Density perturbation in the models reconstructed from jerk parameter
arXiv:1805.02824 · doi:10.1007/s10714-018-2383-3
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.
arXiv comment14 pages; 3 figures; minor typos corrected; Accepted for publication in GRG journal
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