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 …

In this work, we have adopted gravitational decoupling by minimal geometric deformation
(MGD) approach and have developed an anisotropic version of well-known Tolman VII …

In this work, we study a cosmological model of Bianchi type-I Universe in teleparallel gravity
for a perfect fluid. To obtain the cosmological solution of the model, we assume that the …

Motivated by anomalies in cosmic microwave background observations, we investigate the
implications of f (Q, T) gravity in Bianchi type-I spacetime, aiming to characterize the …

In this paper, we present a spatially homogeneous and anisotropic Bianchi type-I
cosmological model with a viscous bulk fluid in f (R, T) gravity where R and T are the Ricci …

The phenomenon of accelerated expansion of the present universe and a cosmic transit
aspect is explored in the framework of a modified gravity theory known as f (R, T) gravity …

In this paper, we have proposed a new form for the varying deceleration parameter that is a
generalization of the form of Ö. Akarsu and T. Dereli [Cosmological models with linearly …

In this work, we have studied the spatially homogeneous anisotropic Bianchi type-I Universe
in f (R, T) gravity (where R is the Ricci scalar and T is the trace of the energy-impulsion …

In this research, we examine a spatially homogeneous anisotropic locally rotationally
symmetric (LRS) Bianchi type-I cosmological model in f (R, T) gravity, for some choices of …

Abstract A flat FLRW (Friedmann–Lemaitre–Robertson–Walker) cosmological model with
perfect fluid comprising of variable Chaplygin gas (VCG) has been studied in the context of f …