Formation of Black holes in Spherically Symmetric Gravitational Collapse
Black holes are predicted by general relativity. It is a mathematical challenge to describe the formation of black holes in gravitational collapse in general relativity. In this course, we will discuss the classical result of Oppenheimer and Snyder on the formation of black holes in spherically symmetric gravitational collapse, and the black hole formation theorem of spherically symmetric self-gravitating massless scalar field by Christodoulou.
讲师
日期
2021年09月14日 至 12月02日
修课要求
Riemannian Geometry, Partial Differential Equation
参考资料
1. Richard C. Tolman: Effect of Inhomogeneity on Cosmological Models
2. J. R. Oppenheimer; H. Snyder: On Continued Gravitational Contraction
3. D. Christodoulou: Violation of Cosmic Censorship in the Gravitational Collapse of a Dust Cloud
4. D. Christodoulou: The Formation of Black Holes and Singularities in Spherically Symmetric Gravitational Collapse
2. J. R. Oppenheimer; H. Snyder: On Continued Gravitational Contraction
3. D. Christodoulou: Violation of Cosmic Censorship in the Gravitational Collapse of a Dust Cloud
4. D. Christodoulou: The Formation of Black Holes and Singularities in Spherically Symmetric Gravitational Collapse
视频公开
不公开
笔记公开
不公开
讲师介绍
乐鹏宇博士毕业于苏黎世联邦理工学院，后在美国密西根大学从事博士后研究，2021年9月入职北京雁栖湖应用数学研究院，担任助理研究员，致力于微分几何和与广义相对论相关的基础数学研究。