Cosmography can be considered as a sort of a model-independent approach to tackle the
dark energy/modified gravity problem. In this review, the success and the shortcomings of …

In this paper, we use all available baryon acoustic oscillation, Hubble parameter, and
quasar angular size data to constrain six dark energy cosmological models, both spatially …

The cosmological jerk parameter j is reconstructed in a non-parametric way from
observational data independent of a fiducial cosmological model. The Cosmic Chronometer …

This research paper deals with a transit dark energy cosmological model in f (R, L m)-gravity
with observational constraints. For this, we consider a flat Friedman–Lamatre–Robertson …

In this paper, we have investigated an anisotropic cosmological model in f (Q) gravity with
string fluid in LRS Bianchi type-I universe. We have considered the arbitrary function f (Q) …

We investigate the flat-FRW model in the dynamical Chern–Simons gravity with interacting
dark energy. We use dynamical system analysis to illustrate the outcomes of the model. The …

In the current study, we have investigated a modified f (Q)-gravity theory in an anisotropic,
locally rotationally symmetric (LRS) Bianchi type-I spacetime universe model. The arbitrary …

In this work we utilize the most recent publicly available type Ia supernova (SN Ia)
compilations and implement a well-formulated cosmological model based on Lemaître …

In this paper, we apply various diagnostic tools to the phantom dark energy (DE) models,
including the big rip (BR), the little sibling of the big rip (LSBR), and the little rip (LR). The …

In this paper, we have examined the Sharma–Mittal holographic dark energy model
(SMHDE) in the framework of an isotropic and spatially homogeneous flat Friedmann …