Exploring nonsupersymmetric black holes with multiple bubbles in five-dimensional minimal supergravity

The topological censorship theorem suggests that higher-dimensional black holes can possess a domain of outer communication (DOC) of nontrivial topology. In this paper, we seek for a black hole coexisting with two bubbles adjacent to the horizon in five-dimensional minimal supergravity, under the assumptions of stationarity and biaxisymmetry. For simplicity, we also assume that the spacetime is symmetric under the exchange of the two axisymmetric Killing vectors. To find the solution, we combine the inverse scattering method and the Harrison transformation, and we present the conditions for the absence of conical, orbifold, and Dirac-Misner string singularities, respectively. As the result, we find that the black hole with topology of <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:msup><a:mi>S</a:mi><a:mn>3</a:mn></a:msup></a:math> or <c:math xmlns:c="http://www.w3.org/1998/Math/MathML" display="inline"><c:msup><c:mi>S</c:mi><c:mn>2</c:mn></c:msup><c:mo>×</c:mo><c:msup><c:mi>S</c:mi><c:mn>1</c:mn></c:msup></c:math> can be supported by two bubbles if we admit the conical singularities (deficits).

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2025-05-15
DOI
https://doi.org/10.1103/physrevd.111.104049
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
0.00

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article

Exploring nonsupersymmetric black holes with multiple bubbles in five-dimensional minimal supergravity

Ryotaku Suzuki, Shinya Tomizawa
Physical review. D/Physical review. D.
Black Holes and Theoretical Physics
article

Exploring nonsupersymmetric black holes with multiple bubbles in five-dimensional minimal supergravity

Ryotaku Suzuki, Shinya Tomizawa
article en

Abstract

The topological censorship theorem suggests that higher-dimensional black holes can possess a domain of outer communication (DOC) of nontrivial topology. In this paper, we seek for a black hole coexisting with two bubbles adjacent to the horizon in five-dimensional minimal supergravity, under the assumptions of stationarity and biaxisymmetry. For simplicity, we also assume that the spacetime is symmetric under the exchange of the two axisymmetric Killing vectors. To find the solution, we combine the inverse scattering method and the Harrison transformation, and we present the conditions for the absence of conical, orbifold, and Dirac-Misner string singularities, respectively. As the result, we find that the black hole with topology of <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:msup><a:mi>S</a:mi><a:mn>3</a:mn></a:msup></a:math> or <c:math xmlns:c="http://www.w3.org/1998/Math/MathML" display="inline"><c:msup><c:mi>S</c:mi><c:mn>2</c:mn></c:msup><c:mo>×</c:mo><c:msup><c:mi>S</c:mi><c:mn>1</c:mn></c:msup></c:math> can be supported by two bubbles if we admit the conical singularities (deficits).

Physical review. D/Physical review. D.Vol. 111(10)
Toyota Technological Institute (JP)
Japan Society for the Promotion of Science
Openalex Percentile: Top 95%
Black Holes and Theoretical Physics
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