论文标题
对二元驱动的Hypernova的简要回顾
A Brief Review of Binary Driven Hypernova
论文作者
论文摘要
二进制驱动的Hypernova（BDHN）模型长伽马射线爆发（GRB）发生在涉及碳 - 氧气核心（CO $ _ {\ rm Core} $）的二进制系统中，而伴侣中子星（NS）或黑洞（BH）。该模型于2012年首次提出，在火eshell模型和诱导的重力崩溃（IGC）范式上取得了成功和改进。经过近十年的发展，BDHN模型已经达到了几乎完整的结构，并解释了所有长突发的所有观察物进入其理论框架，并根据祖细胞的原始特性对长GRB进行了完善的分类。在本文中，我们介绍了BDHN模型的摘要以及在GRB观察框架中正式对现场的事件发生的每一个所设想的情节中工作的物理过程。
Binary driven hypernova (BdHN) models long gamma-ray burst (GRBs) as occurring in the binary systems involving a carbon-oxygen core (CO$_{\rm core}$) and a companion neutron star (NS) or a black hole (BH). This model, first proposed in 2012, succeeds and improves upon the fireshell model and the induced gravitational collapse (IGC) paradigm. After nearly a decade of development, the BdHN model has reached a nearly complete structure, explaining all the observables of long bursts into its theoretical framework, and has given a refined classification of long GRBs according to the original properties of the progenitors. In this article, we present a summary of the BdHN model and the physical processes at work in each of the envisaged Episodes during its occurrence and lifetime, duly contextualized in the framework of GRB observations.
