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COHERENT 2018 at the Spallation Neutron Source

Authors :
Akimov, D.
Albert, J. B.
An, P.
Awe, C.
Barbeau, P. S.
Becker, B.
Belov, V.
Blackston, M. A.
Bolozdynya, A.
Brown, A.
Burenkov, A.
Cabrera-Palmer, B.
Cervantes, M.
Collar, J. I.
Cooper, R. J.
Cooper, R. L.
Daughhetee, J.
Dean, D. J.
Coello, M. del Valle
Detwiler, J. A.
D'Onofrio, M.
Efremenko, Y.
Elliott, S. R.
Erkela, E.
Etenko, A.
Fabris, L.
Febbraro, M.
Fields, N.
Fox, W.
Galindo-Uribarri, A.
Green, M. P.
Heath, M. R.
Hedges, S.
Iverson, E. B.
Kaemingk, M.
Kaufman, L. J.
Klein, S. R.
Khromov, A.
Ki, S.
Konovalov, A.
Kovalenko, A.
Kumpan, A.
Li, L.
Lu, W.
Mann, K.
Melikyan, Y.
Markoff, D. M.
Moreno, H.
Mueller, P. E.
Naumov, P.
Newby, J.
Parno, D. S.
Penttila, S.
Perumpilly, G.
Radford, D.
Rapp, R.
Ray, H.
Raybern, J.
Reyna, D.
Rich, G. C.
Rimal, D.
Rudik, D.
Salvat, D. J.
Scholberg, K.
Scholz, B.
Sinev, G.
Snow, W. M.
Sosnovtsev, V.
Shakirov, A.
Suh, B.
Tayloe, R.
Thornton, R. T.
Tolstukhin, I.
Vanderwerp, J.
Varner, R. L.
Virtue, C. J.
Yoo, J.
Yu, C. -H.
Zettlemoyer, J.
Publication Year :
2018

Abstract

The primary goal of the COHERENT collaboration is to measure and study coherent elastic neutrino-nucleus scattering (CEvNS) using the high-power, few-tens-of-MeV, pulsed source of neutrinos provided by the Spallation Neutron Source (SNS) at Oak Ridge National Laboratory (ORNL). The COHERENT collaboration reported the first detection of CEvNS [Akimov:2017ade] using a CsI[Na] detector. At present the collaboration is deploying four detector technologies: a CsI[Na] scintillating crystal, p-type point-contact germanium detectors, single-phase liquid argon, and NaI[Tl] crystals. All detectors are located in the neutron-quiet basement of the SNS target building at distances 20-30 m from the SNS neutrino source. The simultaneous measurement in all four COHERENT detector subsystems will test the $N^2$ dependence of the cross section and search for new physics. In addition, COHERENT is measuring neutrino-induced neutrons from charged- and neutral-current neutrino interactions on nuclei in shielding materials, which represent a non-negligible background for CEvNS as well as being of intrinsic interest. The Collaboration is planning as well to look for charged-current interactions of relevance to supernova and weak-interaction physics. This document describes concisely the COHERENT physics motivations, sensitivity, and next plans for measurements at the SNS to be accomplished on a few-year timescale.<br />Comment: 22 pages, 14 figures

Details

Database :
arXiv
Publication Type :
Report
Accession number :
edsarx.1803.09183
Document Type :
Working Paper