Black holes in scalar multipolar universes

Recently, a scalar counterpart of the Schwarzschild-Melvin Universe was reported [1] . We show this solution is a special case of a Schwarzschild black hole/mass in a scalar multipolar Universe, that can be constructed algebraically combining known vacuum solutions. This builds on the generalized Weyl construction for scalar-vacuum, that admits two, fully decoupled, independent harmonic functions: one for the gravitational sector and another for the scalar sector. Harmonic solutions with growing multipoles lead to naked singularities (at spatial infinity), including for the scalar counterpart of the Schwarzschild-Melvin; harmonic solutions with decaying (scalar) multipoles are asymptotically flat, but have a singular horizon, in accordance with no-scalar-hair theorems. The scalar-vacuum model can be mapped to a five dimensional pure gravity construction via Kaluza-Klein oxidization and, in this way, to the corresponding D = 5 generalized Weyl construction.

Authors

Publication Details

Journal
Physics Letters B
Published
2024-11-27
DOI
https://doi.org/10.1016/j.physletb.2024.139160
Citations
1
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
0.66

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article

Black holes in scalar multipolar universes

Carlos Herdeiro
1 citations
Physics Letters B
Black Holes and Theoretical Physics
0.66
article

Black holes in scalar multipolar universes

Carlos Herdeiro
article en
1 citations

Abstract

Recently, a scalar counterpart of the Schwarzschild-Melvin Universe was reported [1] . We show this solution is a special case of a Schwarzschild black hole/mass in a scalar multipolar Universe, that can be constructed algebraically combining known vacuum solutions. This builds on the generalized Weyl construction for scalar-vacuum, that admits two, fully decoupled, independent harmonic functions: one for the gravitational sector and another for the scalar sector. Harmonic solutions with growing multipoles lead to naked singularities (at spatial infinity), including for the scalar counterpart of the Schwarzschild-Melvin; harmonic solutions with decaying (scalar) multipoles are asymptotically flat, but have a singular horizon, in accordance with no-scalar-hair theorems. The scalar-vacuum model can be mapped to a five dimensional pure gravity construction via Kaluza-Klein oxidization and, in this way, to the corresponding D = 5 generalized Weyl construction.

Physics Letters BVol. 860
Center for Research and Development in Mathematics and Applications, Fundação para a Ciência e a Tecnologia
Openalex Percentile: Top 14%
Black Holes and Theoretical Physics
0.66
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