Nonlinear kinetic theory of cosmic-ray acceleration in supernova remnants

被引：2

作者：

Berezhko, E ^{[1
]}

机构：

[1] Inst Cosmophys Res & Aeron, Yakutsk 677891, Russia

来源：

SPACE SCIENCE REVIEWS | 2001年 / 99卷 / 1-4期

关键词：

D O I：

10.1023/A:1013813603069

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

A review of kinetic nonlinear theory for cosmic-ray (CR) acceleration and subsequent gamma-ray production due to CR nuclear component in supernova remnants (SNRs) is presented. The correspondence of the expected spectrum and composition of CRs produced inside SNRs in the Galaxy with the experimental data is discussed. Possible explanations of negative results in searching high energy gamma-ray emission from nearby SNRs are analyzed.

引用

页码：295 / 304

页数：10

共 31 条

[1]

Aharonian FA, 1999, ASTRON ASTROPHYS, V351, P330

[2] Cosmic ray acceleration in pulsar-driven supernova remnants: The effect of scattering [J].