Ultra-high-energy cosmic rays and inflation relies

被引：113

作者：

Kuzmin, VA ^{[1
]}

Tkachev, II

机构：

[1] Russian Acad Sci, Inst Nucl Res, 60Th October Anniversary Prospect 7, Moscow 117312, Russia

[2] CERN, Div TH, CH-1211 Geneva 23, Switzerland

来源：

PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS | 1999年 / 320卷 / 1-6期

关键词：

cosmic rays; dark matter; early universe;

D O I：

10.1016/S0370-1573(99)00064-2

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

There are two processes of matter creation after inflation that may be relevant to the resolution of the puzzle of cosmic rays observed with energies beyond GZK cut-off: 1) gravitational creation of superheavy (quasi)stable particles, and 2) non-thermal phase transitions leading to the formation of topological defects. We review both possibilities. (C) 1999 Elsevier Science B.V. All rights reserved.

引用

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页码：199 / 221

页数：23

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