Identifying Galactic sources of high-energy neutrinos

被引：11
|
作者：
Kheirandish, Ali [1 ,2 ]
机构：
[1] Penn State Univ, Dept Phys, University Pk, PA 16802 USA
[2] Penn State Univ, Inst Gravitat & Cosmos, University Pk, PA 16802 USA
来源：
ASTROPHYSICS AND SPACE SCIENCE | 2020年 / 365卷 / 06期
关键词：
High-energy cosmic neutrinos; Cosmic rays; High-energy astrophysics; Milky Way; GAMMA-RAY EMISSION; ELEMENTAL GROUPS; COSMIC-RAYS; ICECUBE; REGION; ACCELERATION; TELESCOPE; RADIATION; ASTRONOMY; SPECTRA;
D O I：
10.1007/s10509-020-03816-3
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
High-energy neutrinos present the ultimate signature for a cosmic ray accelerator. Galactic sources responsible for acceleration of cosmic ray up to the knee in cosmic ray spectrum will provide a guaranteed, albeit subdominant, contribution to the high-energy cosmic neutrino flux. In this review, we discuss the the prospects for identification of high-energy neutrinos from sources of the very high energy gamma ray emission in the Milky Way. We present the status of the search for point-like and extended emission from these sources, and describe how the results of these studies indicate that neutrino telescopes are closing in on identifying Galactic sources of high-energy neutrinos.
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页数：20
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