Exact dynamical black hole solutions in five or higher dimensions

We construct new classes of the dynamical black hole solutions in five or higher dimensional Einstein-Maxwell theory, coupled to a dilaton field, in the presence of an arbitrary cosmological constant. The dilaton field interacts non-trivially with the Maxwell field, as well as the cosmological constant, with two arbitrary coupling constants. The solutions are non-stationary, and almost conformally regular everywhere. To construct the solutions, we use the four-dimensional Bianchi type IX geometry, as the base space. We find three different classes of solutions, based on the values of the coupling constants. We notice that our solutions could be asymptotically de-Sitter, anti-de-Sitter or flat. We find the relevant quantities of the solutions, and discuss the properties of the solutions.

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Publication Details

Journal
The European Physical Journal C
Published
2024-08-20
DOI
https://doi.org/10.1140/epjc/s10052-024-13203-9
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
0.00

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article

Exact dynamical black hole solutions in five or higher dimensions

Bardia H. Fahim, A. M. Ghezelbash
The European Physical Journal C
Black Holes and Theoretical Physics
article

Exact dynamical black hole solutions in five or higher dimensions

Bardia H. Fahim, A. M. Ghezelbash
article en

Abstract

We construct new classes of the dynamical black hole solutions in five or higher dimensional Einstein-Maxwell theory, coupled to a dilaton field, in the presence of an arbitrary cosmological constant. The dilaton field interacts non-trivially with the Maxwell field, as well as the cosmological constant, with two arbitrary coupling constants. The solutions are non-stationary, and almost conformally regular everywhere. To construct the solutions, we use the four-dimensional Bianchi type IX geometry, as the base space. We find three different classes of solutions, based on the values of the coupling constants. We notice that our solutions could be asymptotically de-Sitter, anti-de-Sitter or flat. We find the relevant quantities of the solutions, and discuss the properties of the solutions.

The European Physical Journal CVol. 84(8)
University of Saskatchewan (CA)
Natural Sciences and Engineering Research Council of Canada
Openalex Percentile: Top 96%
Black Holes and Theoretical Physics
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