Dr
Mark Hartz
(Kavli IPMU (WPI), University of Tokyo/TRIUMF)
10/08/2015, 09:30
Prof.
Kendall Mahn
(Michigan State University)
10/08/2015, 09:45
Dr
Angela Papa
(Paul Scherrer Institut)
10/08/2015, 10:15
Prof.
Mu-Chun Chen
(University of California, Irvine)
10/08/2015, 11:00
Working group 1: Neutrino Oscillation Physics
Dr
João Pedro Athayde Marcondes de André
(Penn State University)
10/08/2015, 11:30
Working group 1: Neutrino Oscillation Physics
Dr
Sara Bolognesi
(IRFU, CEA Saclay)
10/08/2015, 12:00
Working group 2: Neutrino Scattering Physics
Dr
Marco Martini
(Ghent University)
10/08/2015, 12:30
Working group 2: Neutrino Scattering Physics
Prof.
Mu-Chun Chen
(University of California, Irvine)
10/08/2015, 14:30
Working group 1: Neutrino Oscillation Physics
Prof.
Dmitry Grigoriev
(Budker Institute of Nuclear Physics)
10/08/2015, 14:30
Working group 4: Muon Physics
Dr
Colin Whyte
(University of Strathclyde)
10/08/2015, 14:30
Working group 3: Accelerator Physics
Dr
Andrew Furmanski
(University of Manchester)
10/08/2015, 14:30
Working group 2: Neutrino Scattering Physics
Dr
Sushant Raut
(KTH Royal Institute of Technology, Stockholm)
10/08/2015, 14:54
Working group 1: Neutrino Oscillation Physics
Dr
Angela Papa
(Paul Scherrer Institut)
10/08/2015, 15:00
Working group 4: Muon Physics
Dr
Milorad Popovic
(FNAL)
10/08/2015, 15:00
Working group 3: Accelerator Physics
Dr
Anushree Ghosh
(Centro Brasileiro de Pesquisas Físicas)
10/08/2015, 15:10
Working group 2: Neutrino Scattering Physics
James Strait
(FNAL)
10/08/2015, 15:18
Working group 1: Neutrino Oscillation Physics
Dr
jean-baptiste lagrange
(Imperial College/Fermilab)
10/08/2015, 15:25
Working group 3: Accelerator Physics
Dr
Tom Feusels
(University of British Columbia)
10/08/2015, 15:42
Working group 1: Neutrino Oscillation Physics
Dr
Derun Li
(LBNL)
10/08/2015, 15:50
Working group 3: Accelerator Physics
Dr
Jonathan Paley
(Fermilab)
10/08/2015, 15:50
Working group 2: Neutrino Scattering Physics
Mr
Ben Krikler
(Imperial College London)
10/08/2015, 16:00
Working group 4: Muon Physics
Prof.
Alan Bross
(Fermilab)
10/08/2015, 16:50
Dr
Daniel Cherdack
(Colorado State University), Prof.
Jingyu Tang
(Institute of High Energy Physics), Prof.
Kenneth Long
(Imperial College London), Dr
Mark Palmer
(Fermilab), Prof.
Takashi Kobayashi
(KEK)
10/08/2015, 17:20
Prof.
Renata Zukanovich Funchal
(University of São Paulo)
11/08/2015, 09:00
Working group 1: Neutrino Oscillation Physics
Prof.
Jingyu Tang
(Institute of High Energy Physics)
11/08/2015, 09:30
Working group 3: Accelerator Physics
Dr
Mark Palmer
(Fermilab)
11/08/2015, 10:00
Working group 3: Accelerator Physics
Prof.
Masaharu Aoki
(Osaka University)
11/08/2015, 11:00
Working group 4: Muon Physics
Prof.
Ye Yuan
(IHEP,Beijing)
11/08/2015, 11:00
Working group 3: Accelerator Physics
Prof.
