We will follow the two-families scenario described in the accompanying paper, in which
compact stars having a very small radius and masses not exceeding about 1.5 M⊙ are …

In the current article, we study anisotropic spherically symmetric strange star under the
background of f (R, T) gravity using the metric potentials of Tolman–Kuchowicz type (Tolman …

In this article, we attempt to find a singularity free solution of Einstein's field equations for
compact stellar objects, precisely strange (quark) stars, considering Schwarzschild metric as …

Within the metric formalism of f (R) theories of gravity, where R is the Ricci scalar, we study
the hydrostatic equilibrium structure of compact stars with the inclusion of anisotropic …

In this article we try to present spherically symmetric isotropic strange star model under the
framework of f (R, Script T) theory of gravity. To this end, we consider that the Lagrangian …

We study strange stars in the framework of f (R, T) theory of gravity. To provide exact
solutions of the field equations it is considered that the gravitational Lagrangian can be …

We investigate the effects of the modified f (R, T) gravity on the charged strange quark stars
with the standard choice of f (R, T)= R+ 2χ T. Those types of stars are supposed to be made …

In the present work, we study about highly dense compact stars which are made of quarks,
specially strange quarks, adopting the Krori–Barua (KB)(Krori and Barua, 1975) metric in the …

We present spherically symmetric anisotropic charged strange stars under the framework of f
(R, T) gravity. For this we consider that the Lagrangian density is a linear function of R and T …

We attempt to study a singularity-free model for the spherically symmetric anisotropic
strange stars under Einstein's general theory of relativity by exploiting the Tolman …