High energy neutrinos and cosmic rays

被引：2

作者：

Sigl, G. ^{[1
]}

机构：

[1] Univ Hamburg, Inst Theoret Phys 2, D-22761 Hamburg, Germany

来源：

NEUTRINO PHYSICS AND ASTROPHYSICS | 2012年 / 182卷

关键词：

MAGNETIC-FIELDS; ARRIVAL DIRECTION; SPECTRUM; ACCELERATION; SEARCH; SIMULATIONS; PROPAGATION; ANISOTROPY; RADIATION; GALAXIES;

D O I：

10.3254/978-1-61499-173-1-145

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

This is a summary of a series of lectures on the current experimental and theoretical status of our understanding of origin and nature of cosmic radiation. Specific focus is put on ultrahigh energy cosmic radiation above similar to 10(17) eV, including secondary neutral particles and in particular neutrinos. The most important open questions are related to the chemical composition and sky distributions of these particles as well as on the location and nature of their sources. High energy neutrinos at GeV energies and above from extra-terrestrial sources have not yet been detected and experimental upper limits start to put strong contraints on the sources and the acceleration mechanism of very high energy cosmic rays.

引用

页码：145 / 184

页数：40

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