Dr
Teppei Katori
(Massachusetts Institute of Technology)
10/22/12, 9:30 AM
Dr
Jaroslaw Nowak
(University of Minnesota)
10/22/12, 11:35 AM
Dr
Yoshinari Hayato
(Kamioka, ICRR, Univ. of Tokyo)
10/22/12, 1:30 PM
Mr
Steven Dytman
(Univ. of Pittsburgh)
10/22/12, 2:00 PM
Dr
Nathan Mayer
(Tufts University), Mr
Tomasz Golan
(Wroclaw University)
10/22/12, 2:45 PM
Summary of NuInt11 and goals of NuInt12
Dr
Philip Rodrigues
(University of Rochester)
10/22/12, 4:00 PM
Dr
Teppei Katori
(Massachusetts Institute of Technology)
10/22/12, 4:30 PM
Prof.
Martin Tzanov
(Louisiana State University)
10/22/12, 5:00 PM
Mr
Kenyi Paolo Hurtado Anampa
(CBPF)
10/22/12, 5:20 PM
Dr
Alfons Weber
(University of Oxford & STFC/RAL)
10/22/12, 5:40 PM
Prof.
Eric Christy
(Hampton University)
10/23/12, 9:00 AM
Dr
Eram Rizvi
(Queen Mary, University of London)
10/23/12, 9:25 AM
Jorge G. Morfin
(Fermilab)
10/23/12, 9:50 AM
Dr
Olga Lalakulich
(Universitaet Giessen)
10/23/12, 10:40 AM
Dr
Olga Lalakulich
(Universitaet Giessen)
10/23/12, 11:00 AM
Prof.
Taka Kajino
(National Astronomical Observatory, University of Tokyo)
10/23/12, 1:30 PM
Dr
Natalie Jachowicz
(Ghent University)
10/23/12, 2:00 PM
Prof.
Toshio Suzuki
(Nihon University)
10/23/12, 2:30 PM
Annelise Malkus
(North Carolina State University)
10/23/12, 3:00 PM
Prof.
Clarence Virtue
(Laurentian University)
10/23/12, 4:00 PM
Prof.
Flavio Cavanna
(Yale U.)
10/23/12, 4:30 PM
Dr
Yoo Jonghee
(Fermi National Accelerator Laboratory)
10/23/12, 5:00 PM
Mr
Guillermo Fernandez Moroni
(Fermilab)
10/24/12, 9:00 AM
Dr
Akihiro Minamino
(Kyoto University)
10/24/12, 9:20 AM
Dr
Alfons Weber
(University of Oxford & STFC/RAL)
10/24/12, 9:45 AM
Dr
Artur Ankowski
(INFN and Department of Physics,``Sapienza'' Universita' di Roma)
10/24/12, 10:10 AM
Jorge G. Morfin
(Fermilab)
10/24/12, 11:25 AM
Dr
davide meloni
(RomaTre University)
10/24/12, 11:50 AM
Dr
Eliecer Hernández-Gajate
(Universidad de Salamanca)
10/25/12, 9:00 AM
Dr
Satoshi Nakamura
(Yukawa Institute, Kyoto University)
10/25/12, 9:30 AM
Dr
MOHAMMAD SAJJAD ATHAR
(DEPARTMENT OF PHYSICS, ALIGARH MUSLIM UNIVERSITY, ALIGARH)
10/25/12, 10:00 AM
Mr
Brandon Eberly
(University of Pittsburgh)
10/25/12, 11:00 AM
Mr
Murdoch Matthew
(University of Liverpool)
10/25/12, 11:20 AM
Dr
Olga Lalakulich
(Universitaet Giessen)
10/25/12, 11:40 AM
Dr
Luis Alvarez-Ruso
(University of Valencia)
10/25/12, 2:00 PM
Dr
Antonin Vacheret
(University of Oxford)
10/25/12, 2:30 PM
Mr
Jose Luis Palomino Gallo
(CBPF)
10/25/12, 2:50 PM
Kendall Mahn
(TRIUMF)
10/25/12, 4:00 PM
Joe Grange
(University of Florida)
10/25/12, 4:25 PM
Dr
Laura Fields
(Northwestern University)
10/25/12, 5:00 PM
Mr
Daniel Ruterbories
(Colorado State University)
10/25/12, 5:30 PM
Prof.
Alejandro Mariano
(Departamento de Física, Universidad Nacional de La plata, Argentina)
10/25/12, 6:00 PM
The one pion production process νA →A'lπN results to be an important background to the quasielactic νA →A'lN process used as signal in neutrino oscillation experiments, at the moment of constrain fake events. When only 1p1h final states are considered, the calculated cross section is rough 50% below the experimental data. In this contribution we analyze the effect of adding 2p2h final states.
