Anisotropic charged stellar models with modified Van der Waals EoS in f(Q) gravity
Abstract This paper is based on the study of compact stars in the context of electric fields and the nonmetricity effects of gravity. Due to this, we are motivated to build stellar models based on spherically symmetric space-time in f(Q) gravity. The space-time solution is obtained by Durgapal and B...
Main Authors: | , , , , |
---|---|
Format: | Article |
Language: | English |
Published: |
SpringerOpen
2023-03-01
|
Series: | European Physical Journal C: Particles and Fields |
Online Access: | https://doi.org/10.1140/epjc/s10052-023-11390-5 |
_version_ | 1797836279039131648 |
---|---|
author | Allah Ditta Xia Tiecheng Abdelghani Errehymy G. Mustafa S. K. Maurya |
author_facet | Allah Ditta Xia Tiecheng Abdelghani Errehymy G. Mustafa S. K. Maurya |
author_sort | Allah Ditta |
collection | DOAJ |
description | Abstract This paper is based on the study of compact stars in the context of electric fields and the nonmetricity effects of gravity. Due to this, we are motivated to build stellar models based on spherically symmetric space-time in f(Q) gravity. The space-time solution is obtained by Durgapal and Bannerji (Phys Rev D 27:328–331,1983) potential along with modified Van der Waals equation of state (EoS) $$p_r=\eta \rho ^2+ \frac{\beta \rho }{\gamma \rho +1}$$ p r = η ρ 2 + β ρ γ ρ + 1 by introducing a specific form of electric charge function $$q(r)=kr^3$$ q ( r ) = k r 3 . In order to validate our charge model, we used observational data from the literature for celestial objects like Her X-1, 4U 1538-52, SAX J1808.4-3658, and SMC X-1. Furthermore, we have also retrieved the uncharged effects of gravity for the model SMC X-1 by taking $$k=0$$ k = 0 . Our present physical analysis shows that all the obtained features for the present solution are in excellent agreement with the viable model as far as observational data is concerned. |
first_indexed | 2024-04-09T15:07:23Z |
format | Article |
id | doaj.art-5c5e73a9b5a84335b5844025499746d6 |
institution | Directory Open Access Journal |
issn | 1434-6052 |
language | English |
last_indexed | 2024-04-09T15:07:23Z |
publishDate | 2023-03-01 |
publisher | SpringerOpen |
record_format | Article |
series | European Physical Journal C: Particles and Fields |
spelling | doaj.art-5c5e73a9b5a84335b5844025499746d62023-04-30T11:25:30ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60522023-03-0183311610.1140/epjc/s10052-023-11390-5Anisotropic charged stellar models with modified Van der Waals EoS in f(Q) gravityAllah Ditta0Xia Tiecheng1Abdelghani Errehymy2G. Mustafa3S. K. Maurya4Department of Mathematics, Shanghai UniversityDepartment of Mathematics, Shanghai UniversityAstrophysics Research Centre, School of Mathematics, Statistics and Computer Science, University of KwaZulu-NatalDepartment of Physics, Zhejiang Normal UniversityDepartment of Mathematical and Physical Sciences, College of Arts and Sciences, University of NizwaAbstract This paper is based on the study of compact stars in the context of electric fields and the nonmetricity effects of gravity. Due to this, we are motivated to build stellar models based on spherically symmetric space-time in f(Q) gravity. The space-time solution is obtained by Durgapal and Bannerji (Phys Rev D 27:328–331,1983) potential along with modified Van der Waals equation of state (EoS) $$p_r=\eta \rho ^2+ \frac{\beta \rho }{\gamma \rho +1}$$ p r = η ρ 2 + β ρ γ ρ + 1 by introducing a specific form of electric charge function $$q(r)=kr^3$$ q ( r ) = k r 3 . In order to validate our charge model, we used observational data from the literature for celestial objects like Her X-1, 4U 1538-52, SAX J1808.4-3658, and SMC X-1. Furthermore, we have also retrieved the uncharged effects of gravity for the model SMC X-1 by taking $$k=0$$ k = 0 . Our present physical analysis shows that all the obtained features for the present solution are in excellent agreement with the viable model as far as observational data is concerned.https://doi.org/10.1140/epjc/s10052-023-11390-5 |
spellingShingle | Allah Ditta Xia Tiecheng Abdelghani Errehymy G. Mustafa S. K. Maurya Anisotropic charged stellar models with modified Van der Waals EoS in f(Q) gravity European Physical Journal C: Particles and Fields |
title | Anisotropic charged stellar models with modified Van der Waals EoS in f(Q) gravity |
title_full | Anisotropic charged stellar models with modified Van der Waals EoS in f(Q) gravity |
title_fullStr | Anisotropic charged stellar models with modified Van der Waals EoS in f(Q) gravity |
title_full_unstemmed | Anisotropic charged stellar models with modified Van der Waals EoS in f(Q) gravity |
title_short | Anisotropic charged stellar models with modified Van der Waals EoS in f(Q) gravity |
title_sort | anisotropic charged stellar models with modified van der waals eos in f q gravity |
url | https://doi.org/10.1140/epjc/s10052-023-11390-5 |
work_keys_str_mv | AT allahditta anisotropicchargedstellarmodelswithmodifiedvanderwaalseosinfqgravity AT xiatiecheng anisotropicchargedstellarmodelswithmodifiedvanderwaalseosinfqgravity AT abdelghanierrehymy anisotropicchargedstellarmodelswithmodifiedvanderwaalseosinfqgravity AT gmustafa anisotropicchargedstellarmodelswithmodifiedvanderwaalseosinfqgravity AT skmaurya anisotropicchargedstellarmodelswithmodifiedvanderwaalseosinfqgravity |