The Mass-Radius relation for Quark Stars in Energy-Momentum Squared Gravity
arXiv:2206.10371 · doi:10.1016/j.aop.2022.169149
Abstract
We study the structure of quark stars (QSs) adopting homogeneously confined matter inside the star with a 3-flavor neutral charge and a fixed strange quark mass . We explore the internal structure, and the physical properties of specific classes of QSs in the recently proposed energy-momentum squared gravity (EMSG). Also, we obtain the mass-radius and mass-central energy density relations for QS using the QCD motivated EoS. The maximum mass for QSs in EMSG is investigated depending on the presence and absence of the free parameter . Furthermore, the stability of stars is determined by the condition . We observe that consideration of the EMSG has specific contributions to the structure of QSs.
8 pages, 5 figures, version accepted in Annals of Physics
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Cited by in corpus (6)
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- Gravitationally induced matter creation in scalar-tensor gravity
- Relativistic structure of charged quark stars in energy-momentum squared gravity
- Weak field and slow motion limits in energy-momentum powered gravity
- Relativistic binary systems in scale-independent energy-momentum squared gravity
- Cosmological perturbations in the energy-momentum squared gravity theory: constraints from gravitational wave standard sirens and redshift space distortions