中子星合并中短伽马射线暴的剥离模型

S. Blinnikov, A. Yudin, N. Kramarev, M. Potashov
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引用次数: 5

摘要

我们概述了短伽马射线暴剥离模型的现状。经过对引力波事件GW170817和伴随的伽马暴GRB170817A的历史联合探测,短伽马暴与中子星并合的关系得到了可靠的证实。GRB170817A的许多特性,与其他短伽马射线爆发相比,被证明是特别的,自然可以用剥离模型来解释,这个模型是我们中的一个人在1984年提出的。我们指出了已故的Dmitriy Nadyozhin(1937-2020)在1990年预测GRB和kilonova性质中的作用。我们还回顾了在该模型的背景下需要解决的问题。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Stripping Model for Short Gamma-Ray Bursts in Neutron Star Mergers
We overview the current status 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. Many properties of GRB170817A, which turned out to be peculiar in comparison with other short gamma-ray bursts, are naturally explained in the stripping model, suggested by one of us in 1984. We point out the role of late Dmitriy Nadyozhin (1937–2020) in predicting the GRB and kilonova properties in 1990. We also review the problems to be solved in the context of this model.
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