论文标题
持续时间伽玛射线爆发及其流出符合GW170817
Short duration gamma-ray bursts and their outflows in light of GW170817
论文作者
论文摘要
GW170817的检测，它是广泛的多波长随访运动，以及随后的大量理论发展和解释，在理解整个二进制中性星星合并现象方面迈出了巨大的一步。它的方面之一是将合并视为短伽马射线爆发（SGRB）的祖先，这将是本次审查的主题。一方面，GW170817的观察结果证实了一些理论上的期望，这证实了二进制中子星合并是SGRB的祖细胞的证实。此外，GW170817的多通电剂性质允许收集前所未有的数据，例如合并的触发时间，检测到伽马射线光子的延迟以及离轴事件的亮点。总的来说，GW170817的数据无与伦比的丰富性使我们能够描绘至少一个SGRB的相当详细的图片。我将详细介绍我们学到的知识，出现了什么新问题，以及在研究了GW170817可弥补的事件的样本时，回答它们的观点。
The detection of GW170817, it's extensive multi-wavelength follow-up campaign, and the large amount of theoretical development and interpretation that followed, have resulted in a significant step forward in the understanding of the binary neutron star merger phenomenon as a whole. One of its aspects is seeing the merger as a progenitor of short gamma-ray bursts (SGRB), which will be the subject of this review. On the one hand, GW170817 observations have confirmed some theoretical expectations, exemplified by the confirmation that binary neutron star mergers are the progenitors of SGRBs. In addition, the multimessenger nature of GW170817 has allowed for gathering of unprecedented data, such as the trigger time of the merger, the delay with which the gamma-ray photons were detected, and the brightening afterglow of an off-axis event. All together, the incomparable richness of the data from GW170817 has allowed us to paint a fairly detailed picture of at least one SGRB. I will detail what we learned, what new questions have arisen, and the perspectives for answering them when a sample of GW170817-comparable events have been studied.
