INTERACTING NON-MINIMALLY COUPLED CANONICAL, PHANTOM AND QUINTOM MODELS OF HOLOGRAPHIC DARK ENERGY IN NON-FLAT UNIVERSE

DOI10.1142/S0218271810018141zbMath1204.83115arXiv0906.1936OpenAlexW2023302485MaRDI QIDQ3067231

Alberto Rozas Fernández, Mohammad R. Setare

Publication date: 20 January 2011

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/0906.1936

zbMATH Keywords

phantomnon-flat universequintom modelnon-minimally coupledinteracting holographic dark energy

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)

Cites Work

• Cardy-Verlinde formula and holographic dark energy
• Generalized second law of thermodynamics in quintom dominated universe
• Bulk-brane interaction and holographic dark energy
• The holographic dark energy in non-flat Brans-Dicke cosmology
• Holographic Chaplygin gas model
• Thermodynamical description of the interaction between holographic dark energy and dark matter
• Le Châtelier-Braun principle in cosmological physics
• Quantum de Sitter cosmology and phantom matter
• Unifying phantom inflation with late-time acceleration: scalar phantom-non-phantom transition model and generalized holographic dark energy
• Holography Stabilizes the Vacuum Energy
• A TRACKER SOLUTION FOR A HOLOGRAPHIC DARK ENERGY MODEL
• INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
• PARAMETRIZATIONS OF THE DARK ENERGY DENSITY AND SCALAR POTENTIALS
• DARK ENERGY: A UNIFYING VIEW
• Effective Field Theory, Black Holes, and the Cosmological Constant
• Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
• Probable Values of the Cosmological Constant in a Holographic Theory
• Interacting quintessence

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