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Black hole formation from a complete regular past

Mihalis Dafermos
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Abstract

An open problem in general relativity has been to construct an asymptotically flat solution to a reasonable Einstein-matter system containing a black hole in the future and yet past-causally geodesically complete, in particular, containing no white holes. We give such an example in this paper--in fact, a family of such examples, stable in a suitable sense--for the case of a self-gravitating scalar field.

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Mihalis Dafermos. 2003-10-07. Black hole formation from a complete regular past. https://doi.org/10.1007/s00220-009-0775-7

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