Neutrino afterglow from gamma-ray bursts:: ∼1018 eV

被引：175

作者：

Waxman, E ^{[1
]}

Bahcall, JN

机构：

[1] Weizmann Inst Sci, Dept Condensed Matter Phys, IL-76100 Rehovot, Israel

[2] Inst Adv Study, Princeton, NJ 08540 USA

来源：

ASTROPHYSICAL JOURNAL | 2000年 / 541卷 / 02期

关键词：

acceleration of particles; elementary particles; gamma rays : bursts;

D O I：

10.1086/309462

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We show that a significant fraction of the energy of a gamma-ray burst (GRB) is probably converted to a burst of 10(17)-10(19) eV neutrinos and multiple GeV gamma-rays that follow the main GRB by similar to 10 s. If GRBs accelerate protons to similar to 10(20) eV, a suggestion that recently gained support from observations of GRB afterglows, then both the neutrinos and the gamma-rays may be detectable.

引用

页码：707 / 711

页数：5

共 41 条

[1]

AKERLOF CW, 1999, GCN, V205

[2]

AXFORD WI, 1977, P 15 INT C COSM RAYS

[3] ACCELERATION OF COSMIC-RAYS IN SHOCK FRONTS .1. [J].