This work aims to investigate the behaviour of compact stars in the background of f (R, T)
f(R,T) theory of gravity. For current work, we consider the Krori‐Barua metric potential ie, ν …

In this paper, we present an anisotropic solution for static and spherically symmetric self-
gravitating systems by demanding the vanishing of the complexity factor (Herrera in Phys …

We investigate the equilibrium and radial stability of spherically symmetric relativistic stars,
considering a polytropic equation of state (EoS), within the framework of f (R, T) gravity with …

Millisecond pulsars are the perfect testable to examine potential matter-geometry coupling
and its physical consequences in the context of the recent Neutron Star Interior Composition …

The spherically symmetric dark energy (DE) stellar model is presented here within the
context of the f (Q) theory of gravity. In order to develop the model, we take into account the …

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 …

Three different exact solutions to the gravitational equations are formulated in this paper in
the context of Rastall theory using the gravitational decoupling strategy. For doing so, the …

We develop multiple analytical solutions to the Rastall field equations using a recently
proposed scheme, named the gravitational decoupling. In order to do this, we assume a …

The compact stars are promising candidates associated with the generation of gravitational
waves (GWs). In this work, we study a special type of compact stars known as strange stars …

In this work, a non-singular spherically symmetric charged anisotropic stellar object has
been obtained in the context of f (R, T)-gravity theory. The field equations in modified f (R, T) …