activity
20042023
most citedBianchi Type III Anisotropic Dark Energy Models with Constant Deceleration Parameter

105 citations · 197 across the 10 of their papers we have counts for

collaborators
Showing gr-qcShow all

6 papers · 1 filter

gr-qc2011★ 27 cited

Cylindrically Symmetric Inhomogeneous Universes with a Cloud of Strings

Anil Kumar Yadav, Vineet Kumar Yadav, Lallan Yadav

Cylindrically symmetric inhomogeneous string cosmological models are investigated in presence of string fluid as a source of matter. To get the three types of exact solutions of Ei…

gr-qc2010★ 105 cited

Bianchi Type III Anisotropic Dark Energy Models with Constant Deceleration Parameter

Anil Kumar Yadav, Lallan Yadav

The Bianchi type III dark energy models with constant deceleration parameter are investigated. The equation of state parameter is found to be time dependent and its existing ra…

gr-qc2009★ 15 cited

Bianchi Type V String Cosmological Models in General Relativity

Anil Kumar Yadav, Vineet Kumar Yadav, Lallan Yadav

Bianchi type V string cosmological models in general relativity are investigated. To get the exact solution of Einstein's field equations, we have taken some scale transformations…

gr-qc2007

String Cosmological Model in Cylindrically Symmetric Inhomogeneous Universe with Electromagnetic Field II

Anirudh Pradhan, S. K. Singh, L. J. S. Yadav

Cylindrically symmetric inhomogeneous string cosmological model of the universe in presence of electromagnetic field is investigated. We have assumed that F_{12} is the only non-va…

gr-qc2007

String Cosmological Model in Cylindrically Symmetric Inhomogeneous Universe with Electromagnetic Field

Anirudh Pradhan, Anju Rai, Raj Bali

Cylindrically symmetric inhomogeneous string cosmological models in presence of electromagnetic field is investigated. We have assumed that is the only non-vanishing compo…

gr-qc2004★ 22 cited

Generation of Bianchi type V cosmological models with varying -term

Anirudh Pradhan, A. K. Yadav, L. Yadav

Bianchi type V perfect fluid cosmological models are investigated with cosmological term varying with time. Using a generation technique (Camci {\it et al.}, 2001), it is shown…