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 …

We discuss spherically symmetric dynamical systems in the framework of a general model of
f (R) gravity, ie f (R)= R e ζ R, where ζ is a dimensional quantity in squared length units [L 2] …

In this paper, we obtain analytical solutions of Einstein field equations for a spherically
symmetric anisotropic matter distributions. For this purpose physically meaningful metric …

Within the framework of f (R, T) theories of gravity, we investigate the hydrostatic equilibrium
of anisotropic neutron stars with a physically relevant equation of state (EoS) for the radial …

This study introduces a pioneering approach to analyzing compact stars through Finslerian
geometry, which has not been previously explored in this context. By employing the Barthel …

We construct a new stellar compact object model in the regime of anisotropic pressure using
the framework of gravitational decoupling via minimal geometric deformation, with the …

This paper provides a simplified description for simulating the coupling of dark energy with
baryonic matter by considering a super-dense pulsar PSRJ1614-2230 as the model star …

In this study, we propose a streamlined approach to analyze the characteristics of compact
stars with a unique equation of state resulting from the hybridization of dark matter and …

In this paper we calculate the speed of sound for three phases that may exist inside a
magnetized hybrid neutron star at different density regions: A hadronic phase at low …

In our investigation, we pioneer the development of geometrically deformed strange stars
within the framework of teleparallel gravity theory through gravitational decoupling via the …