Development of Cryogenic Scintillation Detectors for the Search of New Physics
Keyu Ding

TL;DR
This paper presents the development and characterization of CryoCsI, a cryogenic scintillation detector with low energy threshold aimed at detecting new physics phenomena like CEvNS, dark matter, and non-standard neutrino interactions.
Contribution
It introduces CryoCsI, a novel cryogenic undoped CsI detector with enhanced sensitivity and discusses its construction, light yield improvements, and strategies to address cryogenic SiPM challenges.
Findings
Achieved light yield of 50 photoelectrons per keV$_{ee}$
Measured alpha and neutron quenching factors (~15%)
Identified challenges with cryogenic SiPMs and PMT overshoot effects
Abstract
CryoCsI, the proposed prototype, is a cryogenic undoped CsI scintillating detector, which has a much lower energy threshold potentially down to 0.5 keV compared to the doped CsI. This enhanced sensitivity of CryoCsI allows for the observation of more Coherent elastic neutrino-nucleus scattering events. Precise measurements of CEvNS can not only validate the predictions of the Standard Model but also explore new physics. In conjunction with other COHERENT detectors, CryoCsI has the potential to achieve world-leading sensitivities in a broad range of physics topics within and beyond the SM. The sensitivities of CryoCsI to hidden-sector dark matter, non-standard neutrino interactions, and neutron radius are explored. This thesis delves into the construction of CryoCsI and efforts to enhance its light yield from 20 to photoelectrons per keV electron-equivalent…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Particle Detector Development and Performance · Superconducting and THz Device Technology
