Tolman-Oppenheimer-Volkoff Equations and their implications or the structures of relativistic Stars in f(T) gravity

Abstract

We investigate in this paper the structures of neutron and quark stars in f(T) theory of gravity where T denotes the torsion scalar. Attention is attached to the TOV type equations of this theory and numerical integrations of these equations are performed with suitable EoS. We search for the deviation of the mass-radius diagrams for power-law and exponential type correction from the TT gravity. Our results show that for some values of the input parameters appearing in the considered models, f(T) theory promotes more the structures of the relativistic stars, in consistency with the observational data.

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Cited by in corpus (11)

• Quark Stars in $f(T,\mathcal{T})-$Gravity
• Compact stars in $f(T)$ extended theory of gravity
• A Perturbative Approach to Neutron Stars in $f(T,\mathcal{T})-$Gravity
• Charge Gravastars in $f(T)$ Modified Gravity
• Neutron Star in Covariant $f(Q)$ gravity
• Compact stars in $f(T)=T+\xi T^{\beta }$ gravity
• Solving Tolman-Oppenheimer-Volkoff equations in $f(T)$ gravity: a novel approach applied to polytropic equations of state
• Solving Tolman-Oppenheimer-Volkoff equations in $f(T)$ gravity: a novel approach
• Mass of compact stars in f(T) gravity
• Polytropic Stars in $f(Q)=Q+\xi Q^2$ covariant formulation
• Isotropic stars in higher-order torsion scalar theories