2022
DOI: 10.1016/j.newast.2022.101815
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Anisotropic relativistic fluid spheres with a linear equation of state

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Cited by 10 publications
(3 citation statements)
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“…To clarify the situation, the last equation implies that this compact star results from the equilibrium between these three different forces, as is mentioned in Ref. [50]. In particular, if F p = 0, we obtain the standard TOV equation.…”
Section: Relativistic Stars In General Relativitymentioning
confidence: 86%
“…To clarify the situation, the last equation implies that this compact star results from the equilibrium between these three different forces, as is mentioned in Ref. [50]. In particular, if F p = 0, we obtain the standard TOV equation.…”
Section: Relativistic Stars In General Relativitymentioning
confidence: 86%
“…The equilibrium for a compact star is maintained by the balance of three forces, as established by the previous equation ( 8) [61]. It is noteworthy that if F p is equal to zero, then the standard TOV equation is obtained.…”
Section: Relativistic Spheres Within Grmentioning
confidence: 97%
“…Anisotropic compact stellar objects admitting a linear EOS was studied by [12]. [13] presented a class of relativistic solutions to Einstein field equations for an anisotropic matter distribution utilizing the Buchdahl ansatz for the metric function g rr . Recently, [14] investigated a charged anisotropic stellar solution in paraboloidal spacetime using a linear EOS.…”
Section: Introductionmentioning
confidence: 99%