PIONIC PHOTONS AND NEUTRINOS FROM COSMIC RAY ACCELERATORS

被引：7

作者：

Halzen, Francis ^{[1
]}

机构：

[1] Univ Wisconsin, Dept Phys, Madison, WI 53706 USA

来源：

ACTA PHYSICA POLONICA B | 2011年 / 42卷 / 12期

关键词：

HIGH-ENERGY NEUTRINOS; TEV GAMMA-RAYS; BURSTS; EMISSION;

D O I：

10.5506/APhysPolB.42.2525

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

Identifying the accelerators that produce the Galactic and extragalactic cosmic rays has been a priority mission of several generations of high energy gamma ray and neutrino telescopes; success has been elusive so far. Detecting the gamma ray and neutrino fluxes associated with cosmic rays reaches a new watershed with the completion of Ice Cube, the first neutrino detector with sensitivity to the anticipated fluxes, and the construction of CTA, a ground-based gamma-ray detector that will map and study candidate sources with unprecedented precision. In this paper, we revisit the prospects for revealing the sources of the cosmic rays by a multiwavelength approach; after reviewing the methods, we discuss supernova remnants, gamma-ray bursts, active galaxies and GZK neutrinos in some detail.

引用

页码：2525 / 2545

页数：21

共 50 条

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