On electrogravity duality and black hole with global monopole

By resolving the Riemann curvature into electric and magnetic parts, Einstein’s equation can accordingly be written in terms of electric (active and passive) and magnetic parts. The electrogravity duality is defined by the interchange of active and passive parts. It turns out that in static and stationary spacetimes, there is a subset of the equations (that identifies the effective vacuum equation) that is sufficient to yield the vacuum solution. In spherically symmetric spacetime, the electrograv dual of the effective equation solves to give the Schwarzschild black hole with a global monopole. Interestingly, this is not so for axial symmetry, where the Kerr vacuum solution turns out to be electrograv self-dual. However, in the asymptotic limit where the effect of rotation dies out, the situation reverts to the static case, admitting a global monopole. This is also what follows when we apply the Newman-Janis transformation to the static black hole with a global monopole.

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Publication Details

Journal
Physics Letters B
Published
2025-10-27
DOI
https://doi.org/10.1016/j.physletb.2025.139980
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
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article

On electrogravity duality and black hole with global monopole

Chiranjeeb Singha, Naresh Dadhich
Physics Letters B
Black Holes and Theoretical Physics
article

On electrogravity duality and black hole with global monopole

Chiranjeeb Singha, Naresh Dadhich
article en

Abstract

By resolving the Riemann curvature into electric and magnetic parts, Einstein’s equation can accordingly be written in terms of electric (active and passive) and magnetic parts. The electrogravity duality is defined by the interchange of active and passive parts. It turns out that in static and stationary spacetimes, there is a subset of the equations (that identifies the effective vacuum equation) that is sufficient to yield the vacuum solution. In spherically symmetric spacetime, the electrograv dual of the effective equation solves to give the Schwarzschild black hole with a global monopole. Interestingly, this is not so for axial symmetry, where the Kerr vacuum solution turns out to be electrograv self-dual. However, in the asymptotic limit where the effect of rotation dies out, the situation reverts to the static case, admitting a global monopole. This is also what follows when we apply the Newman-Janis transformation to the static black hole with a global monopole.

Physics Letters BVol. 871
Inter-University Centre for Astronomy and Astrophysics (IN), University of KwaZulu-Natal (ZA)
Openalex Percentile: Top 86%
Black Holes and Theoretical Physics
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