Possible Equilibria of Interacting Dark Energy Models

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Interacting 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.
18 pages, 5 figures

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General Relativity and Quantum Cosmology, High Energy Physics - Phenomenology

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http://salesiana.dossiersoluciones.com/handle/123456789/199916

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/0712.2450
 http://arxiv.org/abs/0712.2450
 Phys.Rev.D77:123504,2008
 doi:10.1103/PhysRevD.77.123504

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arXiv