The main objective of this paper is to examine the viability and stability of anisotropic
compact stellar objects adopting the Karmarkar condition in energy-momentum squared …

This paper uses the Noether symmetry approach to examine the viable and stable
traversable wormhole solutions in the framework of the f (R, T 2) theory, where R is the Ricci …

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In this work, we present a review of Energy-Momentum Squared Gravity (EMSG)--more
specifically, $ f (R, T_ {\mu\nu} T^{\mu\nu}) $ gravity, where $ R $ represents the Ricci scalar …

In this paper, we study the Tsallis holographic dark energy model to examine the cosmic
evolution in the framework of energy–momentum squared gravity. For this purpose, we use …

In this paper, we study the stability of the Einstein static Universe against anisotropic
homogeneous perturbations in energy–momentum squared gravity. For this purpose, we …

In the present work, we derive the motion of light in the weak-field limit of energy-momentum-
squared gravity (EMSG). To do so, we introduce the post-Newtonian expansion of this …

We construct a generalization of the standard Λ CDM model, wherein we simultaneously
replace the spatially flat Robertson-Walker metric with its simplest anisotropic generalization …

This paper studies a few characteristics of the dynamical charged relativistic system by
invoking the effects arising from the quasi-homologous evolution plus the zero complexity …

The main objective of this article is to examine the stability of Einstein static universe using
inhomogeneous perturbations in the context of energy–momentum squared gravity. For this …