2015
DOI: 10.1007/s10509-015-2477-2
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Reconstruction of generalized ghost pilgrim dark energy in F ( R ˜ ) $F(\tilde{R})$ gravity

Abstract: In this paper, we study the reconstruction scenario of a dark energy model in the framework of modified Horava-Lifshitz F (R) gravity or F (R) gravity. We assume generalized ghost pilgrim dark energy model in flat universe. We consider three well-known scale factors to analyze the behavior of reconstructed F (R) model. These scale factors include bouncing and intermediate scale factors as well as scale factor representing the unification of matter and accelerated phases. The graphical representation is adopted… Show more

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Cited by 15 publications
(6 citation statements)
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“…Our results are consistent with them for non-interacting case with μ = 1.55 and ν = 1.91. Jawad and Rani [18] investigated the reconstructed models, their stability and EoS parameter in the modified Horava-Lifshitz f (R) gravity. Our results are in great agreement with their work.…”
Section: Discussionmentioning
confidence: 99%
See 1 more Smart Citation
“…Our results are consistent with them for non-interacting case with μ = 1.55 and ν = 1.91. Jawad and Rani [18] investigated the reconstructed models, their stability and EoS parameter in the modified Horava-Lifshitz f (R) gravity. Our results are in great agreement with their work.…”
Section: Discussionmentioning
confidence: 99%
“…According to this technique, one has to equate energy densities of corresponding DE model and modified theory to derive a reconstructed model. Jawad and Rani [18] discussed GGPDE model by applying this technique in Horava-Lifshitz f (R) gravity. Sharif and Nazir [19] worked on this technique by assuming GGPDE f (T ) model and investigated the behavior of different cosmological parameters.…”
Section: Introductionmentioning
confidence: 99%
“…Our results are consistent with them for non-interacting case with µ = 1.55 and ν = 1.91. Jawad and Rani [18] investigated the reconstructed models, their stability and EoS parameter in the modified Horava-Lifshitz f ( R) gravity. Our results are in great agreement with their work.…”
Section: Discussionmentioning
confidence: 99%
“…Jawad and Rani [26] considered Horava-Lifshitz f (R) to reconstructed the GGPDE model and the same authors reconstructed PDE model in the background of f (G) gravity, respectively. They conclude that the recontracted dynamical model points out towards different DE scenarios.…”
Section: Introductionmentioning
confidence: 99%