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Pasqua, Antonio; Khodam-Mohammadi, A.; Jamil, Mubasher; Myrzakulov, R.

Interacting Ricci dark energy with logarithmic correction. (English) Zbl 1284.83193

Astrophys. Space Sci. 340, No. 1, 199-208 (2012).
Summary: Motivated by the holographic principle, it has been suggested that the dark energy density may be inversely proportional to the area \(A\) of the event horizon of the universe. However, such a model would have a causality problem. In this work, we consider the entropy-corrected version of the holographic dark energy model in the non-flat FRW universe and we propose to replace the future event horizon area with the inverse of the Ricci scalar curvature. We obtain the equation of state (EoS) parameter \(\omega_\Lambda\), the deceleration parameter \(q\) and \(\Omega_D^\prime\) in the presence of interaction between Dark Energy (DE) and Dark Matter (DM). Moreover, we reconstruct the potential and the dynamics of the tachyon, K-essence, dilaton and quintessence scalar field models according to the evolutionary behavior of the interacting entropy-corrected holographic dark energy model.

Cited in 13 Documents

MSC:

83F05 Relativistic cosmology

Keywords:

dark energy; logarithmic entropy correction; Ricci scalar; scalar field model
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References:

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