Black holes and the multiverse
Jaume Garriga, Alexander Vilenkin, Jun Zhang

TL;DR
This paper explores how vacuum bubbles and domain walls during inflation can lead to black hole formation, potentially creating a multiverse with observable astrophysical consequences and implications for dark matter and supermassive black holes.
Contribution
It introduces a generic mechanism for black hole formation from inflationary bubbles and domain walls, linking early universe physics to multiverse structure and observable phenomena.
Findings
Black holes from bubbles can serve as dark matter candidates.
Black hole mass spectrum depends on model parameters.
Multiverse structure involves eternally inflating baby universes connected by wormholes.
Abstract
Vacuum bubbles may nucleate and expand during the inflationary epoch in the early universe. After inflation ends, the bubbles quickly dissipate their kinetic energy; they come to rest with respect to the Hubble flow and eventually form black holes. The fate of the bubble itself depends on the resulting black hole mass. If the mass is smaller than a certain critical value, the bubble collapses to a singularity. Otherwise, the bubble interior inflates, forming a baby universe, which is connected to the exterior FRW region by a wormhole. A similar black hole formation mechanism operates for spherical domain walls nucleating during inflation. As an illustrative example, we studied the black hole mass spectrum in the domain wall scenario, assuming that domain walls interact with matter only gravitationally. Our results indicate that, depending on the model parameters, black holes produced in…
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