What is the fate of a black hole embedded in an expanding universe?
Valerio Faraoni, Changjun Gao, Xuelei Chen, and You-Gen Shen

TL;DR
This paper investigates the long-term behavior of black holes within expanding universes, showing that certain solutions with comoving mass are the typical late-time states.
Contribution
It identifies that black hole solutions with comoving Hawking-Hayward mass are the generic late-time attractors in an expanding universe.
Findings
Solutions with comoving Hawking-Hayward mass are late-time attractors.
Most black hole solutions in an expanding universe tend toward these attractors.
The study clarifies the fate of black holes in cosmological settings.
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.
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