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...

Descripción completa

Guardado en:
Detalles Bibliográficos
Autores principales: M. Farasat Shamir, Ammara Usman, Tayyaba Naz
Formato: article
Lenguaje:EN
Publicado: Hindawi Limited 2021
Materias:
Acceso en línea:https://doaj.org/article/f6af62c453f840aeb4aaac323acc9703
Etiquetas: Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
id oai:doaj.org-article:f6af62c453f840aeb4aaac323acc9703
record_format dspace
spelling 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)
institution DOAJ
collection DOAJ
language EN
topic Physics
QC1-999
spellingShingle Physics
QC1-999
M. Farasat Shamir
Ammara Usman
Tayyaba Naz
Physical Attributes of Bardeen Stellar Structures in fR Gravity
description 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