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arxiv: gr-qc/9809057 · v1 · submitted 1998-09-17 · 🌀 gr-qc

Gravitational dust collapse with cosmological constant

classification 🌀 gr-qc
keywords cosmologicalcollapseconstanthorizonblackgravitationalholeapparent
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We study the fate of gravitational collapse in presence of a cosmological constant. The junctions conditions between static and non-static space-times are deduced. Three apparent horizon are formed, but only two have physical significance, one of them being the black hole horizon and the other the cosmological horizon. The cosmological constant term slows down the collapse of matter, limiting also the size of the black hole.

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Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Gravitational collapse of matter fields in de Sitter spacetimes

    gr-qc 2025-05 unverdicted novelty 4.0

    The authors analyze formation and evolution of trapped surfaces during matter collapse in de Sitter spacetime and conclude that black hole and cosmological horizons develop as time evolution of marginally trapped surfaces.