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.60
Abstract: HA.00060 : Neutrino Physics with PROSPECT Background Characterization at the High Flux Isotope Reactor (HFIR)*
Presenter:
Diego Venegas Vargas
(University of Tennessee, Knoxville, Oak Ridge National Lab)
Authors:
Diego Venegas Vargas
(University of Tennessee, Knoxville, Oak Ridge National Lab)
Alan Salcedo
(University of Tennessee, Knoxville, Oak Ridge National Lab)
Alfredo Galindo-Uribarri
(Oak Ridge National Lab, University of Tennessee, Knoxville)
The Precision Reactor Oscillation and Spectrum Experiment (PROSPECT) is a neutrino experiment at short baselines that aims to search for the existence of sterile neutrinos and precisely measure the energy spectrum of antineutrinos emitted from the Oak Ridge National Laboratory's High Flux Isotope Reactor (HFIR). A complete characterization of background sources present throughout the course of the experiment is required to obtain a proper understanding of the reactor’s response, as well as to investigate the variation of background during operation periods. The PROSPECT detector has been collecting data since March 16th of the present year. This study presents data obtained through measurements and simulations of the background sources at HFIR, along with preliminary results of the detector’s performance. A brief overview of the detector’s status and main physics goals are presented.
*This material is based upon work supported by US Department of Energy (DOE) Office of Science, Office of High Energy Physics and by Oak Ridge National Laboratory under Contract DE-AC05-00OR22725", along with the acknowledgment to the University of Tennessee, Knoxville.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.HAW.HA.60
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