Neutrino Emission from Gamma-Ray Burst Fireballs, Revised

被引：150

作者：

Huemmer, Svenja ^{[1
]}

Baerwald, Philipp ^{[1
]}

Winter, Walter ^{[1
]}

机构：

[1] Univ Wurzburg, Inst Theoret Phys & Astrophys, D-97074 Wurzburg, Germany

来源：

PHYSICAL REVIEW LETTERS | 2012年 / 108卷 / 23期

关键词：

HIGH-ENERGY NEUTRINOS; MUON NEUTRINOS; ICECUBE; FLUX;

D O I：

10.1103/PhysRevLett.108.231101

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

We review the neutrino flux from gamma-ray bursts, which is estimated from gamma-ray observations and used for the interpretation of recent IceCube data, from a particle physics perspective. We numerically calculate the neutrino flux for the same astrophysical assumptions as the analytical fireball neutrino model, including the dominant pion and kaon production modes, flavor mixing, and magnetic field effects on the secondary muons, pions, and kaons. We demonstrate that taking into account the full energy dependencies of all spectra, the normalization of the expected neutrino flux reduces by about one order of magnitude and the spectrum shifts to higher energies, where we can pin down the exact origin of the discrepancies by the recomputation of the analytical models. We also reproduce the IceCube-40 analysis for exactly the same bursts and same assumptions and illustrate the impact of uncertainties. We conclude that the baryonic loading of the fireballs, which is an important control parameter for the emission of cosmic rays, can be constrained significantly with the full-scale experiment after about ten years.

引用

页数：5

共 24 条

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