Ms
Huma Haider
(Aligarh Muslim University), Prof.
M.Sajjad Athar
(Aligarh Muslim University)
10/25/12, 6:00 PM
We shall present the results for the ratio of weak nuclear structure functions $\frac{F_{2}^{A}}{F_{2}^{proton}}$ and $\frac{F_{3}^{A}}{F_{3}^{proton}}$,
where A is the different nuclear targets like $_1^2D$, CH, $H_{2}O$, $^{56}Fe$ and $^{208}Pb$ which are being used in the ongoing Miner$\nu$A experiment at Fermilab.
We have studied these nuclear structure functions
using relativistic...
Aaron Higuera
(Universidad de Guanajuato)
10/25/12, 6:00 PM
MINERvA (Main Injector Experiment for v-A) is a neutrino scattering
experiment in the 1-10 GeV energy range in the NuMI high-intensity neutrino beam at
FermiNational Accelerator Laboratory. MINERvA is measuring neutrino/antineutrino
scattering off a variety of different nuclear materials (C, Fe, Pb, He, H2O). This poster
will describe the analysis of Charged Current Charged Pion...
Mr
David Martinez
(Centro Brasileiro de Pesquisas Fisicas)
10/25/12, 6:00 PM
MINERvA is a few-GeV neutrino scattering experiment that has been taking data in the NuMI beam line at Fermilab
since November 2009. The experiment will provide important inputs, both in support of neutrino oscillation searches and as a
pure weak probe of the nuclear medium. For this, MINERvA employs a fine-grained detector, with an eight ton active target region
composed of plastic...
Mr
Giuliano Maggi
(Universidad Santa María)
10/25/12, 6:00 PM
MINERvA is a neutrino experiment located at Fermilab. The main goal of
the experiment is to study neutrino interactions using different targets
and to measure differential neutrino cross sections. In this poster we
concentrate on Charged Current Neutral Pion Production at the MINERvA
experiment where the signal is defined as a muon, nucleon and neutral pion in the final state. The...
Mr
Guillermo Fiorentini
(CBPF)
10/25/12, 6:00 PM
MINERvA (Main INjector Experiment for v-A) is a neutrino scattering experiment in the NuMI high-intensity neutrino beam at the Fermi National Accelerator Laboratory. MINERvA was designed to make precision measurements of low energy neutrino and antinuetrino cross sections on a variety of different materials (plastic scintillator, C, Fe, Pb, He and H2O). We present the current status of the...
Mr
Guillermo Fernandez Moroni
(Fermilab)
10/25/12, 6:00 PM
This is a new experiment intended to detect very low energy neutrinos coming from a nuclear reactor using CCDs (Charge Coupled Devices). These silicon detectors have very low energy threshold (~7eV RMS) and very good spatial resolution (~15um). Also, nowadays, it is possible to fabricate very thick CCDs (~250um) increasing the detecting mass to 1g. All these characteristics make them a perfect...
Ms
Huma Haider
(Department of Physics, Aligarh Muslim University, India), Prof.
M.Sajjad Athar
(Department of Physics, Aligarh Muslim University, India)
10/25/12, 6:00 PM
We shall present the results of our study of non-isoscalarity corrections and nuclear medium effects in the extraction of $sin^2\theta_W$ using Paschos-Wolfenstein(PW) relation.
PW relation for an isoscalar nuclear target is defined as
\begin{eqnarray} \label{ratio_cross}
R_{PW}=\frac{\sigma(\nu_\mu~A \rightarrow \nu_\mu~X)~-~\sigma(\bar\nu_\mu~A \rightarrow...
Prof.
Gustavo Valdiviesso
(Universidade Federal de Alfenas)
10/25/12, 6:00 PM
Reactor neutrino experiments have observed a 5% deficit of electron anti-neutrino flux, when compared to the one predicted from nuclear physics as a product of the reactor's fission chains. One aspect that might have been overlooked in the literature is the contribution from extreme non-adiabatic effects coming from "decompression" when leaving the high density nuclear fuel rods. This work...
Dr
Antonin Vacheret
(University of Oxford)
10/25/12, 6:00 PM
Single \pi^0 production is one of the most important backgrounds in the \nu_\mu->\nu_e appearance measurement in T2K. Large uncertainties in this production rate make it difficult to predict. Therefore, measurement at the near detector (ND280) is required to constrain efficiently not only the background prediction at the far detector (Super-K) but also at the near detector to improve...
