Axially Symmetric-dS Solution in Teleparallel f(T) Gravity Theories

We apply a tetrad field with six unknown functions to Einstein field equations. Exact vacuum solution, which represents axially symmetric-dS spacetime, is derived. We multiply the tetrad field of the derived solution by a local Lorentz transformation which involves a generalization of the angle ϕ an...

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Main Author: Gamal G. L. Nashed
Format: Article
Language:English
Published: Wiley 2015-01-01
Series:Advances in High Energy Physics
Online Access:http://dx.doi.org/10.1155/2015/915928
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author Gamal G. L. Nashed
author_facet Gamal G. L. Nashed
author_sort Gamal G. L. Nashed
collection DOAJ
description We apply a tetrad field with six unknown functions to Einstein field equations. Exact vacuum solution, which represents axially symmetric-dS spacetime, is derived. We multiply the tetrad field of the derived solution by a local Lorentz transformation which involves a generalization of the angle ϕ and get a new tetrad field. Using this tetrad, we get a differential equation from the scalar torsion T=TαμνSαμν. Solving this differential equation we obtain a solution to the f(T) gravity theories under certain conditions on the form of f(T) and its first derivatives. Finally, we calculate the scalars of Riemann Christoffel tensor, Ricci tensor, Ricci scalar, torsion tensor, and its contraction to explain the singularities associated with this solution.
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institution Kabale University
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series Advances in High Energy Physics
spelling doaj-art-59fda2adf71e45378e20515e632aa7ff2025-02-03T01:12:12ZengWileyAdvances in High Energy Physics1687-73571687-73652015-01-01201510.1155/2015/915928915928Axially Symmetric-dS Solution in Teleparallel f(T) Gravity TheoriesGamal G. L. Nashed0Centre for Theoretical Physics, The British University in Egypt, P.O. Box 43, Shorouk City 11837, EgyptWe apply a tetrad field with six unknown functions to Einstein field equations. Exact vacuum solution, which represents axially symmetric-dS spacetime, is derived. We multiply the tetrad field of the derived solution by a local Lorentz transformation which involves a generalization of the angle ϕ and get a new tetrad field. Using this tetrad, we get a differential equation from the scalar torsion T=TαμνSαμν. Solving this differential equation we obtain a solution to the f(T) gravity theories under certain conditions on the form of f(T) and its first derivatives. Finally, we calculate the scalars of Riemann Christoffel tensor, Ricci tensor, Ricci scalar, torsion tensor, and its contraction to explain the singularities associated with this solution.http://dx.doi.org/10.1155/2015/915928
spellingShingle Gamal G. L. Nashed
Axially Symmetric-dS Solution in Teleparallel f(T) Gravity Theories
Advances in High Energy Physics
title Axially Symmetric-dS Solution in Teleparallel f(T) Gravity Theories
title_full Axially Symmetric-dS Solution in Teleparallel f(T) Gravity Theories
title_fullStr Axially Symmetric-dS Solution in Teleparallel f(T) Gravity Theories
title_full_unstemmed Axially Symmetric-dS Solution in Teleparallel f(T) Gravity Theories
title_short Axially Symmetric-dS Solution in Teleparallel f(T) Gravity Theories
title_sort axially symmetric ds solution in teleparallel f t gravity theories
url http://dx.doi.org/10.1155/2015/915928
work_keys_str_mv AT gamalglnashed axiallysymmetricdssolutioninteleparallelftgravitytheories