Abstract The Einstein–Maxwell (or Einstein) system of field equations plays a substantial
role in the modeling of compact stars. Although due to its non-linearity getting an exact …

In this work, we are guided by the gravitational wave events GW 170817 and GW 190814
together with observations of neutron stars PSR J1614-2230, PSR J1903+ 6620, and LMC X …

The current theoretical development identified as the gravitational decoupling via Complete
Geometric Deformation (CGD) method that has been introduced to explore the nonmetricity …

The major goal of this study is to examine the viability and stability of anisotropic compact
stellar objects using the Karmarkar condition in f (𝒬) gravity, where 𝒬 is a scalar of …

The recent theoretical advance known as the minimal geometric deformation (MGD) method
has initiated renewed interest in investigating higher-curvature gravitational effects in …

In this work we explore the characteristics of a polytropic solution for the anisotropic stellar
object within the framework of Einstein–Gauss–Bonnet (EGB) gravity. We introduce …

In this paper we present two new classes of solutions describing compact objects within the
framework of five‐dimensional Einstein‐Gauss‐Bonnet (EGB) gravity. We employ the …

The observations of pulsars heavier than 2 M⊙ have put strong constraints on the equation
of state (EoS) above nuclear saturation density. For this reason, the internal structure of a …

We present a family of new exact solutions for relativistic anisotropic stellar objects by
considering a four-dimensional spacetime embedded in a five-dimensional pseudo …

We present a new class of solutions to the Einstein field equations for an anisotropic matter
distribution in which the interior space-time obeys the Karmarkar condition. The necessary …