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Holographic Dark Energy Model with Generalized Chaplygin Gas in Higher Dimensions

V. M. Santhi, V. U. M. Rao, N. Sandhya Rani


In this paper, we have studied a five dimensional FRW space-time filled with two minimally interacting fluids: matter and holographic dark energy in Saez-Ballester (1986) scalar tensor theory of gravitation. We have established a correspondence between the holographic dark energy models with the generalised Chaplygin gas. We also reconstructed the potential and dynamics of the scalar field which describes the Chaplygin cosmology. Also, we have discussed physical and geometrical properties of the model.

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