The paper is devoted to study the observational signatures of f (R, G, T) gravity in FRW
universe. In this research article, we present a new cosmological model formulated within …

Within this work, we propose a new generalised quintom dark energy model in the
teleparallel alternative of general relativity theory, by considering a non-minimal coupling …

In this paper, we first obtain the energy density by the approach of the new agegraphic dark
energy model, and then the f (T, B) gravity model is studied as an alternative to the dark …

In this paper, we analyze the modified\(f ({\mathcal {R}})\) gravity models in Friedmann–
Lemaître–Robertson–Walker (FLRW) background. The actions of bouncing cosmology are …

In this paper, we have studied the anisotropic and homogeneous Bianchi type-V universe
filled with two minimally interacting fields, matter and holographic dark energy components …

In this paper, we study F (R) gravity by Hu–Sawicki model in Friedmann–Lemaître–
Robertson–Walker (FLRW) background. The Friedmann equations are calculated by …

For many quantum field theory computations in cosmology it is not possible to use the flat
space trick of obtaining full, interacting states by evolving free states over infinite times. State …

In this paper, we study the model of f (T, B) f(T,B) gravity with viscous fluid in flat-FRW metric,
in which TT and BB are torsion scalar and boundary term, respectively. We obtain the …

In this paper, we study the viscous f (T, B) gravity model as a source of dark energy, and the
Extended Bose–Einstein Condensate (EBEC) as a source of dark matter, in a flat-FRW …

Motivated by the recent works of Golovnev et al.(2008), Chiba (2008)[1, 2] where a model of
inflation has been suggested with non-minimally coupled massive vector fields, we …