What is the fate of a black hole embedded in an expanding universe?
classification
🌀 gr-qc
keywords
blackembeddedholeuniverseassumptionsattractorscertainclass
read the original abstract
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.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.