Gravitational collapse and the formation of black holes for the spherically symmetric Einstein-Vlasov system
arXiv:0812.1645
Abstract
We review results on the spherically symmetric, asymptotically flat Einstein-Vlasov system. We focus on a recent result where we found explicit conditions on the initial data which guarantee the formation of a black hole in the evolution. Among these data there are data such that the corresponding solutions exist globally in Schwarzschild coordinates. We put these results into a more general context, and we include arguments which show that the spacetimes we obtain satisfy the weak cosmic censorship conjecture and contain a black hole in the sense of suitable mathematical definitions of these concepts which are available in the literature.
35 pages
References in corpus (5)
- Sharp bounds on of general spherically symmetric static objects
- A numerical investigation of the stability of steady states and critical phenomena for the spherically symmetric Einstein-Vlasov system
- On static shells and the Buchdahl inequality for the spherically symmetric Einstein-Vlasov system
- The formation of black holes in spherically symmetric gravitational collapse
- Global existence for the spherically symmetric Einstein-Vlasov system with outgoing matter