A Search for Correlated Low-energy Electron Antineutrinos in KamLAND with Gamma-Ray Bursts

Open Access
Authors
  • S. Abe
  • S. Asami
  • A. Gando
  • Y. Gando
  • T. Gima
  • A. Goto
  • T. Hachiya
  • K. Hata
  • K. Hosokawa
  • K. Ichimura
  • S. Ieki
  • H. Ikeda
  • K. Inoue
  • K. Ishidoshiro
  • Y. Kamei
  • N. Kawada
  • Y. Kishimoto
  • T. Kinoshita
  • M. Koga
  • N. Maemura
  • T. Mitsui
  • H. Miyake
  • K. Nakamura
  • K. Nakamura
  • R. Nakamura
  • H. Ozaki
  • T. Sakai
  • I. Shimizu
  • H. Sambonsugi
  • J. Shirai
  • K. Shiraishi
  • A. Suzuki
  • Y. Suzuki
  • A. Takeuchi
  • K. Tamae
  • M. Eizuka
  • M. Kurasawa
  • T. Nakahata
  • S. Futagi
  • H. Watanabe
  • Y. Yoshida
  • S. Obara
  • A. K. Ichikawa
  • S. Yoshida
  • S. Umehara
  • K. Fushimi
  • B. E. Berger
  • B. K. Fujikawa
  • M.P. Decowski
  • H. Song
  • KamLAND Collaboration
Publication date 01-03-2022
Journal Astrophysical Journal
Article number 69
Volume | Issue number 927 | 1
Number of pages 7
Organisations
  • Faculty of Science (FNWI) - Institute of Physics (IoP) - Institute for High Energy Physics (IHEF)
Abstract

We present the results of a time-coincident event search for low-energy electron antineutrinos in the KamLAND detector with gamma-ray bursts (GRBs) from the Gamma-ray Coordinates Network and Fermi Gamma-ray Burst Monitor. Using a variable coincidence time window of ±500 s plus the duration of each GRB, no statistically significant excess above the background is observed. We place the world's most stringent 90% confidence level upper limit on the electron antineutrino fluence below 17.5 MeV. Assuming a Fermi-Dirac neutrino energy spectrum from the GRB source, we use the available redshift data to constrain the electron antineutrino luminosity and effective temperature.

Document type Article
Language English
Published at https://doi.org/10.3847/1538-4357/ac4e7e
Other links https://www.scopus.com/pages/publications/85126716194
Downloads
Abe_2022_ApJ_927_69 (Final published version)
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