Constraining study of charged gravastars solutions in symmetric teleparallel gravity

Fuente: arXiv
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Hauptverfasser: Javed, Faisal, Waseem, Arfa, Mustafa, G., Tchier, Fairouz, Atamurotov, Farruh, Ahmedov, Bobomurat, Abdujabbarov, Ahmadjon
Format: Preprint
Veröffentlicht: 2024
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author Javed, Faisal
Waseem, Arfa
Mustafa, G.
Tchier, Fairouz
Atamurotov, Farruh
Ahmedov, Bobomurat
Abdujabbarov, Ahmadjon
author_facet Javed, Faisal
Waseem, Arfa
Mustafa, G.
Tchier, Fairouz
Atamurotov, Farruh
Ahmedov, Bobomurat
Abdujabbarov, Ahmadjon
contents This study explores the effect of charge on a special astronomical object known as a gravastar, which is viewed as an alternative to a black hole. Based on the conjecture put out by Mazur and Mottola in general relativity, the study primarily focuses on the consequences of $f(Q)$ gravity. The internal domain, the intermediate shell, and the external domain are the three separate sections that make up a gravastar. Using a particular $f(Q)$ gravity model that includes conformal Killing vectors to analyze these areas, we discover that the inner domain shows a repulsive force on the spherical shell since it is assumed that pressure is equivalent to negative energy density. The intermediate shell is made up of ultrarelativistic plasma and pressure, which is proportional to energy density and balances the repulsive force from the interior domain. For exterior region, we use two appraoches as first we calculate the vacuum exact solution and secondly considered as the Reissner-Nordström metric. Then, we match these spacetimes through junction condition and explore the stability constraints for both cases. Our results show that charged gravastar solutions with non-singular physical parameters including length, energy, entropy, and equation of state parameter are physically realistic.
format Preprint
id arxiv_https___arxiv_org_abs_2403_01405
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Constraining study of charged gravastars solutions in symmetric teleparallel gravity
Javed, Faisal
Waseem, Arfa
Mustafa, G.
Tchier, Fairouz
Atamurotov, Farruh
Ahmedov, Bobomurat
Abdujabbarov, Ahmadjon
General Relativity and Quantum Cosmology
This study explores the effect of charge on a special astronomical object known as a gravastar, which is viewed as an alternative to a black hole. Based on the conjecture put out by Mazur and Mottola in general relativity, the study primarily focuses on the consequences of $f(Q)$ gravity. The internal domain, the intermediate shell, and the external domain are the three separate sections that make up a gravastar. Using a particular $f(Q)$ gravity model that includes conformal Killing vectors to analyze these areas, we discover that the inner domain shows a repulsive force on the spherical shell since it is assumed that pressure is equivalent to negative energy density. The intermediate shell is made up of ultrarelativistic plasma and pressure, which is proportional to energy density and balances the repulsive force from the interior domain. For exterior region, we use two appraoches as first we calculate the vacuum exact solution and secondly considered as the Reissner-Nordström metric. Then, we match these spacetimes through junction condition and explore the stability constraints for both cases. Our results show that charged gravastar solutions with non-singular physical parameters including length, energy, entropy, and equation of state parameter are physically realistic.
title Constraining study of charged gravastars solutions in symmetric teleparallel gravity
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2403.01405