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GRB 941017: A CASE STUDY OF NEUTRINO PRODUCTION IN GAMMA-RAY BURSTS

机译:GRB 941017:伽马射线爆发中中微子产生的案例研究

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摘要

GRB 941017, a gamma-ray burst of exceptional fluence, has recently been shown to have a high-energy component that is not consistent with the standard fireball phenomenology. If this component is the result of photomeson interactions in the burst fireball, it provides new and compelling support for substantial high-energy neutrino fluxes from this and similar sources. In this Letter, we consider what impact this new information has on the neutrino spectra of gamma-ray bursts and discuss how this new evidence impacts the prospects for detection of such events in next generation neutrino telescopes.
机译:GRB 941017是一种具有特殊能量密度的伽马射线爆发,最近被证明具有高能量成分,与标准的火球现象学不一致。如果该成分是爆发的火球中光子相互作用的结果,那么它将为来自此来源和类似来源的大量高能中微子通量提供新的和令人信服的支持。在这封信中,我们考虑了这一新信息对伽马射线爆发的中微子谱有何影响,并讨论了这一新证据如何影响下一代中微子望远镜探测此类事件的前景。

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