Interacting holographic generalized Chaplygin gas model
M. R. Setare
TL;DR
This paper explores a model linking holographic dark energy with an interacting generalized Chaplygin gas in a Friedmann-Robertson-Walker universe, reconstructing the scalar field potential to describe this cosmology.
Contribution
It introduces a novel correspondence between holographic dark energy and interacting generalized Chaplygin gas, including scalar field potential reconstruction.
Findings
Established a correspondence between holographic dark energy and Chaplygin gas.
Reconstructed the scalar field potential for the generalized Chaplygin cosmology.
Provided insights into the dynamics of interacting dark energy models.
Abstract
In this paper we consider a correspondence between the holographic dark energy density and interacting generalized Chaplygin gas energy density in FRW universe. Then we reconstruct the potential of the scalar field which describe the generalized Chaplygin cosmology.
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