Density perturbation in the models reconstructed from jerk parameter
General Relativity and Quantum Cosmology
2021-03-17 v2 Cosmology and Nongalactic Astrophysics
Abstract
The present work deals with the late time evolution of the linear density contrast in the dark energy models reconstructed from the jerk parameter. It is found that the non-interacting models are favoured compared to the models where an interaction is allowed in the dark sector.
Keywords
Cite
@article{arxiv.1805.02824,
title = {Density perturbation in the models reconstructed from jerk parameter},
author = {Srijita Sinha and Narayan Banerjee},
journal= {arXiv preprint arXiv:1805.02824},
year = {2021}
}
Comments
14 pages; 3 figures; minor typos corrected; Accepted for publication in GRG journal