Exact Axially Symmetric Solution in f(T) Gravity Theory

A general tetrad field with sixteen unknown functions is applied to the field equations of f(T) gravity theory. An analytic vacuum solution is derived with two constants of integration and an angle Φ that depends on the angle coordinate ϕ and radial coordinate r. The tetrad field of this solution is...

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Main Author: Gamal G. L. Nashed
Format: Article
Language:English
Published: Wiley 2014-01-01
Series:Advances in High Energy Physics
Online Access:http://dx.doi.org/10.1155/2014/857936
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author Gamal G. L. Nashed
author_facet Gamal G. L. Nashed
author_sort Gamal G. L. Nashed
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description A general tetrad field with sixteen unknown functions is applied to the field equations of f(T) gravity theory. An analytic vacuum solution is derived with two constants of integration and an angle Φ that depends on the angle coordinate ϕ and radial coordinate r. The tetrad field of this solution is axially symmetric and the scalar torsion vanishes. We calculate the associated metric of the derived solution and show that it represents Kerr spacetime. Finally, we show that the derived solution can be described by two local Lorentz transformations in addition to a tetrad field that is the square root of the Kerr metric. One of these local Lorentz transformations is a special case of Euler’s angles and the other represents a boost when the rotation parameter vanishes.
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spelling doaj-art-ef538aa97a4045bcb1f93bb2dcf5bd0a2025-08-20T03:21:15ZengWileyAdvances in High Energy Physics1687-73571687-73652014-01-01201410.1155/2014/857936857936Exact Axially Symmetric Solution in f(T) Gravity TheoryGamal G. L. Nashed0Centre for Theoretical Physics, The British University in Egypt, Sherouk City 11837, P.O. Box 43, Cairo, EgyptA general tetrad field with sixteen unknown functions is applied to the field equations of f(T) gravity theory. An analytic vacuum solution is derived with two constants of integration and an angle Φ that depends on the angle coordinate ϕ and radial coordinate r. The tetrad field of this solution is axially symmetric and the scalar torsion vanishes. We calculate the associated metric of the derived solution and show that it represents Kerr spacetime. Finally, we show that the derived solution can be described by two local Lorentz transformations in addition to a tetrad field that is the square root of the Kerr metric. One of these local Lorentz transformations is a special case of Euler’s angles and the other represents a boost when the rotation parameter vanishes.http://dx.doi.org/10.1155/2014/857936
spellingShingle Gamal G. L. Nashed
Exact Axially Symmetric Solution in f(T) Gravity Theory
Advances in High Energy Physics
title Exact Axially Symmetric Solution in f(T) Gravity Theory
title_full Exact Axially Symmetric Solution in f(T) Gravity Theory
title_fullStr Exact Axially Symmetric Solution in f(T) Gravity Theory
title_full_unstemmed Exact Axially Symmetric Solution in f(T) Gravity Theory
title_short Exact Axially Symmetric Solution in f(T) Gravity Theory
title_sort exact axially symmetric solution in f t gravity theory
url http://dx.doi.org/10.1155/2014/857936
work_keys_str_mv AT gamalglnashed exactaxiallysymmetricsolutioninftgravitytheory