Couch Sean M
Department of Physics and Astronomy, Michigan State University, 567 Wilson Road, East Lansing, MI 48824, USA
Philos Trans A Math Phys Eng Sci. 2017 Oct 28;375(2105). doi: 10.1098/rsta.2016.0271.
Core-collapse supernovae (CCSNe) are the explosions that attend the deaths of massive stars. Despite decades of research, several aspects of the mechanism that drives these explosions remain uncertain and the subjects of continued investigation. In this short review, I will give an overview of the CCSN mechanism and current research in the field. In particular, I will focus on recent results from three-dimensional simulations and the impact of turbulence and detailed non-spherical progenitor structure on CCSNe. This contribution is based on a talk given at the 'Bridging the Gap' workshop at Chicheley Hall on 2 June 2016.This article is part of the themed issue 'Bridging the gap: from massive stars to supernovae'.
核心坍缩超新星（CCSNe）是大质量恒星死亡时发生的爆炸。尽管经过了数十年的研究，但驱动这些爆炸的机制的几个方面仍然不确定，仍是持续研究的课题。在这篇简短的综述中，我将概述核心坍缩超新星机制以及该领域的当前研究。特别是，我将重点介绍三维模拟的最新结果以及湍流和详细的非球对称前身星结构对核心坍缩超新星的影响。本稿件基于2016年6月2日在奇切利厅举行的“弥合差距”研讨会上的一次演讲。本文是主题为“弥合差距：从大质量恒星到超新星”特刊的一部分。
