High energy astrophysical neutrinos

被引:0
|
作者
Athar, H [1 ]
机构
[1] Natl Ctr Theoret Sci, Div Phys, Hsinchu 300, Taiwan
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暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
High energy neutrinos with energy typically greater than tens of thousands of GeV may originate from several astrophysical sources. The sources may include, for instance, our Galaxy, the active centers of nearby galaxies, as well as possibly the distant sites of gamma ray bursts. I briefly review some aspects of production and propagation as well as prospects for observations of these high energy astrophysical neutrinos.
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页码:323 / 326
页数:4
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