Physics Letters B (Oct 2020)

Search for exotic neutrino-electron interactions using solar neutrinos in XMASS-I

  • K. Abe,
  • Y. Chen,
  • K. Hiraide,
  • K. Ichimura,
  • S. Imaizumi,
  • N. Kato,
  • K. Kobayashi,
  • M. Kobayashi,
  • S. Moriyama,
  • M. Nakahata,
  • K. Sato,
  • H. Sekiya,
  • T. Suzuki,
  • A. Takeda,
  • S. Tasaka,
  • M. Yamashita,
  • B.S. Yang,
  • N.Y. Kim,
  • Y.D. Kim,
  • Y.H. Kim,
  • R. Ishii,
  • Y. Itow,
  • K. Kanzawa,
  • K. Martens,
  • A. Mason,
  • Y. Suzuki,
  • K. Miuchi,
  • Y. Takeuchi,
  • K.B. Lee,
  • M.K. Lee,
  • Y. Fukuda,
  • H. Ogawa,
  • Y. Kishimoto,
  • K. Nishijima,
  • K. Fushimi,
  • B.D. Xu,
  • S. Nakamura

Journal volume & issue
Vol. 809
p. 135741

Abstract

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We have searched for exotic neutrino-electron interactions that could be produced by a neutrino millicharge, by a neutrino magnetic moment, or by dark photons using solar neutrinos in the XMASS-I liquid xenon detector. We observed no significant signals in 711 days of data. We obtain an upper limit for neutrino millicharge of 5.4×10−12e at 90% confidence level assuming all three species of neutrino have common millicharge. We also set flavor-dependent limits assuming the respective neutrino flavor is the only one carrying a millicharge, 7.3×10−12e for νe, 1.1×10−11e for νμ, and 1.1×10−11e for ντ. These limits are the most stringent yet obtained from direct measurements. We also obtain an upper limit for the neutrino magnetic moment of 1.8×10−10 Bohr magnetons. In addition, we obtain upper limits for the coupling constant of dark photons in the U(1)B−L model of 1.3×10−6 if the dark photon mass is 1×10−3 MeV/c2, and 8.8×10−5 if it is 10 MeV/c2.

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