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Accessing new physics with an undoped, cryogenic CsI CEvNS detector for COHERENT at the SNS

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arxiv 2311.13032 v1 pith:2YXQNDCM submitted 2023-11-21 hep-ex physics.ins-det

P. S. Barbeau , V. Belov , I. Bernardi , C. Bock , A. Bolozdynya , R. Bouabid , J. Browning , B. Cabrera-Palmer
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E. Conley V. da Silva J. Daughhetee J. Detwiler K. Ding M. R. Durand Y. Efremenko S. R. Elliott A. Erlandson L. Fabris M. Febbraro A. Galindo-Uribarri M. P. Green J. Hakenmüller M. R. Heath S. Hedges B. A. Johnson T. Johnson A. Khromov A. Konovalov E. Kozlova A. Kumpan O. Kyzylova J. M. Link J. Liu A. Major K. Mann D. M. Markoff J. Mattingly P. E. Mueller J. Newby N. Ogoi J. O'Reilly D. S. Parno D. Pérez-Loureiro S. I. Penttila D. Pershey C. G. Prior J. Queen R. Rapp H. Ray O. Razuvaeva D. Reyna G. C. Rich D. Rudik J. Runge D. J. Salvat J. Sander K. Scholberg A. Shakirov G. Simakov W. M. Snow V. Sosnovtsev M. Stringer T. Subedi B. Suh B. Sur R. Tayloe K. Tellez-Giron-Flores Y.-T. Tsai J. Vanderwerp E. E. van Nieuwenhuizen R. L. Varner C. J. Virtue G. Visser K. Walkup E. M. Ward T. Wongjirad Y. Yang J. Yoo C.-H. Yu A. Zaalishvili
This is my paper · ORCID
classification hep-exphysics.ins-det
keywords detectorphysicscoherentcryogenicneutrinoundopedaccelerator-producedaccessing
verification ladder T0 review T1 audit T2 compute T3 formal
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We consider the potential for a 10-kg undoped cryogenic CsI detector operating at the Spallation Neutron Source to measure coherent elastic neutrino-nucleus scattering and its sensitivity to discover new physics beyond the standard model. Through a combination of increased event rate, lower threshold, and good timing resolution, such a detector would significantly improve on past measurements. We considered tests of several beyond-the-standard-model scenarios such as neutrino non-standard interactions and accelerator-produced dark matter. This detector's performance was also studied for relevant questions in nuclear physics and neutrino astronomy, namely the weak charge distribution of CsI nuclei and detection of neutrinos from a core-collapse supernova.

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