2022
DOI: 10.3847/1538-4357/ac9410
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Impact of Rastall Gravity on Mass, Radius, and Sound Speed of the Pulsar PSR J0740+6620

Abstract: Millisecond pulsars are perfect laboratories to test possible matter–geometry coupling and its physical implications in light of recent Neutron Star Interior Composition Explorer (NICER) observations. We apply Rastall field equations of gravity, where matter and geometry are nonminimally coupled, to Krori–Barua interior spacetime whereas the matter source is assumed to be anisotropic fluid. We show that all physical quantities inside the star can be expressed in terms of Rastall, ϵ, and compactness, C = 2GM/Rc… Show more

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Cited by 26 publications
(7 citation statements)
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“…Remarkably, other physical constraints put more restrictive bounds on the compactness in strong anisotropic cases [32][33][34][35]. Same conclusion has been obtained when nonminimal coupling between geometry and matter is considered [26,36,37]. In this sense, it is useful to examine this constraint within the quadratic f (R) gravity as considered in the present study.…”
Section: Equation Of State and Mass-radius Relationsupporting
confidence: 57%
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“…Remarkably, other physical constraints put more restrictive bounds on the compactness in strong anisotropic cases [32][33][34][35]. Same conclusion has been obtained when nonminimal coupling between geometry and matter is considered [26,36,37]. In this sense, it is useful to examine this constraint within the quadratic f (R) gravity as considered in the present study.…”
Section: Equation Of State and Mass-radius Relationsupporting
confidence: 57%
“…In spite of the capability of the model to lower the speed of sound in comparison to the GR or quadratic gravity with positive ϵ cases, it is still above the conjectured conformal upper bound on the maximum sound speed c 2 s = c 2 /3. This result may favor matter-geometry nonminimal coupling scenario to provide better framework for treating that issue as suggested by [26,37,84].…”
Section: Jcap09(2023)038mentioning
confidence: 90%
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“…Here F h and F g are the hydrostatic and the gravitational forces. We defined the different forces as (Nashed & El Hanafy 2022;El Hanafy 2022):…”
Section: The Adiabatic and Hydrodynamic Equilibrium Conditionsmentioning
confidence: 99%
“…of PSR J0740+6620 was studied in Ref. [62]. Considering perfect fluid spheres, the impact of Rastall parameter was investigated in Ref.…”
Section: Introductionmentioning
confidence: 99%