Magnetic black universes and wormholes with a phantom scalar
S.V. Bolokhov, K.A. Bronnikov, M.V. Skvortsova

TL;DR
This paper presents new explicit solutions in general relativity featuring phantom scalar fields that describe traversable wormholes and regular black holes, including black universes with diverse horizon structures.
Contribution
It introduces a variety of new regular black hole and wormhole solutions with phantom scalar fields, expanding the known configurations and potential cosmological models.
Findings
Solutions include black universes with expanding interiors
Configurations contain up to four Killing horizons
Diverse structures of regular black holes are demonstrated
Abstract
We construct explicit examples of globally regular static, spherically symmetric solutions in general relativity with scalar and electromagnetic fields which describe traversable wormholes (with flat and AdS asymptotics) and regular black holes, in particular, black universes. A black universe is a nonsingular black hole where, beyond the horizon, instead of a singularity, there is an expanding, asymptotically isotropic universe. The scalar field in these solutions is phantom (i.e., its kinetic energy is negative), minimally coupled to gravity and has a nonzero self-interaction potential. The configurations obtained are quite diverse and contain different numbers of Killing horizons, from zero to four. This substantially widens the list of known structures of regular black hole configurations. Such models can be of interest both as descriptions of local objects (black holes and…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
