Physical Attributes of Bardeen Stellar Structures in fR Gravity
The main aim of our study is to explore some relativistic configurations of compact object solution in the background of fR gravity, by adopting the Krori-Barua spacetime. In this regard, we establish the field equations for spherically symmetric spacetime along with charged anisotropic matter sourc...
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2021
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oai:doaj.org-article:f6af62c453f840aeb4aaac323acc97032021-11-29T00:55:28ZPhysical Attributes of Bardeen Stellar Structures in fR Gravity1687-736510.1155/2021/4742306https://doaj.org/article/f6af62c453f840aeb4aaac323acc97032021-01-01T00:00:00Zhttp://dx.doi.org/10.1155/2021/4742306https://doaj.org/toc/1687-7365The main aim of our study is to explore some relativistic configurations of compact object solution in the background of fR gravity, by adopting the Krori-Barua spacetime. In this regard, we establish the field equations for spherically symmetric spacetime along with charged anisotropic matter source by assuming the specific form of the metric potentials, i.e., νr=Br2+C and λr=Ar2. Further, to calculate the constant values, we consider the Bardeen model as an exterior spacetime at the surface boundary. To ensure the viability of the fR gravity model, the physical characteristics including energy density, pressure components, energy bonds, equilibrium condition, Herrera cracking concept, mass-radius relation, and adiabatic index are analyzed in detail. It is observed that all the outcomes by graphical exploration and tabular figures show that the Bardeen black hole model describes the physically realistic stellar structures.M. Farasat ShamirAmmara UsmanTayyaba NazHindawi LimitedarticlePhysicsQC1-999ENAdvances in High Energy Physics, Vol 2021 (2021) |
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Physics QC1-999 M. Farasat Shamir Ammara Usman Tayyaba Naz Physical Attributes of Bardeen Stellar Structures in fR Gravity |
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The main aim of our study is to explore some relativistic configurations of compact object solution in the background of fR gravity, by adopting the Krori-Barua spacetime. In this regard, we establish the field equations for spherically symmetric spacetime along with charged anisotropic matter source by assuming the specific form of the metric potentials, i.e., νr=Br2+C and λr=Ar2. Further, to calculate the constant values, we consider the Bardeen model as an exterior spacetime at the surface boundary. To ensure the viability of the fR gravity model, the physical characteristics including energy density, pressure components, energy bonds, equilibrium condition, Herrera cracking concept, mass-radius relation, and adiabatic index are analyzed in detail. It is observed that all the outcomes by graphical exploration and tabular figures show that the Bardeen black hole model describes the physically realistic stellar structures. |
format |
article |
author |
M. Farasat Shamir Ammara Usman Tayyaba Naz |
author_facet |
M. Farasat Shamir Ammara Usman Tayyaba Naz |
author_sort |
M. Farasat Shamir |
title |
Physical Attributes of Bardeen Stellar Structures in fR Gravity |
title_short |
Physical Attributes of Bardeen Stellar Structures in fR Gravity |
title_full |
Physical Attributes of Bardeen Stellar Structures in fR Gravity |
title_fullStr |
Physical Attributes of Bardeen Stellar Structures in fR Gravity |
title_full_unstemmed |
Physical Attributes of Bardeen Stellar Structures in fR Gravity |
title_sort |
physical attributes of bardeen stellar structures in fr gravity |
publisher |
Hindawi Limited |
publishDate |
2021 |
url |
https://doaj.org/article/f6af62c453f840aeb4aaac323acc9703 |
work_keys_str_mv |
AT mfarasatshamir physicalattributesofbardeenstellarstructuresinfrgravity AT ammarausman physicalattributesofbardeenstellarstructuresinfrgravity AT tayyabanaz physicalattributesofbardeenstellarstructuresinfrgravity |
_version_ |
1718407809642528768 |