Bulletin of the American Physical Society
5th Joint Meeting of the APS Division of Nuclear Physics and the Physical Society of Japan
Volume 63, Number 12
Tuesday–Saturday, October 23–27, 2018; Waikoloa, Hawaii
Session HA: Conference Experience for Undergraduates Poster Session (2:00pm - 3:45pm)
2:00 PM,
Friday, October 26, 2018
Hilton
Room: Grand Promenade
Abstract ID: BAPS.2018.HAW.HA.124
Abstract: HA.00124 : Coherent CAPTAIN-Mills: Measuring Low-Energy Neutrino Cross Sections at Los Alamos Neutron Science Center*
Presenter:
Jose Plata Salas
(Universidad Nacional Autónoma de México, Los Alamos National Laboratory)
Authors:
Jose Plata Salas
(Universidad Nacional Autónoma de México, Los Alamos National Laboratory)
Richard G Van de Water
(Los Alamos National Laboratory, Los Alamos National Laboratory)
William Charles Louis
(Los Alamos National Laboratory, Los Alamos National Laboratory)
Robert L Cooper
(New Mexico State University, Los Alamos National Laboratory)
Core-collapse supernovae (SN) release 99% of their gravitational binding energy in neutrinos with energies of a few tens-of-MeV over a timescale of a few tens-of-seconds. The flavor composition, energy spectrum and time structure of the neutrino burst in a SN explosion provide information about the supernova properties, including its core-collapse, explosion and neutron star cooling mechanism. Coherent CAPTAIN-Mills (CCM) is a Liquid Argon (LAr) detector located at the Lujan Center at the Los Alamos Neutron Science Center which is a prolific source of neutrinos up to 50 MeV from stopped pion and muon decay. By instrumenting CCM with photo-multiplier tubes (PMTs) and fast electronics, a significant measurement of low-energy neutrino scattering cross sections can be performed. We propose to use the CCM detector to measure the νe and νμ nuclear cross sections on liquid argon with an uncertainty of roughly 10%, focusing on the supernova energy range. This poster discusses the importance of the measurements of low-energy neutrino cross sections for the observation of supernovae explosions, as well as the PMT background rate and energy distribution, status of the detector and Fall commissioning run.
*We acknowledge Los Alamos National Laboratory for LDRD funding.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.HAW.HA.124
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