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

P. S. Barbeau; V. Belov; I. Bernardi; C. Bock; A. Bolozdynya; R. Bouabid; J. Browning; B. Cabrera-Palmer; 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

doi:10.1103/PhysRevD.109.092005

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

P. S. Barbeau, V. Belov, I. Bernardi, C. Bock, A. Bolozdynya, R. Bouabid, J. Browning, B. Cabrera-Palmer, 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-UribarriM. 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

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Abstract

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 (BSM). 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 BSM scenarios such as neutrino nonstandard 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 Cs and I nuclei and detection of neutrinos from a core-collapse supernova.

Original language	English
Article number	092005
Journal	Physical Review D
Volume	109
Issue number	9
DOIs	https://doi.org/10.1103/PhysRevD.109.092005
State	Published - May 1 2024

Funding

COHERENT collaborators thank Peter Denton and Julia Gehrlein for conversations on the interplay between NSIs and neutrino mixing. We thank Adam Aurisano for thoughts about the sterile oscillation disappearance probability for NC interactions. We also thank Jorge Piekarewicz for thoughts on the role of neutrino-scattering measurements in constraining nuclear structure. The COHERENT Collaboration acknowledges the generous resources provided by the ORNL Spallation Neutron Source, a DOE Office of Science User Facility, and thanks Fermilab for the continuing loan of the CENNS-10 detector. We also acknowledge support from the Alfred P. Sloan Foundation, the Consortium for Nonproliferation Enabling Capabilities, the National Science Foundation, the Korea National Research Foundation (No. NRF 2022R1A3B1078756), and the U.S. Department of Energy, Office of Science. Laboratory Directed Research and Development funds from ORNL also supported this project. This work was performed under the auspices of the U.S. Department of Energy by Lawrence Livermore National Laboratory under Contract No. DE-AC52-07NA27344. This research used the Oak Ridge Leadership Computing Facility, which is a DOE Office of Science User Facility. The work was supported by the Ministry of Science and Higher Education of the Russian Federation, Project \u201CNew Phenomena in Particle Physics and the Early Universe\u201D FSWU-2023-0073. CNL support was provided by Canada\u2019s Federal Science and Technology Program.

Funders	Funder number
National Science Foundation
Oak Ridge National Laboratory
U.S. Department of Energy
Alfred P. Sloan Foundation
Office of Science
National Research Foundation of Korea	NRF 2022R1A3B1078756
National Research Foundation of Korea
Lawrence Livermore National Laboratory	DE-AC52-07NA27344
Lawrence Livermore National Laboratory
Ministry of Education and Science of the Russian Federation	FSWU-2023-0073
Ministry of Education and Science of the Russian Federation

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10.1103/PhysRevD.109.092005

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Barbeau, P. S., Belov, V., Bernardi, I., Bock, C., Bolozdynya, A., Bouabid, R., Browning, J., Cabrera-Palmer, B., Conley, E., Da Silva, V., Daughhetee, J., Detwiler, J., Ding, K., Durand, M. R., Efremenko, Y., Elliott, S. R., Erlandson, A., Fabris, L., Febbraro, M., ... Zaalishvili, A. (2024). Accessing new physics with an undoped, cryogenic CsI CEvNS detector for COHERENT at the SNS. Physical Review D, 109(9), Article 092005. https://doi.org/10.1103/PhysRevD.109.092005

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

abstract = "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 (BSM). 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 BSM scenarios such as neutrino nonstandard 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 Cs and I nuclei and detection of neutrinos from a core-collapse supernova.",

author = "Barbeau, {P. S.} and V. Belov and I. Bernardi and C. Bock and A. Bolozdynya and R. Bouabid and J. Browning and B. Cabrera-Palmer and E. Conley and {Da Silva}, V. and J. Daughhetee and J. Detwiler and K. Ding and Durand, {M. R.} and Y. Efremenko and Elliott, {S. R.} and A. Erlandson and L. Fabris and M. Febbraro and A. Galindo-Uribarri and Green, {M. P.} and J. Hakenm{\"u}ller and Heath, {M. R.} and S. Hedges and Johnson, {B. A.} and T. Johnson and A. Khromov and A. Konovalov and E. Kozlova and A. Kumpan and O. Kyzylova and Link, {J. M.} and J. Liu and A. Major and K. Mann and Markoff, {D. M.} and J. Mattingly and Mueller, {P. E.} and J. Newby and N. Ogoi and J. O'Reilly and Parno, {D. S.} and D. P{\'e}rez-Loureiro and Penttila, {S. I.} and D. Pershey and Prior, {C. G.} and J. Queen and R. Rapp and H. Ray and O. Razuvaeva and D. Reyna and Rich, {G. C.} and D. Rudik and J. Runge and Salvat, {D. J.} and J. Sander and K. Scholberg and A. Shakirov and G. Simakov and Snow, {W. M.} and V. Sosnovtsev and M. Stringer and T. Subedi and B. Suh and B. Sur and R. Tayloe and K. Tellez-Giron-Flores and Tsai, {Y. T.} and J. Vanderwerp and {Van Nieuwenhuizen}, {E. E.} and Varner, {R. L.} and Virtue, {C. J.} and G. Visser and K. Walkup and Ward, {E. M.} and T. Wongjirad and Y. Yang and J. Yoo and Yu, {C. H.} and A. Zaalishvili",

note = "Publisher Copyright: {\textcopyright} 2024 authors. Published by the American Physical Society. ",

