期刊
ASTROPHYSICAL JOURNAL
卷 633, 期 2, 页码 1013-1017出版社
UNIV CHICAGO PRESS
DOI: 10.1086/466514
关键词
cosmic rays; gamma rays : bursts; gamma rays : theory; stars : individual (SGR 1806-20); stars : neutron
We estimate the high-energy neutrino flux from the giant flare of SGR 1806 - 20 on 2004 December 27, which irradiated Earth with a gamma-ray flux similar to 10(4) times larger than the most luminous gamma-ray bursts (GRBs) ever detected. The Antarctic Cerenkov neutrino detector AMANDA was online during the flare and may either have detected high-energy neutrinos for the first time from a cosmic point source or put constraints on the flare mechanism of magnetars. If TeV neutrinos are detected, one would also expect detectable EeV cosmic rays and possibly TeV gamma-ray emission in coincidence.
作者
我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。
推荐
暂无数据