Mrs
Thamys Abrahão
(PUC-Rio/CBPF)
10/25/12, 6:00 PM
The Angra II nuclear reactor, which has the 4 GW of thermal power, is located in the Angra dos Reis nuclear power plant in the State of Rio de Janeiro in Brazil. The large fission rate of 10²⁰ per second produce about 5000 antineutrino interactions per day in a detector with only 1 m³ at the distance of 30 m from the reactor core. As the flux of antineutrinos is proportional to the thermal...
Prof.
Steven Manly
(University of Rochester)
10/25/12, 6:00 PM
Preliminary results on semi-inclusive charged pion production in eA
collisions at Ebeam=5 GeV/c2 are presented. These data are thought to be useful for tuning the hadronic production models used in extracting results from current and next-generation neutrino oscillation experiments.
The data were collected using the CLAS detector, which is a multipurpose,
large acceptance, magnetic...
Dr
Richard Gran
(University of Minnesota - Duluth)
10/25/12, 6:00 PM
We exposed a scaled-down version of the MINERvA detector to a beam of pions, kaons, and protons with momenta between 400 and 2000 MeV. These data are important for constraining the detector response to hadrons for our neutrino analyses in many respects: calorimetry, tracking, and PID response, and to constrain detector and Geant4 model uncertainties. For this, we built and operated a new...
Ms
Cheryl Patrick
(Northwestern University)
10/25/12, 6:00 PM
Current and future neutrino oscillation experiments depend on precise knowledge of neutrino-nucleus cross-sections. MINERvA is a neutrino scattering experiment at Fermilab, studying the interactions of muon neutrinos and antineutrinos with various nuclear targets. In order to make these measurements, it is vital that we carefully calibrate our detector. This poster explains the various in situ...
Abner Gomes
(Federal University of Goias - UFG)
10/25/12, 6:00 PM
Experimental evidences showed that the time evolution of a particular neutrino flavor state can produce the transition to a different flavor state, a phenomena called neutrino oscillation. In this work we aim to study the oscillation model by doing a phenomenological analysis using the MINOS (Main Injector Neutrino Oscillation Search) published data. We first review the muon neutrino CC...
Dr
Carlos Javier Solano Salinas
(UNI, Peru)
10/25/12, 6:00 PM
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 and, hopefully, neutrinos.
In particular, the reactions (a) gamma + p -> H + X, (b) gamma + p(up) -> pi(+-) = X, and (c) p(up) + p -> gamma + X are considered where gamma = resolved photon, and...
Mr
Marcelo Jorge Nascimento Souza
(CBPF)
10/25/12, 6:00 PM
We will present the status of the Neutrino ANGRA project, aimed at developing an antineutrino detector for monitoring nuclear reactor activity. The Angra experiment will be deployed at the Brazilian nuclear power plant Angra II. A water Cherenkov detector of one ton target will be placed in a commercial container next to the reactor containment, about 30 m from the reactor core. The 4 GW...
Mr
Iwa Ou
(Okayama University)
10/25/12, 6:00 PM
We plan to measure the branching ratios of \gamma-ray emission (E_\gamma >5 MeV) from giant resonance of ^16O and ^12C, as the functions of excitation energy (E_x).
This measurement will provide the fundamental and important information not only for the \gamma-ray production from primary neutral-current neutrino-oxygen (-carbon) interactions but also for that from the secondary hadronic...
Stefano Tognini
(Federal University of Goias - UFG)
10/25/12, 6:00 PM
The collision between a cosmic ray and an atmosphere nucleus produces a set of secondary particles, which will decay or interact with other atmosphere elements. This set of events produced by a primary particle is known as an extensive air shower (EAS) and is composed by a muonic, a hadronic and an electromagnetic component. The muonic flux, produced mainly by pion and kaon decays, has a...
Minerba Betancourt
(University of Minnesota)
10/25/12, 6:00 PM
NOvA is a 14 KTon long-baseline neutrino oscillation experiment currently
being installed in the NUMI off-axis neutrino beam produced at Fermilab.
A 222 Ton prototype NOvA detector (NDOS) was built and
operated in the neutrino beam for over a year to understand the the
response of the detector and its construction. Muon neutrino interaction
data collected in this test are being analyzed...
Dr
Arturo Samana
(Universidade Estadual de Santa Cruz)
10/25/12, 6:00 PM
In this work we performed a systematic study of the inclusive muon capture rates for the nuclei 12C, 20Ne, 32Mg, 28Si, 40Ar, 52Cr, 54Cr, 56Fe, and 58Ni using the Projected Random Quase-particle Phase
Approximation (PQRPA) as nuclear model.
