The formation of black holes in spherically symmetric gravitational collapse
نویسندگان
چکیده
We consider the spherically symmetric, asymptotically flat Einstein equations coupled to a suitable matter model and find explicit conditions on the initial data which guarantee the formation of a black hole in the evolution. We establish such results for general matter models characterized by general conditions on the matter quantities, and we prove that the collisionless gas as described by the Vlasov equation satisfies these conditions for a large class of initial data.
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تاریخ انتشار 2007