Kendall Mahn
(Michigan State University)
11/08/2015, 11:00
Working group 1: Neutrino Oscillation Physics
Dr
Nikolaos Vassilopoulos
(IHEP, CAS)
11/08/2015, 11:24
Working group 3: Accelerator Physics
Dr
Akihiro Minamino
(Kyoto University)
11/08/2015, 11:24
Working group 1: Neutrino Oscillation Physics
Mr
Roman Gredig
(Physik-Institut UZH)
11/08/2015, 11:30
Working group 4: Muon Physics
Mr
Jianfei Tong
(Institute of High Energy Physics, CAS, China)
11/08/2015, 11:48
Working group 3: Accelerator Physics
Prof.
Kirk McDonald
(Princeton University)
11/08/2015, 11:48
Working group 1: Neutrino Oscillation Physics
Dr
Kevin Lynch
(York College/CUNY)
11/08/2015, 12:00
Working group 4: Muon Physics
Dr
Jason St. John
(University of Cincinnati)
11/08/2015, 12:12
Working group 1: Neutrino Oscillation Physics
Dr
Cai Meng
(Institute of High Energy Physics)
11/08/2015, 12:12
Working group 3: Accelerator Physics
Prof.
Mayly Sanchez
(Iowa State University)
11/08/2015, 12:36
Working group 1: Neutrino Oscillation Physics
Mr
Yingpeng Song
(Institute of High Energy Physics, CAS)
11/08/2015, 12:36
Working group 3: Accelerator Physics
Dr
Hisakazu Minakata
(University of São Paulo)
11/08/2015, 14:30
Working group 1: Neutrino Oscillation Physics
Prof.
Craig Blocker
(Brandeis University)
11/08/2015, 14:30
Working group 4: Muon Physics
Prof.
Alan Bross
(Fermilab)
11/08/2015, 14:30
Working group 3: Accelerator Physics
Mr
Guillermo Daniel Megias Vazquez
(University of Seville, Spain)
11/08/2015, 14:30
Working group 2: Neutrino Scattering Physics
Dr
Jun Kameda
(Institute for Cosmic Ray Research, University of Tokyo)
11/08/2015, 14:54
Working group 1: Neutrino Oscillation Physics
Dr
claudia cecchi
(Università di Perugia e INFN Perugia)
11/08/2015, 15:00
Working group 4: Muon Physics
Dr
Jaroslaw Pasternak
(Imperial College/RAL-STFC)
11/08/2015, 15:00
Working group 3: Accelerator Physics
Prof.
Carlotta Giusti
(University Pavia)
11/08/2015, 15:00
Working group 2: Neutrino Scattering Physics
Dr
João Pedro Athayde Marcondes de André
(Penn State University)
11/08/2015, 15:18
Working group 1: Neutrino Oscillation Physics
Dr
jean-baptiste lagrange
(Imperial College/Fermilab)
11/08/2015, 15:25
Working group 3: Accelerator Physics
Mr
Tom Van Cuyck
(Ghent University)
11/08/2015, 15:30
Working group 2: Neutrino Scattering Physics
Mr
Alexander Nehrkorn
(CMS)
11/08/2015, 15:30
Working group 4: Muon Physics
Dr
Sanjeev Kumar Verma
(University of Delhi)
11/08/2015, 15:42
Working group 1: Neutrino Oscillation Physics
Dr
Alex Bogacz
(Jefferson Lab)
11/08/2015, 15:50
Working group 3: Accelerator Physics
Ms
Elise Wursten
(University of Leuven)
11/08/2015, 16:00
Working group 4: Muon Physics
Dr
Arturo Samana
(Universidade Estadual de Santa Cruz)
11/08/2015, 16:00
Working group 2: Neutrino Scattering Physics
Joao Coelho
(Tufts University)
11/08/2015, 16:06
Working group 1: Neutrino Oscillation Physics
Prof.
