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Astrophysics > High Energy Astrophysical Phenomena

arXiv:1503.02137 (astro-ph)
[Submitted on 7 Mar 2015 (v1), last revised 15 Jun 2015 (this version, v2)]

Title:Study of electron anti-neutrinos associated with gamma-ray bursts using KamLAND

Authors:K. Asakura, A. Gando, Y. Gando, T. Hachiya, S. Hayashida, H. Ikeda, K. Inoue, K. Ishidoshiro, T. Ishikawa, S. Ishio, M. Koga, S. Matsuda, T. Mitsui, D. Motoki, K. Nakamura, S. Obara, Y. Oki, T. Oura, I. Shimizu, Y. Shirahata, J. Shirai, A. Suzuki, H. Tachibana, K. Tamae, K. Ueshima, H. Watanabe, B.D. Xu, H. Yoshida, A. Kozlov, Y. Takemoto, S. Yoshida, K. Fushimi, A. Piepke, T. I. Banks, B. E. Berger, T. O'Donnell, B.K. Fujikawa, J. Maricic, J.G. Learned, M. Sakai, L. A. Winslow, Y. Efremenko, H. J. Karwowski, D. M. Markoff, W. Tornow, J. A. Detwiler, S. Enomoto, M.P. Decowski
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Abstract:We search for electron anti-neutrinos ($\overline{\nu}_e$) from long and short-duration gamma-ray bursts~(GRBs) using data taken by the KamLAND detector from August 2002 to June 2013. No statistically significant excess over the background level is found. We place the tightest upper limits on $\overline{\nu}_e$ fluence from GRBs below 7 MeV and place first constraints on the relation between $\overline{\nu}_e$ luminosity and effective temperature.
Comments: 16 pages and 5 figures
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE); High Energy Physics - Experiment (hep-ex)
Cite as: arXiv:1503.02137 [astro-ph.HE]
  (or arXiv:1503.02137v2 [astro-ph.HE] for this version)
  https://doi.org/10.48550/arXiv.1503.02137
Journal reference: ApJ 806 87 2015
Related DOI: https://doi.org/10.1088/0004-637X/806/1/87

Submission history

From: Koji Ishidoshiro [view email]
[v1] Sat, 7 Mar 2015 07:39:09 UTC (1,057 KB)
[v2] Mon, 15 Jun 2015 04:49:04 UTC (1,055 KB)
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