中子转换-扩散:与GRB 170817兼容的结构短伽马暴射流新模型

Edwan Pr'eau, K. Ioka, P. M'esz'aros
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引用次数: 1

摘要

我们提出了一个通用的理论模型,用于构造通过双中子星合并事件的抛射物传播的相对论性射流,引入了中子转换-扩散的影响,它提供了一个从抛射物向射流轴横向传播的重子通量。这自然导致了外喷流重子负载结构的增加,其能量分布近似各向同性$E_{iso}(\theta) \propto \theta^{-4}$,这与在喷流离轴角观测到的第一次引力波和短伽马射线暴事件GW170817/GRB 170817A是一致的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Neutron conversion–diffusion: a new model for structured short gamma-ray burst jets compatible with GRB 170817
We present a generic theoretical model for the structuring of a relativistic jet propagating through the ejecta of a binary neutron star merger event, introducing the effects of the neutron conversion-diffusion, which provides a baryon flux propagating transversely from the ejecta towards the jet axis. This results naturally in an increased baryon load structure of the outer jet with the approximate isotropic energy distribution $E_{iso}(\theta) \propto \theta^{-4}$, which is compatible with the first gravitational wave and short gamma-ray burst event GW170817/GRB 170817A observed at an off-axis angle of the jet.
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