Mayly Sanchez
(Iowa State University)
11/08/2015, 17:00
Working group 1: Neutrino Oscillation Physics
Ms
Kirsty Duffy
(University of Oxford)
11/08/2015, 17:30
Working group 1: Neutrino Oscillation Physics
Brendan Kiburg
(Fermilab)
12/08/2015, 09:00
Working group 4: Muon Physics
Dr
Yoshi Uchida
(Imperial College London)
12/08/2015, 09:30
Working group 4: Muon Physics
Prof.
Hugh Gallagher
(Tufts University)
12/08/2015, 10:00
Working group 2: Neutrino Scattering Physics
Dr
Pavel Snopok
(IIT/Fermilab)
12/08/2015, 11:00
Working group 3: Accelerator Physics
Joao Coelho
(Tufts University)
12/08/2015, 11:00
Working group 1: Neutrino Oscillation Physics
Prof.
Dinko Pocanic
(University of Virginia)
12/08/2015, 11:00
Working group 4: Muon Physics
Mr
Mateus Carneiro
(CBPF)
12/08/2015, 11:00
Working group 2: Neutrino Scattering Physics
Mr
Ben Krikler
(Imperial College London)
12/08/2015, 11:23
Working group 4: Muon Physics
Dr
Diktys Stratakis
(Brookhaven National Laboratory)
12/08/2015, 11:25
Working group 3: Accelerator Physics
Dr
Chiara Sirignano
(University of Padova & INFN)
12/08/2015, 11:30
Working group 1: Neutrino Oscillation Physics
Mr
Martti Nirkko
(University of Bern)
12/08/2015, 11:45
Dr
Kevin Lynch
(York College/CUNY)
12/08/2015, 11:46
Working group 4: Muon Physics
Dr
Mark Palmer
(Fermilab)
12/08/2015, 11:50
Working group 3: Accelerator Physics
Serra Nicola
(University of Zurich)
12/08/2015, 12:00
Working group 1: Neutrino Oscillation Physics
Brendan Kiburg
(Fermilab)
12/08/2015, 12:09
Working group 4: Muon Physics
Dr
Yury Kolomensky
(LBNL)
13/08/2015, 09:30
Working group 1: Neutrino Oscillation Physics
Dr
Paride Paradisi
(University of Padua, Italy)
13/08/2015, 10:00
Working group 4: Muon Physics
Dr
Daniel Cherdack
(Colorado State University)
13/08/2015, 11:00
Working group 3: Accelerator Physics
Dr
Mark Hartz
(Kavli IPMU (WPI), University of Tokyo/TRIUMF)
13/08/2015, 11:30
Working group 3: Accelerator Physics
Alessandro Bravar
(University of Geneva)
13/08/2015, 12:00
Working group 3: Accelerator Physics
Dr
Deborah Harris
(Fermilab)
13/08/2015, 12:30
Working group 3: Accelerator Physics
Dr
Satoshi Nakamura
(Osaka University)
13/08/2015, 14:30
Working group 2: Neutrino Scattering Physics
Dr
Jaroslaw Pasternak
(Imperial College/RAL-STFC)
13/08/2015, 14:30
Working group 3: Accelerator Physics
Prof.
Gabriel Orebi Gann
(UC Berkeley / LBNL)
13/08/2015, 14:30
Working group 1: Neutrino Oscillation Physics
Mr
Guillaume Pronost
(Subatech)
13/08/2015, 14:52
Working group 1: Neutrino Oscillation Physics
Dr
Vladimir Nagaslaev
(Pbar)
13/08/2015, 14:53
Working group 3: Accelerator Physics
Dr
Tom Feusels
(University of British Columbia)
13/08/2015, 15:00
Prof.
Kyung Kwang Joo
(Chonnam National University)
13/08/2015, 15:14
Working group 1: Neutrino Oscillation Physics
Prof.
