2008/10/31 by M. R. Setare, Emmanuel N. Saridakis, E. N. Saridakis · 7 citations
Physics and Astronomy · #Advanced Differential Geometry Research #Astrophysics #Black Holes and Theoretical Physics #Classical mechanics #Cosmology #Cosmology and Gravitation Theories #Dark energy #Equation of state #Holography #Imaging phantom #Optics #Physics #Quantum mechanics #Theoretical physics #astro-ph #hep-th
paper · pdf · doi:10.1016/j.physletb.2008.12.026
9 pages, 5 figures, version published in Phys. Lett. B
arxiv created 2008/12/11 · openalex publication_date 2008/12/17 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
We investigate canonical, phantom and quintom models, with the various fields being non-minimally coupled to gravity, in the framework of holographic dark energy. We classify them and we discuss their cosmological implications. In particular, we examine the present value of the dark energy equation-of-state parameter and the crossing through the phantom divide, and we extract the conditions for a future cosmological singularity. The combined scenarios are in agreement with observations and reveal interesting cosmological behaviors.