Holographic Dark Energy Scenario and Variable Modified Chaplygin Gas
Surajit Chattopadhyay, Ujjal Debnath
TL;DR
This paper explores a cosmological model where holographic dark energy interacts with variable modified Chaplygin gas in an FRW universe, reconstructing the scalar field potential to describe this scenario.
Contribution
It introduces a novel correspondence between holographic dark energy and interacting variable modified Chaplygin gas, including potential reconstruction.
Findings
Established a link between holographic dark energy and Chaplygin gas.
Reconstructed scalar field potential for the cosmological model.
Analyzed the interaction effects in an FRW universe.
Abstract
In this letter, we have considered that the universe is filled with normal matter and variable modified Chaplygin gas. Also we have considered the interaction between normal matter and variable modified Chaplygin gas in FRW universe. Then we have considered a correspondence between the holographic dark energy density and interacting variable modified Chaplygin gas energy density. Then we have reconstructed the potential of the scalar field which describes the variable modified Chaplygin cosmology.
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