First Measurement of Coherent Elastic Neutrino-Nucleus Scattering on Argon

D. Akimov, J. B. Albert, P. An, C. Awe, P. S. Barbeau, B. Becker, V. Belov, I. Bernardi, M. A. Blackston, L. Blokland, A. Bolozdynya, B. Cabrera-Palmer, N. Chen, D. Chernyak, E. Conley, R. L. Cooper, J. Daughhetee, M. Del Valle Coello, J. A. Detwiler, M. R. DurandY. Efremenko, S. R. Elliott, L. Fabris, M. Febbraro, W. Fox, A. Galindo-Uribarri, A. Gallo Rosso, M. P. Green, K. S. Hansen, M. R. Heath, S. Hedges, M. Hughes, T. Johnson, M. Kaemingk, L. J. Kaufman, A. Khromov, A. Konovalov, E. Kozlova, A. Kumpan, L. Li, J. T. Librande, J. M. Link, J. Liu, K. Mann, D. M. Markoff, O. McGoldrick, H. Moreno, P. E. Mueller, J. Newby, D. S. Parno, S. Penttila, D. Pershey, D. Radford, R. Rapp, H. Ray, J. Raybern, O. Razuvaeva, D. Reyna, G. C. Rich, D. Rudik, J. Runge, D. J. Salvat, K. Scholberg, A. Shakirov, G. Simakov, G. Sinev, W. M. Snow, V. Sosnovtsev, B. Suh, R. Tayloe, K. Tellez-Giron-Flores, R. T. Thornton, I. Tolstukhin, J. Vanderwerp, R. L. Varner, C. J. Virtue, G. Visser, C. Wiseman, T. Wongjirad, J. Yang, Y. R. Yen, J. Yoo, C. H. Yu, J. Zettlemoyer

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Abstract

We report the first measurement of coherent elastic neutrino-nucleus scattering (CEvNS) on argon using a liquid argon detector at the Oak Ridge National Laboratory Spallation Neutron Source. Two independent analyses prefer CEvNS over the background-only null hypothesis with greater than 3σ significance. The measured cross section, averaged over the incident neutrino flux, is (2.2±0.7)×10-39 cm2 - consistent with the standard model prediction. The neutron-number dependence of this result, together with that from our previous measurement on CsI, confirms the existence of the CEvNS process and provides improved constraints on nonstandard neutrino interactions.

Original languageEnglish
Article number012002
JournalPhysical Review Letters
Volume126
Issue number1
DOIs
StatePublished - Jan 7 2021

Funding

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. This material is based upon work supported by the U.S. Department of Energy, Office of Science, Office of Workforce Development for Teachers and Scientists, Office of Science Graduate Student Research (SCGSR) program. The SCGSR program is administered by the Oak Ridge Institute for Science and Education (ORISE) for the DOE. ORISE is managed by ORAU under Contract No. DE-SC0014664. We also acknowledge support from the Alfred P. Sloan Foundation, the Consortium for Nonproliferation Enabling Capabilities, the Institute for Basic Science (IBS-R017-D1-2020-a00/IBS-R017-G1-2020-a00), the National Science Foundation, and the Russian Foundation for Basic Research (Projects No. 17-02-01077_a, 20-02-00670_a, and 18-32–00910 mol_a). The work was supported by the Ministry of Science and Higher Education of the Russian Federation, Project Fundamental properties of elementary particles and cosmology No. 0723-2020-0041, and the Russian Science Foundation, Contract No. 18-12-00135. Laboratory Directed Research and Development funds from ORNL also supported this project. This research used the Oak Ridge Leadership Computing Facility, which is a DOE Office of Science User Facility. This work has been partially supported by U.S. DOE Award No. DE-FG02-13ER41967. ORNL is managed by UT-Battelle, LLC, under Contract No. DE-AC05-00OR22725 for the U.S. Department of Energy. The U.S. Government retains and the publisher, by accepting the article for publication, acknowledges that the U.S. Government retains a nonexclusive, paid-up, irrevocable, worldwide license to publish or reproduce the published form of this manuscript, or allow others to do so, for U.S. Government purposes.

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