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 …

In this work we investigate neutron stars (NS) in f (Script R, T) gravity for the case R+ 2λ
Script T, Script R is the Ricci scalar and Script T the trace of the energy-momentum tensor …

This work analyses the hydrostatic equilibrium configurations of strange stars in a non-
minimal geometry-matter coupling (GMC) theory of gravity. Those stars are made of strange …

In this work, we study the influence of f (R, T) gravity on rapidly rotating neutron stars. First
we discuss the main aspects of this modified theory of gravity where the gravitational …

A crucial aspect of wormhole (WH) physics is the inclusion of exotic matter, which requires
violating the null energy condition. Here, we explore the potential for WHs to be sustained by …

We discuss strange stars admixed with fermionic dark matter in the presence of a strong
magnetic field using the two-fluid Tolman-Oppenheimer-Volkov equations. We describe …

Wormholes are tunnels connecting different regions in spacetime. They were obtained
originally as a solution for Einstein's General Theory of Relativity and according to this …

In this paper, we proposed a new mathematical model of charged isotropic compact
relativistic object in the f (R, T) gravity. In the f (R, T) framework, the gravitational action …

The primary objective of this paper is to develop a well-behaved class of Heintzmann IIa [H.
Heintzmann, Z. Physik 228, 489-493 (1969)] solution in the context of\(f (R,\, T)\) gravity. In …

In this study, we explore the structural properties of quark stars (QSs) within the Energy-
Momentum Squared Gravity (EMSG) framework, a modified gravity theory characterized by a …