Takashi Kobayashi
(KEK), Dr
Tetsuro Sekiguchi
(KEK)
13/08/2015, 15:16
Working group 3: Accelerator Physics
Dr
Aaron Higuera
(University of Houston)
13/08/2015, 15:30
Dr
Suprabh Prakash
(Harish-Chandra Research Institute)
13/08/2015, 15:36
Working group 1: Neutrino Oscillation Physics
Mr
Ye Yang
(Kyushu University / KEK)
13/08/2015, 15:38
Working group 3: Accelerator Physics
Dr
Wei Wang
(College of William and Mary)
13/08/2015, 16:30
Working group 1: Neutrino Oscillation Physics
Dr
Craig Moore
(Fermilab)
13/08/2015, 17:00
Working group 3: Accelerator Physics
Dr
Claudio Dib
(Universidad Tecnica Federico Santa Maria)
14/08/2015, 09:30
Dr
Yury Malyshkin
(Pontifical Catholic University of Chile)
14/08/2015, 11:00
Working group 1: Neutrino Oscillation Physics
Alessandro Bravar
(University of Geneva)
14/08/2015, 11:00
Working group 2: Neutrino Scattering Physics
Dr
Marcos Dracos
(IPHC-IN2P3/CNRS)
14/08/2015, 11:00
Working group 3: Accelerator Physics
Mr
Kazuhiro Terao
(Nevis Laboratories, Columbia University)
14/08/2015, 11:30
Working group 1: Neutrino Oscillation Physics
Dr
Melissa Uchida
(Imperial College London)
14/08/2015, 11:30
Working group 3: Accelerator Physics
Prof.
Gail Dodge
(Old Dominion University)
14/08/2015, 11:30
Working group 2: Neutrino Scattering Physics
Francesco Terranova
(Univ. of Milano-Bicocca and INFN)
14/08/2015, 12:00
Working group 3: Accelerator Physics
Alessandro Bravar
(University of Geneva)
14/08/2015, 12:00
Working group 1: Neutrino Oscillation Physics
Dr
Carla Bonifazi
(Instituto de Física - Universidade Federal do Rio de Janeiro)
14/08/2015, 14:00
Working group 2: Neutrino Scattering Physics
Dr
ottone caretta
(RAL)
14/08/2015, 14:00
Working group 3: Accelerator Physics
Dr
CHIARA GHIANO
(universita di Genova, Italia)
14/08/2015, 14:00
Working group 1: Neutrino Oscillation Physics
Mr
Bjorn Scholz
(University Of Chicago)
14/08/2015, 14:30
Working group 2: Neutrino Scattering Physics
Dr
Eito Iwai
(KEK)
14/08/2015, 14:30
Working group 1: Neutrino Oscillation Physics
Prof.
Kirk McDonald
(Princeton University)
14/08/2015, 14:30
Working group 3: Accelerator Physics
James Strait
(FNAL)
14/08/2015, 15:00
Working group 3: Accelerator Physics
Jorge G. Morfin
(Fermilab)
14/08/2015, 15:00
Working group 2: Neutrino Scattering Physics
Dr
David Martinez Caicedo
(Illinois Institute of Technology)
14/08/2015, 15:00
Working group 1: Neutrino Oscillation Physics
14/08/2015, 16:00
Working group 1: Neutrino Oscillation Physics
Prof.
Alexandre Sousa
(University of Cincinnati)
15/08/2015, 09:00
Working group 1: Neutrino Oscillation Physics
Prof.
Kendall Mahn
(Michigan State University), Dr
Marco Martini
(Ghent University)
15/08/2015, 09:25
Working group 2: Neutrino Scattering Physics
Dr
Pavel Snopok
(IIT/Fermilab)
15/08/2015, 09:50
Working group 3: Accelerator Physics
Dr
Andrew Norman
(Fermilab)
15/08/2015, 10:15
Working group 4: Muon Physics
Prof.
Takashi Kobayashi
(KEK)
15/08/2015, 11:10
Working group 1: Neutrino Oscillation Physics
Prof.
