Isotropization of locally rotationally symmetric Bianchi-I universe in f(Q)-gravity
Despite having the somewhat successful description of accelerated cosmology, the early
evolution of the universe always challenges mankind. Our promising approach lies in a new …
evolution of the universe always challenges mankind. Our promising approach lies in a new …
Modeling wormholes in gravity
In this work, we propose the modeling of static wormholes within the f (R, T) extended theory
of gravity perspective. We present some models of wormholes, which are constructed from …
of gravity perspective. We present some models of wormholes, which are constructed from …
Study of anisotropic strange stars in gravity: An embedding approach under the simplest linear functional of the matter-geometry coupling
The present work is focused on the investigation of the existence of compact structures
describing anisotropic matter distributions within the framework of modified gravity theories …
describing anisotropic matter distributions within the framework of modified gravity theories …
Krori–Barua Bardeen compact stars in f (R, T) gravity
The current study emphasizes the impact of electric charge for static spherically symmetric
stellar structures using isotropic distribution in f (R, T) theory of gravity. For this purpose, we …
stellar structures using isotropic distribution in f (R, T) theory of gravity. For this purpose, we …
The simplest non-minimal matter–geometry coupling in the f(R, T) cosmology
Abstract f (R, T) gravity is an extended theory of gravity in which the gravitational action
contains general terms of both the Ricci scalar R and the trace of the energy-momentum …
contains general terms of both the Ricci scalar R and the trace of the energy-momentum …
Late-time acceleration in f (Q) gravity: Analysis and constraints in an anisotropic background
This paper is devoted to investigate the anisotropic locally rotationally symmetric (LRS)
Bianchi type-I space–time in the context of the recently proposed f (Q) gravity in which Q is …
Bianchi type-I space–time in the context of the recently proposed f (Q) gravity in which Q is …
Stellar equilibrium configurations of compact stars in f (R, T) theory of gravity
In this article we study the hydrostatic equilibrium configuration of neutron stars and strange
stars, whose fluid pressure is computed from the equations of state p= ωρ 5/3 and p= 0.28 …
stars, whose fluid pressure is computed from the equations of state p= ωρ 5/3 and p= 0.28 …
Gravastars in gravity
We propose a unique stellar model under the f (R, T) gravity by using the conjecture of
Mazur-Mottola [P. Mazur and E. Mottola, Report No. LA-UR-01-5067, P. Mazur and E …
Mazur-Mottola [P. Mazur and E. Mottola, Report No. LA-UR-01-5067, P. Mazur and E …
Observational constraints on the equation of state of viscous fluid in f (R, T) gravity
In this paper, we investigate a cosmological model based on viscous f (R, T) gravity as a
potential alternative to dark energy. This model incorporates bulk viscosity and is analyzed …
potential alternative to dark energy. This model incorporates bulk viscosity and is analyzed …
[HTML][HTML] Static spherically symmetric wormholes in f (R, T) gravity
In this work, we explore wormhole solutions in f (R, T) theory of gravity, where R is the scalar
curvature and T is the trace of stress-energy tensor of matter. To investigate this, we consider …
curvature and T is the trace of stress-energy tensor of matter. To investigate this, we consider …