the issues with the NuMI beam. The goal of our study is to maintain the quality of the MM signal and to establish the neutrino beam profile and MM signal correlations. This study could also inform the LBNF decision ... More
Presented by Yiding YU on 11 Jun 2019 at 2:35 PM
Type: Oral Session: Tuesday Morning II
The expected precision of current long-baseline neutrino oscillation experiments (T2K, NO$\nu$A) will be limited by uncertainties in neutrino interaction models in addition to sample statistics. The interaction uncertainties will also play a significant role in next-generation experiments (DUNE, Hyper-K), which aim to collect much larger samples of oscillated neutrinos. Without significant advance ... More
Presented by Dr. Luke PICKERING on 11 Jun 2019 at 12:30 PM
Type: Oral Session: Monday Afternoon I
The Short-Baseline Near Detector (SBND) will be one of three liquid argon neutrino detectors sitting in the Booster Neutrino Beam (BNB) at Fermilab as part of the Short-Baseline Neutrino (SBN) Program. SBND is a 112-ton active mass liquid argon time projection chamber (LArTPC) to be located only 110 m from the BNB neutrino source. An important aspect of LArTPC detector design is that the readout a ... More
Presented by Ryan LAZUR on 10 Jun 2019 at 3:15 PM
Type: Oral Session: Tuesday Morning I
A brief overview of perturbative QCD and its role in precision measurements at the LHC. There will be a focus on efforts that are being done here at Fermilab. Here at Fermilab, the QCD group focuses on three distinct topics. Therefore, the talk will focus on the importance of improving precision for measurements at the LHC, through the use of higher order corrections, analytic resummation, and par ... More
Presented by Joshua ISAACSON on 11 Jun 2019 at 9:15 AM
Type: Oral Session: Tuesday Afternoon II
The Muon g-2 experiment at Fermilab (E989) aims to measure the anomalous magnetic moment of the muon, $a_{\mu}$, to a precision of $140$ ppb, a four-fold increase in precision over the previous experiment at Brookhaven National Laboratory (BNL). The value of $a_{\mu}$ from BNL currently differs from the Standard Model prediction by $\sim 3.5$ standard deviations or higher, suggesting the potential ... More
Presented by Ms. Meghna BHATTACHARYA on 11 Jun 2019 at 5:00 PM
Type: Oral Session: Monday Morning II
This study is focused on the development of an in-situ plasma cleaning procedure for 1.3GHz 9-cell TESLA shaped SRF cavities. The goal of this technique is to reduce field emission through the removal of adsorbed hydrocarbons that lower the work function of the cavity surface. In this work I present the first results of plasma processing applied to LCLS-II cavities focusing on plasma ignition an ... More
Presented by Bianca GIACCONE on 10 Jun 2019 at 11:00 AM
Type: Oral Session: Monday Afternoon I
Next generation neutrino oscillation experiments aim towards high-precision extraction of oscillation parameters, which in turn requires an unprecedented understanding of neutrino-nucleus interactions. Neutrino processes producing a charged lepton and a single intact nucleon in the final state can offer an important window into the dynamics of neutrino interactions with direct importance for ac ... More
Presented by Ms. Afroditi PAPADOPOULOU on 10 Jun 2019 at 2:15 PM
Type: Oral Session: Tuesday Morning I
Clustering of charged particle tracks along the beam axis is the first step in reconstructing the positions of proton-proton (p-p) collisions at Large Hadron Collider (LHC) experiments. In this talk, we formulate this problem for a 2048 qubit D-Wave quantum computer that works by quantum annealing. We show the performance of the quantum annealer on artificial events generated from p-p collision an ... More
Presented by Andrew WILDRIDGE, Souvik DAS, Mr. Sachin VAIDYA on 11 Jun 2019 at 10:15 AM
Type: Oral Session: Monday Afternoon I
The Short-Baseline Near Detector (SBND) will be a 112 ton liquid argon time projection chamber devoted to researching neutrino oscillations. Located 110 m downstream from the Booster Neutrino Beam (BNB) target, SBND will be the near detector of the three-detector Short Baseline Neutrino (SBN) program at Fermilab. The SBN program will probe neutrino oscillations at the $\sim \! 1 \textrm{eV}^2$ sca ... More
Presented by Iker DE ICAZA ASTIZ on 10 Jun 2019 at 3:00 PM
Type: Oral Session: Tuesday Morning I
The CMS Phase II upgrade, High Granularity Calorimeter (HGCal) will have fine transverse and longitudinal segmentation to allow for superior particle identification and pileup rejection in the high radiation and large event pileup environment of the endcap region. A significant portion of the hadronic portion of the HGCal will be instrumented with scintillator tiles directly coupled to Silicon Pho ... More
Presented by Ramanpreet SINGH on 11 Jun 2019 at 9:45 AM
Type: Oral Session: Tuesday Morning II
In traditional searches for physics beyond the standard model, a requirement of high missing transverse momentum (MET) is often used. However, without any signs of significant deviations from the standard model expectations, we decided to relax this requirement for the search reported in this talk. Many new physics models, including versions of supersymmetry (SUSY) characterized by R-parity violat ... More
