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Stability of relativistic stars

作者:   时间:2018-06-25   点击数:

演讲人:林治武 教授  美国佐治亚理工学院

报告时间:2018年6月28日(周四)下午 3:00至 4:00

报告地点:知新楼B座924

演讲题目:Stability of relativistic stars

邀请人:胡锡俊教授

摘要:I will discuss the stability of non-rotating relativistic stars (white dwarfs, neutron stars etc.) modeled by Euler-Einstein equation. A turning point principle for the sharp stability criterion is obtained and used to explain the stability picture with a realistic equation of state. The linear instability is always true in the strong relativistic limit, in contrast to the Newtonian stars modeled by Euler-Poisson system. I will also discuss the critical phenomena for gravitational collapse and its relation to the dynamics near unstable stars. This is joint work with Hadzic and Rein.

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