Kenneth Long
(Imperial College London)
15/08/2015, 11:50
Working group 1: Neutrino Oscillation Physics
Working group 3: Accelerator Physics
Yury Malyshkin
(Institute for Nuclear Research RAS, Russia; Pontifical Catholic University of Chile)
Working group 1: Neutrino Oscillation Physics
Poster
A neutrino deficit is observed in radio-chemical solar neutrino experiments GALLEX and SAGE in measurements with radioactive sources. This result can be explained by neutrino transitions to a hypothetical sterile state on a short baseline, corresponding to the squared mass difference of the order of 1 eV^2. A new underground experiment to search for this type of neutrino transition is planed...
Yury Malyshkin
(Pontifical Catholic University of Chile)
Working group 1: Neutrino Oscillation Physics
Poster
Daya Bay is an international experiment based in China. Its primary goal is the measurement of the neutrino mixing angle \theta_{13} with unprecedented precision. In addition, it can address other topics in neutrino physics including sterile-neutrino searches, and high-statistics measurements of reactor anti-neutrinos. In Daya Bay, electron anti-neutrinos from 6 reactor cores are detected via...
Mr
Renan Picoreti
(Universidade Estadual de Campinas)
Working group 1: Neutrino Oscillation Physics
Poster
Before the establishment of the LMA-MSW solution, Neutrino Decay was studied - both by itself and together with standard flavor oscillations - to explain the difference between the expected Solar Neutrino flux from nuclear fusion processes in the Sun and the detected flux on Earth - the so-called Solar Neutrino Problem (SNP).
In this work, we studied Neutrino Decay as a sub-leading effect...
Dr
Andrew Furmanski
(University of Manchester)
Working group 2: Neutrino Scattering Physics
Poster
MicroBooNE is a 170 ton liquid argon TPC placed in the Booster Neutrino Beam at Fermilab. The detector is currently being commissioned and first neutrino beam data is expected towards the end of this year. Located in a beam with energies between 0.1 and 3GeV, MicroBooNE is able to make high statistics measurements of CCQE-like events. Recently, there have been indications experiments of...
Dr
Bruno Miguez
(Unicamp - LNGS)
Working group 2: Neutrino Scattering Physics
Poster
In the limit of low momentum transfer for neutrino nuclei elastic scattering is expected to observe a coherent superposition in the cross section for the nucleons that compose the nucleus, increasing the interaction cross section. This effect was already observed for scattering for electrons, but due to experimental difficulties it have never been verified in neutrino scattering. Some groups...
Gabriela Vitti Stenico
(Universidade Estadual de Campinas)
Working group 2: Neutrino Scattering Physics
Poster
Atmospheric neutrinos are produced by the interactions of cosmic rays with Earth’s atmosphere which create unstable secondary particles that decay producing neutrinos. Due to have a wide energy spectrum of some hundreds of MeV until order of TeV, these neutrinos are good objects to test new theories and to study neutrino oscillation where there is a change of neutrino flavor state to another....
Dr
Alexander Quiroga
(PUC-Rio)
Working group 1: Neutrino Oscillation Physics
Poster
We show that precision measurement of sum of neutrino masses by cosmological observation and efective neutrino mass by neutrinoless double beta decay, together with beta decay experiments, have a synergy which allows us to get information on the Majorana phase of neutrinos. In order to quantify this information, we use, in addition to the allowed region plots, the CP exclusion fraction...
Dr
Alexander Quiroga
(PUC-Rio)
Working group 1: Neutrino Oscillation Physics
Poster
In this work we use the fact that JUNO has the best opportunity to put the most stringent constraint in nu_3 lifetime over others experiments which utilize artificial neutrinos source. If there is a neutrino decay into invisible states, we find, by studying the \chi^2, that the \nu_3 timelife can be constrained to \tau_3/m_3 > 7.5 (5.5) x 10^(-11) s/eV at 95%(99%) C.L. by JUNO by 100kt.years...
