Isotropic Stars in Higher-Order Torsion Scalar Theories

Two different nondiagonal tetrad spaces reproducing spherically symmetric spacetime are applied to the field equations of higher-order torsion scalar theories. Assuming the existence of conformal Killing vector, two isotropic solutions are derived. We show that the first solution is not stable while...

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Main Author: Gamal G. L. Nashed
Format: Article
Language:English
Published: Wiley 2016-01-01
Series:Advances in High Energy Physics
Online Access:http://dx.doi.org/10.1155/2016/7020162
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author Gamal G. L. Nashed
author_facet Gamal G. L. Nashed
author_sort Gamal G. L. Nashed
collection DOAJ
description Two different nondiagonal tetrad spaces reproducing spherically symmetric spacetime are applied to the field equations of higher-order torsion scalar theories. Assuming the existence of conformal Killing vector, two isotropic solutions are derived. We show that the first solution is not stable while the second one confirms a stable behavior. We also discuss the construction of the stellar model and show that one of our solutions is capable of such construction while the other is not. Finally, we discuss the generalized Tolman-Oppenheimer-Volkoff and show that one of our models has a tendency to equilibrium.
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spelling doaj-art-218fb0cf523a41b38836243d29c82c9e2025-02-03T05:45:27ZengWileyAdvances in High Energy Physics1687-73571687-73652016-01-01201610.1155/2016/70201627020162Isotropic Stars in Higher-Order Torsion Scalar TheoriesGamal G. L. Nashed0Centre for Theoretical Physics, The British University in Egypt, P.O. Box 43, El-Sherouk City 11837, EgyptTwo different nondiagonal tetrad spaces reproducing spherically symmetric spacetime are applied to the field equations of higher-order torsion scalar theories. Assuming the existence of conformal Killing vector, two isotropic solutions are derived. We show that the first solution is not stable while the second one confirms a stable behavior. We also discuss the construction of the stellar model and show that one of our solutions is capable of such construction while the other is not. Finally, we discuss the generalized Tolman-Oppenheimer-Volkoff and show that one of our models has a tendency to equilibrium.http://dx.doi.org/10.1155/2016/7020162
spellingShingle Gamal G. L. Nashed
Isotropic Stars in Higher-Order Torsion Scalar Theories
Advances in High Energy Physics
title Isotropic Stars in Higher-Order Torsion Scalar Theories
title_full Isotropic Stars in Higher-Order Torsion Scalar Theories
title_fullStr Isotropic Stars in Higher-Order Torsion Scalar Theories
title_full_unstemmed Isotropic Stars in Higher-Order Torsion Scalar Theories
title_short Isotropic Stars in Higher-Order Torsion Scalar Theories
title_sort isotropic stars in higher order torsion scalar theories
url http://dx.doi.org/10.1155/2016/7020162
work_keys_str_mv AT gamalglnashed isotropicstarsinhigherordertorsionscalartheories