Field Equations and Radial Solutions in a Noncommutative Spherically Symmetric Geometry

We study a noncommutative theory of gravity in the framework of torsional spacetime. This theory is based on a Lagrangian obtained by applying the technique of dimensional reduction of noncommutative gauge theory and that the yielded diffeomorphism invariant field theory can be made equivalent to a...

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Main Author: Aref Yazdani
Format: Article
Language:English
Published: Wiley 2014-01-01
Series:Advances in High Energy Physics
Online Access:http://dx.doi.org/10.1155/2014/349659
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author Aref Yazdani
author_facet Aref Yazdani
author_sort Aref Yazdani
collection DOAJ
description We study a noncommutative theory of gravity in the framework of torsional spacetime. This theory is based on a Lagrangian obtained by applying the technique of dimensional reduction of noncommutative gauge theory and that the yielded diffeomorphism invariant field theory can be made equivalent to a teleparallel formulation of gravity. Field equations are derived in the framework of teleparallel gravity through Weitzenbock geometry. We solve these field equations by considering a mass that is distributed spherically symmetrically in a stationary static spacetime in order to obtain a noncommutative line element. This new line element interestingly reaffirms the coherent state theory for a noncommutative Schwarzschild black hole. For the first time, we derive the Newtonian gravitational force equation in the commutative relativity framework, and this result could provide the possibility to investigate examples in various topics in quantum and ordinary theories of gravity.
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spelling doaj-art-de0c2ada28ad4195b281dbee474cba9b2025-02-03T05:52:41ZengWileyAdvances in High Energy Physics1687-73571687-73652014-01-01201410.1155/2014/349659349659Field Equations and Radial Solutions in a Noncommutative Spherically Symmetric GeometryAref Yazdani0Department of Physics, Faculty of Basic Sciences, University of Mazandaran, P.O. Box 47416-95447, Babolsar, IranWe study a noncommutative theory of gravity in the framework of torsional spacetime. This theory is based on a Lagrangian obtained by applying the technique of dimensional reduction of noncommutative gauge theory and that the yielded diffeomorphism invariant field theory can be made equivalent to a teleparallel formulation of gravity. Field equations are derived in the framework of teleparallel gravity through Weitzenbock geometry. We solve these field equations by considering a mass that is distributed spherically symmetrically in a stationary static spacetime in order to obtain a noncommutative line element. This new line element interestingly reaffirms the coherent state theory for a noncommutative Schwarzschild black hole. For the first time, we derive the Newtonian gravitational force equation in the commutative relativity framework, and this result could provide the possibility to investigate examples in various topics in quantum and ordinary theories of gravity.http://dx.doi.org/10.1155/2014/349659
spellingShingle Aref Yazdani
Field Equations and Radial Solutions in a Noncommutative Spherically Symmetric Geometry
Advances in High Energy Physics
title Field Equations and Radial Solutions in a Noncommutative Spherically Symmetric Geometry
title_full Field Equations and Radial Solutions in a Noncommutative Spherically Symmetric Geometry
title_fullStr Field Equations and Radial Solutions in a Noncommutative Spherically Symmetric Geometry
title_full_unstemmed Field Equations and Radial Solutions in a Noncommutative Spherically Symmetric Geometry
title_short Field Equations and Radial Solutions in a Noncommutative Spherically Symmetric Geometry
title_sort field equations and radial solutions in a noncommutative spherically symmetric geometry
url http://dx.doi.org/10.1155/2014/349659
work_keys_str_mv AT arefyazdani fieldequationsandradialsolutionsinanoncommutativesphericallysymmetricgeometry