COHERENT 2018 at the Spallation Neutron Source
COHERENT 2018 at the Spallation Neutron Source
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2018-03
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通讯作者:
D. Akimov;J. Albert;Peibo An;C. Awe;P. Barbeau;B. Becker;V. Belov;M. Blackston;A. Bolozdynya;A. Brown;A. Burenkov;B. Cabrera-Palmer;M. Cervantes;J. Collar;R. Cooper;R. Cooper;J. Daughhetee;D. Dean;M. D. V. Coello;J. Detwiler;M. D'Onofrio;Y. Efremenko;S. Elliott;E. Erkela;A. Etenko;L. Fabris;M. Febbraro;N. Fields;W. Fox;A. Galindo-Uribarri;M. Green;M. Heath;S. Hedges;E. Iverson;M. Kaemingk;L. Kaufman;S. Klein;A. Khromov;S. Ki;A. Konovalov;A. Kovalenko;A. Kumpan;L. Li;W. Lu;K. Mann;Y. Melikyan;D. Markoff;H. Moreno;P. Mueller;P. Naumov;J. Newby;D. Parno;S. Penttila;G. Perumpilly;D. Radford;R. Rapp;H. Ray;J. Raybern;D. Reyna;G. Rich;D. Rimal;D. Rudik;D. Salvat;K. Scholberg;B. Scholz;G. Sinev;W. Snow;V. Sosnovtsev;A. Shakirov;B. Suh;R. Tayloe;R. Thornton;I. Tolstukhin;J. Vanderwerp;R. Varner;C. Virtue;J. Yoo;C.-H. Yu;J. Zettlemoyer
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作者:
D. Akimov;J. Albert;Peibo An;C. Awe;P. Barbeau;B. Becker;V. Belov;M. Blackston;A. Bolozdynya;A. Brown;A. Burenkov;B. Cabrera-Palmer;M. Cervantes;J. Collar;R. Cooper;R. Cooper;J. Daughhetee;D. Dean;M. D. V. Coello;J. Detwiler;M. D'Onofrio;Y. Efremenko;S. Elliott;E. Erkela;A. Etenko;L. Fabris;M. Febbraro;N. Fields;W. Fox;A. Galindo-Uribarri;M. Green;M. Heath;S. Hedges;E. Iverson;M. Kaemingk;L. Kaufman;S. Klein;A. Khromov;S. Ki;A. Konovalov;A. Kovalenko;A. Kumpan;L. Li;W. Lu;K. Mann;Y. Melikyan;D. Markoff;H. Moreno;P. Mueller;P. Naumov;J. Newby;D. Parno;S. Penttila;G. Perumpilly;D. Radford;R. Rapp;H. Ray;J. Raybern;D. Reyna;G. Rich;D. Rimal;D. Rudik;D. Salvat;K. Scholberg;B. Scholz;G. Sinev;W. Snow;V. Sosnovtsev;A. Shakirov;B. Suh;R. Tayloe;R. Thornton;I. Tolstukhin;J. Vanderwerp;R. Varner;C. Virtue;J. Yoo;C.-H. Yu;J. Zettlemoyer
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.