Fan-Wang type regular black holes in Quasi-Topological Gravity

Fuente: arXiv
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Autori principali: Tsuda, Ren, Suzuki, Ryotaku, Tomizawa, Shinya
Natura: Preprint
Pubblicazione: 2026
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author Tsuda, Ren
Suzuki, Ryotaku
Tomizawa, Shinya
author_facet Tsuda, Ren
Suzuki, Ryotaku
Tomizawa, Shinya
contents We construct a class of regular black hole solutions of the Fan-Wang type within quasi-topological gravity (QTG) in arbitrary spacetime dimensions greater than four. In contrast to the original Fan-Wang solution, which was obtained in four-dimensional general relativity coupled to nonlinear electrodynamics, our higher-dimensional generalization does not require any matter fields. Instead, regularity is achieved purely through an infinite tower of higher-curvature corrections. We demonstrate that the Fan-Wang-type metric is a solution to the QTG field equations by explicitly determining the corresponding coupling constants for each curvature order. Within an appropriate parameter regime, the solution describes an asymptotically flat black hole spacetime with a regular center. Remarkably, even in the case of negative mass, the geometry can remain completely regular, in sharp contrast to Einstein gravity.
format Preprint
id arxiv_https___arxiv_org_abs_2602_16754
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Fan-Wang type regular black holes in Quasi-Topological Gravity
Tsuda, Ren
Suzuki, Ryotaku
Tomizawa, Shinya
General Relativity and Quantum Cosmology
High Energy Physics - Theory
We construct a class of regular black hole solutions of the Fan-Wang type within quasi-topological gravity (QTG) in arbitrary spacetime dimensions greater than four. In contrast to the original Fan-Wang solution, which was obtained in four-dimensional general relativity coupled to nonlinear electrodynamics, our higher-dimensional generalization does not require any matter fields. Instead, regularity is achieved purely through an infinite tower of higher-curvature corrections. We demonstrate that the Fan-Wang-type metric is a solution to the QTG field equations by explicitly determining the corresponding coupling constants for each curvature order. Within an appropriate parameter regime, the solution describes an asymptotically flat black hole spacetime with a regular center. Remarkably, even in the case of negative mass, the geometry can remain completely regular, in sharp contrast to Einstein gravity.
title Fan-Wang type regular black holes in Quasi-Topological Gravity
topic General Relativity and Quantum Cosmology
High Energy Physics - Theory
url https://arxiv.org/abs/2602.16754