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Main Authors: Gul, M. Zeeshan, Javed, Faisal, Sharif, M., Alkarni, Shalan
Format: Preprint
Published: 2024
Subjects:
Online Access:https://arxiv.org/abs/2412.01411
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author Gul, M. Zeeshan
Javed, Faisal
Sharif, M.
Alkarni, Shalan
author_facet Gul, M. Zeeshan
Javed, Faisal
Sharif, M.
Alkarni, Shalan
contents This research paper investigates the impact of non-metricity and matter source on the geometry of charged spheres in the presence of anisotropic matter configuration. We use a specific model of extended symmetric teleparallel theory to minimize the complexity of the field equations. Moreover, the feasible non-singular solutions are used to examine the interior composition of the charged spheres. The Darmois junction conditions are used to determine the unknown constants in the metric coefficients. We explore some significant properties in the interior of compact stars under consideration to check their viable existence in this modified framework. The equilibrium state of the charged spheres is discussed using the Tolman-Oppenheimer-Volkoff equation and stability is analyzed by sound speed and Herrera cracking approach. We find that the charged spheres in this theoretical framework are physically viable and stable.
format Preprint
id arxiv_https___arxiv_org_abs_2412_01411
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Exploring the viability of charged Spheres admitting non-metricity and matter source
Gul, M. Zeeshan
Javed, Faisal
Sharif, M.
Alkarni, Shalan
General Relativity and Quantum Cosmology
This research paper investigates the impact of non-metricity and matter source on the geometry of charged spheres in the presence of anisotropic matter configuration. We use a specific model of extended symmetric teleparallel theory to minimize the complexity of the field equations. Moreover, the feasible non-singular solutions are used to examine the interior composition of the charged spheres. The Darmois junction conditions are used to determine the unknown constants in the metric coefficients. We explore some significant properties in the interior of compact stars under consideration to check their viable existence in this modified framework. The equilibrium state of the charged spheres is discussed using the Tolman-Oppenheimer-Volkoff equation and stability is analyzed by sound speed and Herrera cracking approach. We find that the charged spheres in this theoretical framework are physically viable and stable.
title Exploring the viability of charged Spheres admitting non-metricity and matter source
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2412.01411