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The Cosmological Dynamics of Interacting Holographic Dark Energy Model

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arxiv 0704.2070 v2 pith:RCTPD6YE submitted 2007-04-16 hep-th astro-phgr-qc

M. R. Setare , Elias C. Vagenas This is my paper · ORCID
classification hep-thastro-phgr-qc
keywords cosmologicaldarkenergyevolutionholographicinteractingmodelmodels
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Motivated by the recent observations for the cosmic acceleration and the suitable evolution of the Universe provided an interaction (decay of dark energy to matter) is incorporated in a cosmological model, we study the cosmological evolution of the Interacting Holographic Dark Energy scenario. Critical points are derived and their corresponding cosmological models are presented. The dynamical character of these models is revealed.

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Cited by 1 Pith paper

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  1. Constraints on Barrow and Tsallis Holographic Dark Energy from DESI DR2 BAO data

    gr-qc 2025-06 conditional novelty 5.0 of 10

    Barrow and Tsallis holographic dark energy models fit DESI DR2 data but are disfavored by information criteria versus LambdaCDM and do not ease the Hubble tension.

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