Abstract
In this paper, the model of the holographic Chaplygin gas has been extended to two general cases: first the case of a modified variable Chaplygin gas and second the case of the viscous generalized Chaplygin gas. The dynamics of the model is expressed by the use of scalar fields and scalar potentials.
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Jamil, M., Farooq, M.U. & Rashid, M.A. Generalized holographic dark energy model. Eur. Phys. J. C 61, 471–476 (2009). https://doi.org/10.1140/epjc/s10052-009-1021-3
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DOI: https://doi.org/10.1140/epjc/s10052-009-1021-3