Rotating black holes in a Randall-Sundrum brane with a cosmological constant

Rotating black holes in a Randall-Sundrum brane with a cosmological constant

In this work we have constructed axially symmetric vacuum solutions of the gravitational field equations in a Randall-Sundrum brane. A non-null effective cosmological constant is considered, and asymptotically de Sitter and anti-de Sitter spacetimes are obtained. The solutions describe rotating blac...

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Veröffentlicht in:arXiv.org 2013-01
Hauptverfasser: Neves, J C S, Molina, C
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Sprache:eng
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Congruences
Cosmological constant
Gravitational fields
Physics - Cosmology and Nongalactic Astrophysics
Physics - General Relativity and Quantum Cosmology
Physics - High Energy Physics - Theory
Rotation
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description In this work we have constructed axially symmetric vacuum solutions of the gravitational field equations in a Randall-Sundrum brane. A non-null effective cosmological constant is considered, and asymptotically de Sitter and anti-de Sitter spacetimes are obtained. The solutions describe rotating black holes in a four-dimensional brane. Optical features of the solutions are treated, emphasizing the rotation of the polarization vector along null congruences.
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subjects Congruences
Cosmological constant
Gravitational fields
Physics - Cosmology and Nongalactic Astrophysics
Physics - General Relativity and Quantum Cosmology
Physics - High Energy Physics - Theory
Rotation
title Rotating black holes in a Randall-Sundrum brane with a cosmological constant
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