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Spherically symmetric spacetimes with a trapped surface

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arxiv gr-qc/0403032 v2 pith:NYYY47CM submitted 2004-03-08 gr-qc

Mihalis Dafermos This is my paper · ORCID
classification gr-qc
keywords classsphericallysurfacesymmetrictrappedspacetimesareaasymptotically
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This paper investigates the global properties of a class of spherically symmetric spacetimes. The class contains the maximal development of asymptotically flat spherically symmetric initial data for a wide variety of coupled Einstein-matter systems. For this class, it is proven here that the existence of a single trapped surface or marginally trapped surface implies the completeness of future null infinity and the formation of an event horizon whose area radius is bounded by twice the final Bondi mass.

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Cited by 2 Pith papers

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  1. Unveiling horizons in quantum critical collapse

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    Semiclassical quantum corrections in critical collapse yield a finite mass gap and transition from classical Type II to quantum Type I behavior, providing a quantum enforcement of weak cosmic censorship.

  2. Charged cosmological black holes: a thorough study of a family of solutions

    gr-qc 2019-08 conditional novelty 6.0 of 10

    The Shah-Vaidya charged cosmological black hole metric is shown to be an exact solution of Einstein-Maxwell equations with a cuscuton field, and its causal structure is classified into four parameter regions with diff...

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