Department of Astrophysical Sciences, Princeton University, Princeton, NJ, USA.
Department of Astronomy, University of California, Berkeley, CA, USA.
Nature. 2021 Jan;589(7840):29-39. doi: 10.1038/s41586-020-03059-w. Epub 2021 Jan 6.
Most supernova explosions accompany the death of a massive star. These explosions give birth to neutron stars and black holes, and eject solar masses of heavy elements. However, determining the mechanism of explosion has been a half-century journey of great numerical and physical complexity. Here we present the status of this theoretical quest and the physics and astrophysics upon which its resolution seems to depend. The delayed neutrino-heating mechanism is emerging as the key driver of supernova explosions, but there remain many issues to address, such as the chaos of the involved dynamics.
大多数超新星爆炸伴随着大质量恒星的死亡。这些爆炸产生了中子星和黑洞,并抛出了太阳质量的重元素。然而,确定爆炸的机制一直是一个具有巨大数值和物理复杂性的半个世纪的探索。在这里,我们展示了这一理论探索的现状,以及似乎取决于其解决的物理和天体物理学。延迟中微子加热机制正在成为超新星爆炸的关键驱动因素,但仍有许多问题需要解决,例如涉及的动力学的混沌。