Abstract

This paper provides an overview of the current state of the stripping model for short gamma-ray bursts. After the historical joint detection of the gravitational wave event GW170817 and the accompanying gamma-ray burst GRB170817A, the relation between short gamma-ray bursts and neutron star mergers has been reliably confirmed. We show that many properties of GRB170817A, which turned out to be peculiar in comparison with other short gamma-ray bursts, are naturally explained in the context of the stripping model, specifically, the time (1.7 s) between the peak of the gravitational wave signal and the detection of the gamma-ray burst, its total isotropic energy, and the parameters of the red and blue components of the accompanying kilonova.

中文翻译：

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中子星合并和伽马射线爆发：剥离模型

摘要

本文概述了短伽玛射线暴的剥离模型的当前状态。在对重力波事件GW170817及其伴随的伽马射线爆发GRB170817A进行历史联合检测之后，已经可靠地确认了短伽马射线爆发与中子星合并的关系。我们显示，在剥离模型的背景下，很自然地解释了GRB170817A的许多特性，这些特性与其他短伽马射线暴相比是特有的，具体来说就是重力波峰值之间的时间（1.7 s）信号和伽马射线爆发的探测，其总的各向同性能量以及伴随的千新星的红色和蓝色分量的参数。