2023
DOI: 10.1142/s0217751x23501531
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Anisotropic stellar modeling with clouds of string and quintessence field in Rastall gravity

Allah Ditta,
Xia Tiecheng,
Irfan Mahmood
et al.

Abstract: This paper proposes a new framework to investigate the spherically symmetric of anisotropic stars with clouds of strings and quintessence field in Rastall gravity. We develop the field equations in a spherically symmetric space–time with a quintessence field and clouds of string. We utilize the mass and radius of Her X-1, Vela X-1, SMC X-1, SAX J1808 0.4-3658 and 4 U 1538-52, which are well mentioned in the literature. We applied the matching conditions by considering outer space calculated in Rastall gravity … Show more

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Cited by 1 publication
(5 citation statements)
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“…Moreover, our results in the case of quintessence and the cloud of strings field are less dense than the simple quintessence field. In our recent studies [16,20], we studied the quintessence and the cloud of strings stellar configurations using the ansatz of f (Q) gravity and Rastall gravity, but this study is based upon the paradigm of General relativity. Moreover, our results in this study are denser than the Rastall gravity and less dense than the f (Q) gravity paradigm.…”
Section: Discussionmentioning
confidence: 99%
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“…Moreover, our results in the case of quintessence and the cloud of strings field are less dense than the simple quintessence field. In our recent studies [16,20], we studied the quintessence and the cloud of strings stellar configurations using the ansatz of f (Q) gravity and Rastall gravity, but this study is based upon the paradigm of General relativity. Moreover, our results in this study are denser than the Rastall gravity and less dense than the f (Q) gravity paradigm.…”
Section: Discussionmentioning
confidence: 99%
“…However, there are six unknowns in each of the three equations, which are η (r), ϑ(r), ρ, p r , p t , ρ q ; hence, it is impossible to determine the explicit solutions. To this end, we have taken into account EoS (16) and metric potential functions η(r), ϑ(r) computed using the Karmarkar condition, which for finite values of r are finite everywhere, given as [67]:…”
Section: S S = S S = S S S = S Bs Bs S Smentioning
confidence: 99%
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