2006/01/31 by M. S. Berger, Micheal S. Berger, Hamed Shojaei
Mathematics · Physics and Astronomy · #Advanced Differential Geometry Research #Astronomy #Astrophysics #Attractor #Black Holes and Theoretical Physics #COSMIC cancer database #Coincidence #Cosmology #Cosmology and Gravitation Theories #Dark energy #Dark fluid #Mathematics #Physical cosmology #Physics #Theoretical physics #Universe #gr-qc
paper · pdf · doi:10.1103/physrevd.73.083528
published as Phys.Rev. D73 (2006) 083528 · 8 pages, 3 figures, Phys. Rev. D version
openalex publication_date 2006/04/27 · arxiv created 2006/05/02 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
The introduction of an interaction for dark energy to the standard cosmology offers a potential solution to the cosmic coincidence problem. We examine the conditions on the dark energy density that must be satisfied for this scenario to be realized. Under some general conditions we find a stable attractor for the evolution of the Universe in the future. Holographic conjectures for the dark energy offer some specific examples of models with the desired properties.