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Interacting holographic viscous dark energy model. (English) Zbl 1186.83123

Summary: We present a generalization of the interacting holographic dark energy model using the viscous generalized Chaplygin gas. We also study the model by considering a dynamical Newton’s constant \(G\). Then we reconstruct the potential and the dynamics of the scalar field which describe the viscous Chaplygin cosmology.

MSC:

83D05 Relativistic gravitational theories other than Einstein’s, including asymmetric field theories
83F05 Relativistic cosmology

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