Interacting holographic generalized Chaplygin gas model

2007/08/20 by M. R. Setare
Mathematics · Physics and Astronomy · #Advanced Differential Geometry Research #Black Holes and Theoretical Physics #Chaplygin gas #Classical mechanics #Cosmology #Cosmology and Gravitation Theories #Dark energy #Friedmann–Lemaître–Robertson–Walker metric #Geometry #Holographic principle #Holography #Mathematical physics #Mathematics #Physics #Quantum mechanics #Scalar (mathematics) #Scalar field #Theoretical physics #hep-th

paper · pdf · doi:10.1016/j.physletb.2007.08.038

published as Phys.Lett.B654:1-6,2007 · 12 pages, no figure

openalex publication_date 2007/08/20 · arxiv created 2007/09/20 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

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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