OF ELECTRON ANTINEUTRINOS ANTINEUTRINOS ANTINEUTRINOS ASSOCIATED WITH GAMMA-RAY BURSTS USING KamLAND

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,B. K. Fujikawa, O T., 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

semanticscholar（2015）

引用 0|浏览1

暂无评分

摘要

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 ne fluence from GRBs below 7MeV and place first constraints on the relation between ne luminosity and effective temperature.

查看译文

AI 理解论文

溯源树

样例

生成溯源树，研究论文发展脉络

Chat Paper

正在生成论文摘要