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What is the fate of a black hole embedded in an expanding universe?

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arxiv 0811.4667 v1 pith:63K46RS7 submitted 2008-11-28 gr-qc

classification gr-qc
keywords blackembeddedholeuniverseassumptionsattractorscertainclass
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Within a large class of exact solutions of the Einstein equations describing a black hole embedded in a Friedmann universe it is shown that, under certain assumptions, only those with comoving Hawking-Hayward quasi-local mass are generic, in the sense that they are late-time attractors.

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Cited by 1 Pith paper

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  1. Evaporating cosmologically coupled black holes

    astro-ph.CO 2026-07 conditional novelty 6.0 of 10

    If a black hole's mass grows with cosmic expansion, Hawking evaporation is slowed or reversed, weakening gamma-ray bounds on primordial black holes.

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