Possible Equilibria of Interacting Dark Energy Models

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dc.creatorBerger, Micheal S.
dc.creatorShojaei, Hamed
dc.date2007-12-14
dc.date2008-06-06
dc.date.accessioned2026-07-07T11:39:26Z
dc.date.available2026-07-07T11:39:26Z
dc.descriptionInteracting dark energy and the holographic principle offer a possible way of addressing the cosmic coincidence problem as well as accounting for the size of the dark energy component. The equilibrium points of the Friedmann equations which govern the evolution behavior of dark energy, matter, and curvature components can determine the qualitative behavior of the cosmological models. These possible equilibria and their behavior are examined in a general framework, and some illustrative examples are presented.
dc.description18 pages, 5 figures
dc.identifierhttps://arxiv.org/abs/0712.2450
dc.identifierhttp://arxiv.org/abs/0712.2450
dc.identifierPhys.Rev.D77:123504,2008
dc.identifierdoi:10.1103/PhysRevD.77.123504
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/199916
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.titlePossible Equilibria of Interacting Dark Energy Models
dc.typetext

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