High-energy cosmic rays from gamma-ray burst sources: A stronger case

被引：63

作者：

Waxman, E ^{[1
]}

机构：

[1] Weizmann Inst Sci, Fac Phys, IL-76100 Rehovot, Israel

来源：

ASTROPHYSICAL JOURNAL | 2004年 / 606卷 / 02期

关键词：

cosmic rays; gamma rays : bursts;

D O I：

10.1086/383116

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The suggested association between the sources of gamma-ray bursts (GRBs) and the sources of ultrahigh-energy cosmic rays (UHECRs) is based on two arguments: ( 1) the constraints that UHECR sources must satisfy in order to allow proton acceleration to greater than 10(20) eV are similar to those inferred for GRB sources from gamma-ray observations, and ( 2) the average energy generation rate of UHECRs is similar to the gamma-ray generation rate of GRBs. We show that recent GRB and UHECR observations strengthen both arguments and hence strengthen the suggested association.

引用

页码：988 / 993

页数：6

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