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Gravitational dust collapse and black holes in general relativity and beyond

2024-09-02 08:55:51
报告人 时间 14:00-15:30
地点 E4-233 2024
月日 09-03

Time:14:00-15:30, Tuesday, September 3 2024

Venue:E4-233, Yungu Campus


Host:Congjun Wu, ITS

Speaker:Hongguang Liu, Friedrich-Alexander-Universität Erlangen-Nürnberg

Title:Gravitational dust collapse and black holes in general relativity and beyond

Abstract:An outstanding problem in gravitational physics is to understand the final state of gravitational collapse and the formation of black holes or singularities. Dust-filled spacetime is the simplest model to study such a problem. The dynamics of dust-filled spherically symmetric spacetime in general relativity can be described by a first-order quasi-linear partial differential equation (PDE) system that is analogous to fluid dynamics. The characteristics of this PDE system transform the dynamics into a decoupled cosmological model with a Hamiltonian formulation, where the quasi-local Misner-Sharp mass appears naturally. In this talk, I will provide a brief introduction to this system in general relativity. I will then discuss the generalization of such dynamics to modified gravity systems beyond general relativity and their connection to effective descriptions of canonical quantum gravity. As a concrete example, I will present the spherically symmetric solution space of the extended model, which belongs to the mimetic gravity class and collapses to regular black holes.

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