Mr
Cesar Peixoto Ferreira
(Unicamp)
Working group 3: Accelerator Physics
Poster
We study sterile neutrinos in an extension of the standard model, based on the gauge group $SU(3)_C\otimes SU(3)_L\otimes SU(3)_R\otimes U(1)_N$, and use this model to illustrate how to apply cosmological limits to thermalized particles that decouple while relativistic. These neutrinos, $N_{aL}$, can be dark matter candidates, with a keV mass range arising rather naturally in this model. We...
Dr
Roberto Oliveira
(UNICAMP)
Working group 1: Neutrino Oscillation Physics
Poster
Focusing in the next generation of Long Baseline Neutrino Experiments, we study phenomenologically the neutrino oscillations behavior when decoherence and relaxation effects are taken into account in the propagation. In three neutrino oscillation approach, we can see that one particular oscillation channel may be enhanced due to decoherence and matter effect in the resonant region decoherence....
Dr
Masashi Otani
(KEK)
Working group 4: Muon Physics
Poster
The muon anomalous magnetic moment (g-2) and electric dipole moment
(EDM) are one of the effective paths to beyond Standard Model of
elementary particle physics. The E34 experiment aims to measure g-2 with
a precision of 0.1 ppm and search EDM with a sensitivity to 10-21 e*cm
with high intensity proton driver at J-PARC and a newly developed novel
technique of the ultra-cold muon beam. The...
Working group 4: Muon Physics
Edith Tueros
(CRAAM)
Working group 4: Muon Physics
Poster
We present preliminary results of cosmic rays flux behavior during a
disturbed geomagnetic period detected by CARPET installed in CASLEO at
the Argentinian Andes.CARPET was conceived to study cosmic rays
modulation during transients and, sporadic events associated with coronal
mass ejections (CME) and solar proton events, as well as long duration
phenomena associated with 11-year solar...
Mr
Ye Yang
(Kyushu University)
Working group 3: Accelerator Physics
Poster
High intensity muon beam is required for the muon electron transition experiment due to its low branching ratio. Thus, the pion capture superconducting solenoid has to be operated under the high radiation environment. Currently, LTS coil has small temperature margin and limit of magnetic field, whereas HTS coil has not only the large temperature margin but also good radiation resistance. We...
Prof.
Orlando Luis Goulart Peres
(UNICAMP)
Working group 1: Neutrino Oscillation Physics
Poster
Recent results from the neutrino experiments show evidence for light sterile neutrinos which do not have any SM interactions. These light sterile states are disfavored by cosmology due to the constraints from onthe Big Bang nucleosynthesis and the Large Scale Structure Formation. This tension could be solved if the sterile neutrino states could have interaction with a light gauge boson X with...
Mr
Mike Kroll
(Ruhr-Uni Bochum)
Working group 2: Neutrino Scattering Physics
Poster
We present a new calculation of the neutrino nucleon cross sections for charged and neutral currents using recent PDF fits that incorporate LHC data. We have performed a simple LO calculation as well as full NLO calculation, and further include corrections important at O(1GeV) energies such as lepton mass suppression for $\nu_\tau$ and target mass corrections (TMC).
Dr
Arturo Rodolfo Samana
(Universidade Estadual de Santa Cruz), Ms
Danaisis Vargas
(Universidade Estadual de Santa Cruz)
Working group 2: Neutrino Scattering Physics
Poster
Some years ago, the CRISP (Collaboration Rio-Ilhéus-São Paulo) code was developed to describe spallation and fission reactions [1] using the Monte Carlo method approach. In order to improve the physics and the capacity of prediction of the code, the neutrino channel is being implemented. This improvement could be applied in several experiments where the neutrino-nucleon/nucleus cross section...
Mr
Guilherme Gomes
(Campinas State University - Unicamp)
Working group 1: Neutrino Oscillation Physics
Poster
In the framework of quantum open systems we analyze data from KamLAND by using a model which considers neutrino oscillation in a three-family approximation with the inclusion of the decoherence effect. Using a χ² test we find new limits for the decoherence parameter which we call γ, considering the most recent data by KamLAND.
