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Yoo, Jong Hee
액시온 및 극한상호작용 연구단
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Sensitivity of the COHERENT experiment to accelerator-produced dark matter

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Title
Sensitivity of the COHERENT experiment to accelerator-produced dark matter
Author(s)
Akimov, D; An, P; Awe, C; Barbeau, PS; Becker, B; Belov, V; Blackston, MA; Bolozdynya, A; Cabrera-Palmer, B; Chen, N; Conley, E; Cooper, RL; Daughhetee, J; Coello, MD; Detwiler, JA; Durand, MR; Efremenko, Y; Elliott, SR; Fabris, L; Febbraro, M; Fox, W; Galindo-Uribarri, A; Green, MP; Hansen, KS; Heath, MR; Hedges, S; Johnson, T; Kaemingk, M; Kaufman, LJ; Khromov, A; Konovalov, A; Kozlova, E; Kumpan, A; Li, L; Librande, JT; Link, JM; Liu, J; Mann, K; Markoff, DM; Moreno, H; Mueller, PE; Newby, J; Parno, DS; Penttila, S; Pershey, D; Radford, D; Rapp, R; Ray, H; Raybern, J; Razuvaeva, O; Reyna, D; Rich, GC; Rudik, D; Runge, J; Salvat, DJ; Scholberg, K; Shakirov, A; Simakov, G; Sinev, G; Snow, WM; Sosnovtsev, V; Suh, B; Tayloe, R; Tellez-Giron-Flores, K; Thornton, RT; Tolstukhin, I; Vanderwerp, J; Varner, RL; Virtue, CJ; Visser, G; Wiseman, C; Wongjirad, T; Yang, J; Yen, YR; Yoo, Jong Hee; Yu, CH; Zettlemoyer, J
Subject
Antineutrinos, ; Neutrino Oscillations, ; Reactor Cores
Publication Date
2020-09
Journal
PHYSICAL REVIEW D, v.102, no.5, pp.052007-1 - 052007-10
Publisher
AMER PHYSICAL SOC
Abstract
© 2020 authors. Published by the American Physical Society. The COHERENT experiment is well poised to test sub-GeV dark matter models using detectors sensitive to coherent elastic neutrino-nucleus scattering (CEvNS) in the pi(+) decay-at-rest (pi-DAR) neutrino beam produced by the Spallation Neutron Source. We show a planned 750-kg single-phase liquid argon scintillation detector would place leading limits on scalar light dark matter models for dark matter particles produced through vector and leptophobic portals in the absence of other effects beyond the standard model. The characteristic timing profile of a pi-DAR beam allows a unique opportunity for constraining systematic uncertainties on the standard model background using a time window where dark matter signal is not expected, enhancing expected sensitivity. Additionally, we discuss future prospects which show that an on-axis CEvNS detector would probe the thermal abundance for a scalar dark matter candidate for all couplings alpha' <= 1 for 15 MeV dark matter with just 1.0 tonne-yr of exposure with increased exposure testing a wider range of dark matter masses and spins
URI
https://pr.ibs.re.kr/handle/8788114/7628
DOI
10.1103/PhysRevD.102.052007
ISSN
2470-0010
Appears in Collections:
Center for Axion and Precision Physics Research(액시온 및 극한상호작용 연구단) > 1. Journal Papers (저널논문)
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