G-corrected holographic dark energy model

M. Malekjani; M. Honari-Jafarpour

doi:10.1007/s10509-013-1475-5

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arXiv · 1302.3445

G-corrected holographic dark energy model

M. Malekjani·M. Honari-Jafarpour

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Abstract

Here we investigate the holographic dark energy model in the framework of FRW cosmology where the Newtonian gravitational constant,$G$, is varying with cosmic time. Using the complementary astronomical data which support the time dependency of $G$, the evolutionary treatment of EoS parameter and energy density of dark energy model are calculated in the presence of time variation of $G$. It has been shown that in this case, the phantom regime can be achieved at the present time. We also calculate the evolution of $G$- corrected deceleration parameter for holographic dark energy model and show that the dependency of $G$ on the comic time can influence on the transition epoch from decelerated expansion to the accelerated phase. Finally we perform the statefinder analysis for $G$- corrected holographic model and show that this model has a shorter distance from the observational point in $s-r$ plane compare with original holographic dark energy model.

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M. Malekjani, M. Honari-Jafarpour. 2013-05-01. G-corrected holographic dark energy model. https://doi.org/10.1007/s10509-013-1475-5

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