Dr
Carlos Javier Solano Salinas
(UNI, Peru)
Working group 2: Neutrino Scattering Physics
Poster
A phenomenological model which has had some success in explaining polarization phenomena and left-right asymmetry in inclusive proton-proton scattering is considered for reactions involving photons. In particular,the reactions (a) γ + p → H + X; (b) γ + p(↑) → π± + X and (c) p(↑) + p → γ + X are considered
where γ = resolved photon and hyperon H = Λ, Σ, Ξ etc. Predictions for hyperon...
Mr
Pedro Simoni Pasquini
(Unicamp)
Working group 1: Neutrino Oscillation Physics
Poster
Motivated by discovery of scalar particles at the LHC, we revisit the bounds from Yukawa couplings of scalar particles with neutrinos. Using data from meson decays and including for the first time the spectrum from meson decays we manage to put the following constraints for massless scalars: $|g_e|^2<1.9\times10^{-6}$, $|g_\mu|^2<7.4\times10^{-8}$ and $|g_\tau|^2<2.1\times10^{-2}$ at $90\%...
Prof.
Daniel Kaplan
(Illinois Institute of Technology)
Working group 3: Accelerator Physics
Poster
Two beamline Cherenkov detectors (Ckov-a,-b) support particle ID in the MICE beam line. Electrons and high-momentum muons and pions can be identified with good efficiency. We report on the Ckov-a,-b performance in detecting pions and muons with Step I data.
Dr
Yoshitaro Takaesu
(University of Tokyo)
Working group 1: Neutrino Oscillation Physics
Poster
In this presentation, we revisit the sensitivity studies of a Tokai-to-Kamioka-and-Korea (T2KK) and Tokai-to-Kamioka-and-Oki (T2KO) proposals where a 100 kton detector is placed in Korea (L = 1000 km) and Oki island (L = 653 km) in Japan, respectively, in addition to the Super-Kamiokande (SK) for determination of the neutrino mass hierarchy and leptonic CP phase (δCP).
We systematically...
Prof.
Diego Gratieri
(Universidade Federal Fluminense, UFF)
Working group 2: Neutrino Scattering Physics
Poster
We investigate how the uncertainties in neutrino-nucleon charged-current cross-section due the different QCD dynamic models would modify the neutrino absorption while they travel across the Earth. We compare the predictions from FJKPPP model, based in linear QCD evolution equation for the parton densities with BBMT model, which impose a Froissart unitarity of CC neutrino-nucleon cross-section...
Mr
Roger Rodrigo Galindo Orjuela
(Universidad Tecnica Federico Santa Maria)
Working group 2: Neutrino Scattering Physics
Poster
The $\nu_{e}$ from radioactive decays (238U, 232Th, 40K) inside the Earth, called geoneutrinos provide the best way to investigate the composition of the Earth. First experimental results and evidence of these neutrinos were observed by KamLAND and Borexino utilising the inverse beta decay process. Using this process the directionality of the neutrino can not be measured making the...
Dr
C. M. Castromonte
(Universidade Federal de Goiás)
Working group 4: Muon Physics
Poster
Atmospheric muons are produced when primary cosmic ray nuclei interact near the top of the atmosphere to produce hadronic showers which contain pions and kaons. These secondary mesons can either interact in further collisions in the atmosphere or decay to produce atmospheric muons. Since the majority of primary cosmic rays are protons, there is an excess of positively charged mesons in the...
Dr
Stefan Wagner
(CBPF)
Working group 1: Neutrino Oscillation Physics
Poster
The *Neutrinos Angra* experiment aims to measure the antineutrino flux from the reactor cores of the Angra dos Reis nuclear power plant. The main objective is to determine the reactor power and the nuclear fuel composition from the detected antineutrinos. Since this method could find application as a tool for nuclear safeguards and non-proliferation, the detector is designed to be safe,...