The theoretical results of the capture rates within the PQRPA have been compared with those obtained in other works using other models.
We reckon that...
Dr
Satoshi Nakamura
(Yukawa Institute, Kyoto University)
10/25/12, 6:00 PM
An accurate understanding of the neutrino nucleus reactions is of great importance owing to the increasing precision of the neutrino oscillation experiments. The purpose of our study is to develop a reaction model for the lepton nucleus reaction from a few hundred MeV to a few GeV. We report on our analysis of the lepton nucleus reaction with the updated resonance model and the nuclear PDF in...
Dr
Deborah Harris
(Fermilab)
10/25/12, 6:00 PM
The Neutrinos at the Main Injector (NuMI) beamline delivers intense neutrino and anti-neutrino beams in an energy range of 2-20 GeV. Understanding these fluxes is crucial for measuring absolute cross sections in MINERvA. Three techniques for constraining these fluxes are being considered in MINERvA: in situ neutrino event rate measurements, external hadron production data and in situ muon...
Dr
Luis Alvarez-Ruso
(Instituto de Física Corpuscular (IFIC), Centro Mixto Universidad de Valencia ‐ CSIC, E‐46071 Valencia, Spain), Mr
M Rafi Alam
(aligarh muslim university, aligarh, india), Prof.
M Sajjad Athar
(aligarh muslim university, aligarh, india)
10/25/12, 6:00 PM
$\eta$ production off the nucleon induced by (anti)neutrinos is studied at
the low and intermediate energies for the ongoing and future neutrino oscillation experiments.
The non-resonant terms are calculated using a microscopical model based on the SU(3) chiral Lagrangians.
We consider $S_{11}$(1535) and $S_{11}$(1650) resonances. The vector part of the N-$S_{11}$ transition form factor...
Ms
Marcela Batkiewicz
(Institute of Nuclear Physics Polish Academy of Sciences (IFJ PAN))
10/25/12, 6:00 PM
Good knowledge of both inclusive and exclusive neutrino interaction cross sections is one of the key issues for a precise determination of the neutrino oscillation parameters in the T2K experiment.These studies are performed at the near detector (ND280). Its central tracker part equipped with a water target serves, among others, to study the νμ CCπ0 reaction. At the energies of the T2K...
Ms
Kinga Partyka
(Yale University)
10/26/12, 9:00 AM
Dr
Artur Ankowski
(INFN and Department of Physics,``Sapienza'' Universita' di Roma)
10/26/12, 9:25 AM
Mr
Andrea Meucci
(Universita' di Pavia)
10/26/12, 9:45 AM
Dr
Juan Nieves
(IFIC (CSIC-UV))
10/26/12, 10:05 AM
Prof.
Eric Christy
(Hampton University)
10/26/12, 11:00 AM
Dr
Donal Day Day
(University of Virginia)
10/26/12, 11:30 AM
Prof.
Maria Benedetta Barbaro
(University of Turin, Italy)
10/26/12, 12:00 PM
Prof.
Rocco Schiavilla
(Jefferson Lab/Old Dominion University)
10/26/12, 2:00 PM
Dr
Ornella Palamara
(Yale University)
10/26/12, 2:30 PM
Dr
Mark Hartz
(University of Toronto/York University)
10/26/12, 4:00 PM
Georgia Karagiorgi
(Columbia University)
10/26/12, 4:25 PM
Dr
Marc Bergevin
(UC Davis)
10/26/12, 5:15 PM
Dr
Juan Nieves
(IFIC (CSIC-UV))
10/27/12, 9:40 AM
Dr
Luis Alvarez-Ruso
(University of Valencia)
10/27/12, 10:00 AM
Mr
Steven Dytman
(Univ. of Pittsburgh)
10/27/12, 10:20 AM
Jan Sobczyk
(Wroclaw University/Fermilab)
10/27/12, 10:40 AM
Dr
Heather Ray
(University of Florida)
10/27/12, 11:00 AM
Prof.
Toshio Suzuki
(Nihon University)
10/27/12, 11:50 AM
Dr
Hiroshi Nunokawa
(Department of Physics, Pontificia Universidade Catolica do Rio de Janeiro)
10/27/12, 12:10 PM
Prof.
Kevin McFarland
(University of Rochester)
10/27/12, 12:30 PM
Dr
Luis Alvarez-Ruso
(University of Valencia)
10/27/12, 1:00 PM
Mr
Guillermo Fernandez Moroni
(Fermilab)