STUDY of ELECTRON ANTI-NEUTRINOS ASSOCIATED with GAMMA-RAY BURSTS USING KamLAND

The Kamland Collaboration, 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. ShimizuY. 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, B. K. Fujikawa, T. O'Donnell, J. G. Learned, J. Maricic, M. Sakai, L. A. Winslow, Y. Efremenko, H. J. Karwowski, D. M. Markoff, W. Tornow, J. A. Detwiler, S. Enomoto, M. P. Decowski

研究成果: Article査読

4 被引用数 (Scopus)

抄録

We search for electron anti-neutrinos (ne) from long-and short-duration gamma-ray bursts (GRBs) using data taken by the Kamioka Liquid Scintillator Anti-Neutrino Detector (KamLAND) from 2002 August to 2013 June. No statistically significant excess over the background level is found. We place the tightest upper limits on e fluence from GRBs below 7 MeV and place first constraints on the relation between ne luminosity and effective temperature.

本文言語English
論文番号87
ジャーナルAstrophysical Journal
806
1
DOI
出版ステータスPublished - 2015 6 10

ASJC Scopus subject areas

  • 天文学と天体物理学
  • 宇宙惑星科学

フィンガープリント

「STUDY of ELECTRON ANTI-NEUTRINOS ASSOCIATED with GAMMA-RAY BURSTS USING KamLAND」の研究トピックを掘り下げます。これらがまとまってユニークなフィンガープリントを構成します。

引用スタイル