The paper presents late time cosmology in f (Q, T) gravity where the dark energy is purely
geometric in nature. We start by employing a well motivated f (Q, T) gravity model, f (Q, T)= m …

The article presents modeling of inflationary scenarios for the first time in the f (R, T) theory of
gravity. We assume the f (R, T) functional form to be R+ η T R+ η T, where R denotes the …

We present a new class of nonsingular bounce cosmology free from instabilities, using a
single scalar field coupled to gravity within the framework of the Degenerate Higher-Order …

In this paper, we highlight the variables preserving stability of a very restricted class of
anisotropic axial symmetrical compact geometry in the scenario of f (R, T) gravity, where T …

In this paper, we study a theory of gravity called mimetic f (R, T) in the presence of
swampland dS conjecture. For this purpose, we introduce several inflation solutions of the …

Modelling of matter bounce in f (R, T) gravity has been presented with no violation of the null
energy condition. Only a closed universe with negative pressure is allowed in good …

The occurrences of singularities where spacetime curvature becomes infinite and geodesic
evolution breaks down are inevitable events in classical general relativity (GR) unless one …

This research paper is an investigation of dark energy nature of logarithmic f (R, T)-gravity
cosmology in a flat FLRW space–time universe. We have derived modified Einstein's field …

In today's scenario, going beyond Einstein's theory of gravity leads us to some more
complete and modified gravity theories. One of them is the f (R, T) gravity in which R is the …

In this paper, we study the bouncing behavior of our universe under f (G, T) theory, by taking
Friedmann–Lemaître–Robertson–Walker metric, which is assumed to be coupled with an …