Abstract
AbstractInvestigated in this work were sensitivities of a prototype detector for the detection of low-mass dark matter particles produced at the Spallation Neutron Source at the Oak Ridge National Laboratory in 2 years of data taking. The presumed prototype consisted of 10 kg undoped CsI or NaI scintillation crystals directly coupled with SiPM arrays operated at 77 K. Compared to the COHERENT CsI(Na) detector, a much higher light yield was assumed for the prototype. An experiment with a cylindrical 1 kg undoped CsI crystal coupled directly to two photomultiplier tubes at about 77 K was conducted as the first step to verify the idea. A light yield of $$26.0 \pm 0.4$$26.0±0.4 photoelectrons per keV electron-equivalent was achieved. This eliminated the concern of self light absorption in large crystals raised in some of the early studies.
Funder
Natural Science Foundation
Publisher
Springer Science and Business Media LLC
Subject
Physics and Astronomy (miscellaneous),Engineering (miscellaneous)
Reference76 articles.
1. G. Jungman, M. Kamionkowski, K. Griest, Phys. Rep. 267(5), 195 (1996)
2. M. Schumann, J. Phys. G 46(10), 103003 (2019)
3. C.A.J. O’Hare, Can we overcome the neutrino floor at high masses? (2020), arXiv: 2002.07499
4. D.S. Akerib et al., Phys. Rev. Lett. 118, 021303 (2017)
5. M. Battaglieri, et al., US Cosmic Visions: New Ideas in Dark Matter 2017: Community Report (2017). arXiv:1707.04591
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