Presented by Christopher MADRID on 11 Jun 2019 at 11:15 AM
Type: Oral Session: Tuesday Morning II
Searches for dark matter in the past two decades have largely focused on Weakly Interacting Massive Particles (WIMPs). But what if instead of just one type of dark matter particle, there exists a richer dark sector hidden from ordinary view? This opens up a whole new paradigm for dark matter searches, allowing us to focus not only on the coupling between dark matter and the Standard Model, but als ... More
Presented by Andre STERENBERG FRANKENTHAL on 11 Jun 2019 at 11:30 AM
Type: Oral Session: Tuesday Morning II
Most theories that predict dark matter production at colliders rely on weakly coupled dark matter and the existence of WIMPs, or weakly interacting massive particles; however, there can be dark matter signatures in colliders that emerge from strongly coupled dark matter. These signatures are varied, ranging from emerging jets to Stealth Dark Matter. Another possible signature is semi-visible jets. ... More
Presented by Colin FALLON on 11 Jun 2019 at 11:00 AM
Type: Oral Session: Monday Morning I
The Milky Way satellites are among the least luminous and most dark matter-dominated galaxies in the known universe. I present on a search for low-luminosity dwarf galaxy companions of the Milky Way in three years of data from the Dark Energy Survey (DES) and the Panoramic Survey Telescope and Rapid Response System (Pan-STARRS PS1). Together, these two surveys cover roughly three-quarters of the s ... More
Presented by Sidney MAU on 10 Jun 2019 at 9:25 AM
Type: Oral Session: Tuesday Morning II
ProtoDUNE-SP, the prototype of the single-phase DUNE far detector, is constructed and operated at the CERN Neutrino Platform with total liquid argon (LAr) mass of 0.77 kt and using full-scale components of the design for DUNE. The physics program of protoDUNE-SP aims to understand and control the systematic uncertainties for future oscillation measurements at DUNE, the charged-particle beam test a ... More
Presented by Carlos SARASTY SEGURA
Type: Oral Session: Monday Morning II
The Muon Campus at Fermilab presently houses two experiments that aim to find discrepancies (if any) in the Standard Model. The Delivery Ring is a 500m circumference storage ring which is used to deliver protons to muon experiments Muon g-2 and Mu2e. Although these experiments are based on the same particle, they require different intensities because of their detector constraints. For the Mu2e cas ... More
Presented by Mr. Prudhvi Raj Varma CHINTALAPATI on 10 Jun 2019 at 11:15 AM
Type: Oral Session: Monday Morning I
Modern cosmic sky surveys (e.g., CMB S4, DES, LSST) collect a complex diversity of astronomical objects. Each of class of objects presents different requirements for observation time and sensitivity. For determining the best sequence of exposures for mapping the sky systematically, conventional scheduling methods do not optimize the use of survey time and resources. We present an alternative sched ... More
Presented by Mr. Andres Felipe ALBA HERNANDEZ
Type: Oral Session: Monday Morning I
Strong gravitational lenses are cosmic magnifying glasses that can be used as a probe of cosmic phenomena, like dark energy and dark matter. However, strong lensing systems are rare and complex, which means they are both hard to find and analyze. We present two important results in strong lensing science: 1) new deep learning techniques for finding and measuring strong lenses; and 2) dark energy f ... More
Presented by Jason POH on 10 Jun 2019 at 9:40 AM
Type: Oral Session: Monday Afternoon II
The Super Cryogenic Dark Matter Search (SuperCDMS) is at the low-threshold frontier. Our detector technology can detect nuclear recoils at the eV-scale energies necessary for generation-two low-mass dark matter searches. The SNOLAB installation, which will be commissioned in the next two years, will produce world-class limits on the presence of low-mass (between 0.5 and 10\,GeV/c$^2$) dark matter. ... More
Presented by Dr. Anthony VILLANO on 10 Jun 2019 at 5:45 PM
Type: Oral Session: Tuesday Afternoon I
NOvA is a two-detector long-baseline neutrino oscillation experiment which aims to make a determination of the neutrino mass hierarchy, the octant of ${\theta}_{23}$, and measure possible CP violation. The NOvA Test Beam program consists of a scaled-down NOvA detector placed in a beamline capable of delivering 0.3 - 2.0 GeV/c protons, electrons, pions, and kaons. The beamline detectors provide us ... More
Presented by Teresa LACKEY on 11 Jun 2019 at 3:50 PM
Type: Oral Session: Monday Afternoon I
The MicroBooNE experiment is an 87 t active mass Liquid Argon Time Projection Chamber (LArTPC) located on the Booster Neutrino Beam (BNB) at Fermilab, Chicago. The primary physics goals of this experiment are to investigate the excess of low energy electron-like events observed by MiniBooNE, perform precise measurements of neutrino on argon cross sections, and provide research and development for ... More
Presented by Mr. Krishan MISTRY on 10 Jun 2019 at 2:30 PM
Presented by Dr. Gavin S. DAVIES on 11 Jun 2019 at 2:10 PM
Session: Monday Morning I
Presented by Andrew FURMANSKI, Andrew FURMANSKI on 10 Jun 2019 at 9:00 AM