Ultra-high Energy Cosmic Rays and Neutrinos from Gamma-Ray Bursts, Hypernovae and Galactic Shocks

P. Mészáros
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引用次数: 17

Abstract

I review gamma-ray burst models (GRBs) and observations, and discuss the possible production of ultra-high energy cosmic rays and neutrinos in both the standard internal shock models and the newer generation of photospheric and hadronic GRB models, in the light of current constraints imposed by IceCube, Auger and TA observations. I then discuss models that have been proposed to explain the recent astrophysical PeV neutrino observations, including star-forming and star-burst galaxies, hypernovae and galaxy accretion and merger shocks.

伽玛射线暴、超超新星和银河激波产生的超高能量宇宙射线和中微子
我回顾了伽玛射线暴模型(GRBs)和观测,并讨论了在标准的内部激波模型和新一代的光球和强子伽玛射线暴模型中可能产生的超高能量宇宙射线和中微子,根据冰立方体、俄歇和TA观测施加的当前限制。然后,我讨论了已经提出的模型来解释最近的天体物理学PeV中微子观测,包括恒星形成和恒星爆发星系,超新星和星系吸积和合并冲击。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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