activity
20202022
most citedEvaluation of cosmological models in gravity in different dark energy scenario

29 citations · 45 across the 2 of their papers we have counts for

collaborators

7 papers

gr-qc202216 cited

A new class of holographic dark energy models in LRS Bianchi Type-I

Anirudh Pradhan, Vinod Kumar Bhardwaj, Archana Dixit +1

In this paper, we examine the (LRS) Bianchi-type-I cosmological model with holographic dark energy. The exact solutions to the corresponding field equations are obtained by using g…

gr-qc202129 cited

Evaluation of cosmological models in gravity in different dark energy scenario

Vinod Kumar Bhardwaj, Anirudh Pradhan

In present paper, we search the existence of dark energy scalar field models within in gravity theory established by Harko et al. (Phys. Rev. D 84, 024020, 2011) in a fla…

gr-qc2021

Barrow HDE model for Statefinder diagnostic in non-flat FRW universe

Archana Dixit, Vinod Kumar Bharadwaj, Anirudh Pradhan

In this work we study a non-flat Friedmann-Robertson-Walker universe filled with a pressure-less dark matter (DM) and Barrow holographic dark energy (BHDE) whose IR cutoff is the a…

gr-qc2021

Statefinder hierarchy model for the Barrow holographic dark energy

Vinod Kumar Bhardwaj, Archana Dixit, Anirudh Pradhan

In this paper, we have used the state finder hierarchy for Barrow holographic dark energy (BHDE) model in the system of the FLRW Universe. We apply two DE diagnostic tools to deter…

gr-qc2021

Barrow HDE model for Statefinder diagnostic in FLRW Universe

Anirudh Pradhan, Archana Dixit, Vinod Kumar Bhardwaj

We have analyzed the Barrow holographic dark energy (BHDE) in the framework of the flat FLRW Universe by considering the various estimations of Barrow exponent . Here we…

gr-qc2020

Compatibility between the scalar field models of tachyon, -essence and quintessence in gravity

Vinod Kumar Bhardwaj, Anirudh Pradhan, Archana Dixit

We investigate the behavior of the scalar field in gravity (Harko et al., Phys. Rev. D 84, 024020, 2011) inside the structure of a flat FRW cosmological model, where $R…