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Barbeau, PS, Belov, V, Bernardi, I, Bock, C, Bolozdynya, A, Bouabid, R, Browning, J, Cabrera-Palmer, B, Conley, E, Da Silva, V, Daughhetee, J, Detwiler, J, Ding, K, Durand, MR, Efremenko, Y, Elliott, SR, Erlandson, A, Fabris, L, Febbraro, M, Galindo-Uribarri, A, Green, MP, Hakenmüller, J, Heath, MR, Hedges, S, Johnson, BA, Johnson, T, Khromov, A, Konovalov, A, Kozlova, E, Kumpan, A, Kyzylova, O, Link, JM, Liu, J, Major, A, Mann, K, Markoff, DM, Mattingly, J, Mueller, PE, Newby, J, Ogoi, N, O'Reilly, J, Parno, DS, Pérez-Loureiro, D, Penttila, SI, Pershey, D, Prior, CG, Queen, J, Rapp, R, Ray, H, Razuvaeva, O, Reyna, D, Rich, GC, Rudik, D, Runge, J, Salvat, DJ, Sander, J, Scholberg, K, Shakirov, A, Simakov, G, Snow, WM, Sosnovtsev, V, Stringer, M, Subedi, T, Suh, B, Sur, B, Tayloe, R, Tellez-Giron-Flores, K, Tsai, YT, Vanderwerp, J, Van Nieuwenhuizen, EE, Varner, RL, Virtue, CJ, Visser, G, Walkup, K, Ward, EM, Wongjirad, T, Yang, Y, Yoo, J, Yu, CH & Zaalishvili, A 2024, 'Accessing new physics with an undoped, cryogenic CsI CEvNS detector for COHERENT at the SNS', Physical Review D, vol. 109, no. 9, 092005. https://doi.org/10.1103/PhysRevD.109.092005

TY - JOUR

T1 - Accessing new physics with an undoped, cryogenic CsI CEvNS detector for COHERENT at the SNS

AU - Barbeau, P. S.

AU - Belov, V.

AU - Bernardi, I.

AU - Bock, C.

AU - Bolozdynya, A.

AU - Bouabid, R.

AU - Browning, J.

AU - Cabrera-Palmer, B.

AU - Conley, E.

AU - Da Silva, V.

AU - Daughhetee, J.

AU - Detwiler, J.

AU - Ding, K.

AU - Durand, M. R.

AU - Efremenko, Y.

AU - Elliott, S. R.

AU - Erlandson, A.

AU - Fabris, L.

AU - Febbraro, M.

AU - Galindo-Uribarri, A.

AU - Green, M. P.

AU - Hakenmüller, J.

AU - Heath, M. R.

AU - Hedges, S.

AU - Johnson, B. A.

AU - Johnson, T.

AU - Khromov, A.

AU - Konovalov, A.

AU - Kozlova, E.

AU - Kumpan, A.

AU - Kyzylova, O.

AU - Link, J. M.

AU - Liu, J.

AU - Major, A.

AU - Mann, K.

AU - Markoff, D. M.

AU - Mattingly, J.

AU - Mueller, P. E.

AU - Newby, J.

AU - Ogoi, N.

AU - O'Reilly, J.

AU - Parno, D. S.

AU - Pérez-Loureiro, D.

AU - Penttila, S. I.

AU - Pershey, D.

AU - Prior, C. G.

AU - Queen, J.

AU - Rapp, R.

AU - Ray, H.

AU - Razuvaeva, O.

AU - Reyna, D.

AU - Rich, G. C.

AU - Rudik, D.

AU - Runge, J.

AU - Salvat, D. J.

AU - Sander, J.

AU - Scholberg, K.

AU - Shakirov, A.

AU - Simakov, G.

AU - Snow, W. M.

AU - Sosnovtsev, V.

AU - Stringer, M.

AU - Subedi, T.

AU - Suh, B.

AU - Sur, B.

AU - Tayloe, R.

AU - Tellez-Giron-Flores, K.

AU - Tsai, Y. T.

AU - Vanderwerp, J.

AU - Van Nieuwenhuizen, E. E.

AU - Varner, R. L.

AU - Virtue, C. J.

AU - Visser, G.

AU - Walkup, K.

AU - Ward, E. M.

AU - Wongjirad, T.

AU - Yang, Y.

AU - Yoo, J.

AU - Yu, C. H.

AU - Zaalishvili, A.

PY - 2024/5/1

Y1 - 2024/5/1

N2 - 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 (BSM). 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 BSM scenarios such as neutrino nonstandard 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 Cs and I nuclei and detection of neutrinos from a core-collapse supernova.

AB - 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 (BSM). 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 BSM scenarios such as neutrino nonstandard 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 Cs and I nuclei and detection of neutrinos from a core-collapse supernova.

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U2 - 10.1103/PhysRevD.109.092005

DO - 10.1103/PhysRevD.109.092005

M3 - Article

AN - SCOPUS:85192741421

SN - 2470-0010

VL - 109

JO - Physical Review D

JF - Physical Review D

IS - 9

M1 - 092005

ER -

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

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