Stellar equilibrium configurations of compact stars in f ( R , T ) theory of gravity

In this article we study the hydrostatic equilibrium configuration of neutron stars and strange stars, whose fluid pressure is computed from the equations of state p =ωρ 5/3 and p =0.28(ρ−4ℬ), respectively, with ω and ℬ being constants and ρ the energy density of the fluid. We start by deriving the ... View More