http://arxiv.org/abs/1805.02824
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.
N. Banerjee and S. Sinha
Wed, 9 May 18
39/55
Comments: 14 pages; 3 figures. Accepted for publication in GRG journal
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