Kerr–Schild metrics in teleparallel gravity

Abstract We show that the Kerr–Schild ansatz can be extended from the metric to the tetrad, and then to teleparallel gravity where curvature vanishes but torsion does not. We derive the equations of motion for the Kerr–Schild null vector, and describe the solution for a rotating black hole in this f...

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Main Author: Markus B. Fröb
Format: Article
Language:English
Published: SpringerOpen 2021-08-01
Series:European Physical Journal C: Particles and Fields
Online Access:https://doi.org/10.1140/epjc/s10052-021-09551-5
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spelling doaj-4cc75e7545784f589f9eaaff3fa894372021-08-29T11:16:14ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522021-08-0181811110.1140/epjc/s10052-021-09551-5Kerr–Schild metrics in teleparallel gravityMarkus B. Fröb0Institut für Theoretische Physik, Universität LeipzigAbstract We show that the Kerr–Schild ansatz can be extended from the metric to the tetrad, and then to teleparallel gravity where curvature vanishes but torsion does not. We derive the equations of motion for the Kerr–Schild null vector, and describe the solution for a rotating black hole in this framework. It is shown that the solution depends on the chosen tetrad in a non-trivial way if the spin connection is fixed to be the one of the flat background spacetime. We show furthermore that any Kerr–Schild solution with a flat background is also a solution of $$f({\mathcal {T}})$$ f ( T ) gravity.https://doi.org/10.1140/epjc/s10052-021-09551-5
collection DOAJ
language English
format Article
sources DOAJ
author Markus B. Fröb
spellingShingle Markus B. Fröb
Kerr–Schild metrics in teleparallel gravity
European Physical Journal C: Particles and Fields
author_facet Markus B. Fröb
author_sort Markus B. Fröb
title Kerr–Schild metrics in teleparallel gravity
title_short Kerr–Schild metrics in teleparallel gravity
title_full Kerr–Schild metrics in teleparallel gravity
title_fullStr Kerr–Schild metrics in teleparallel gravity
title_full_unstemmed Kerr–Schild metrics in teleparallel gravity
title_sort kerr–schild metrics in teleparallel gravity
publisher SpringerOpen
series European Physical Journal C: Particles and Fields
issn 1434-6044
1434-6052
publishDate 2021-08-01
description Abstract We show that the Kerr–Schild ansatz can be extended from the metric to the tetrad, and then to teleparallel gravity where curvature vanishes but torsion does not. We derive the equations of motion for the Kerr–Schild null vector, and describe the solution for a rotating black hole in this framework. It is shown that the solution depends on the chosen tetrad in a non-trivial way if the spin connection is fixed to be the one of the flat background spacetime. We show furthermore that any Kerr–Schild solution with a flat background is also a solution of $$f({\mathcal {T}})$$ f ( T ) gravity.
url https://doi.org/10.1140/epjc/s10052-021-09551-5
work_keys_str_mv AT markusbfrob kerrschildmetricsinteleparallelgravity
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