High-energy neutrinos from gamma ray bursts

被引：126

作者：

Dermer, CD

Atoyan, A

机构：

[1] USN, Res Lab, High Energy Space Environm Branch, Washington, DC 20375 USA

[2] Univ Montreal, CRM, Montreal, PQ H3C 3J7, Canada

来源：

PHYSICAL REVIEW LETTERS | 2003年 / 91卷 / 07期

关键词：

D O I：

10.1103/PhysRevLett.91.071102

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

We treat high-energy neutrino production in gamma ray bursts (GRBs). Detailed calculations of photomeson neutrino production are presented for the collapsar model, where internal nonthermal synchrotron radiation is the primary target photon field, and the supranova model, where external pulsar-wind synchrotron radiation provides important additional target photons. Detection of greater than or similar to10 TeV neutrinos from GRBs with Doppler factors greater than or similar to200, inferred from gamma-ray observations, would support the supranova model. Detection of less than or similar to10 TeV neutrinos is possible for neutrinos formed from nuclear production. Only the most powerful bursts at fluence levels greater than or similar to3x10(-4) erg cm(-2) offer a realistic prospect for detection of nu(mu).

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