Anisotropic cosmology with a dilaton field coupled to ghost dark energy

DOI10.1134/S0040577918030091zbMath1400.83063WikidataQ129971026 ScholiaQ129971026MaRDI QIDQ1792398

Yanyan Li

Publication date: 11 October 2018

Published in: Theoretical and Mathematical Physics (Search for Journal in Brave)

zbMATH Keywords

perturbation theorygeneralized second law of thermodynamicsanisotropic universegeneralized ghost dark energyghost dark energydilaton scalar field

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Classical and relativistic thermodynamics (80A10) Astrophysical cosmology (85A40)

Cites Work

• Interacting generalized ghost dark energy in non-isotropic background
• A dark energy model characterized by the age of the Universe
• Instability of interacting ghost dark energy model in an anisotropic universe
• \(f(R)\) theories
• The generalized second law for the interacting new agegraphic dark energy in a non-flat FRW universe enclosed by the dynamical apparent horizon
• A new class of LRS Bianchi type-I cosmological models in Lyra geometry
• The QCD nature of dark energy
• Interacting ghost dark energy in non-flat universe
• Instability of holographic dark energy models
• Validity of the generalized second law of thermodynamics of the universe bounded by the event horizon in holographic dark energy model
• de Sitter brane universe induced by phantom and quantum effects
• Quantum de Sitter cosmology and phantom matter
• Stable exact solutions in cosmological models with two scalar fields
• Dark Energy
• The cosmological constant and dark energy
• Unified dark energy thermodynamics: varying w and the −1-crossing
• Thermodynamics of interacting holographic dark energy with the apparent horizon as an IR cutoff
• DYNAMICS OF DARK ENERGY
• THE COSMOLOGICAL DYNAMICS OF INTERACTING HOLOGRAPHIC DARK ENERGY MODEL
• INSTABILITY OF QCD GHOST DARK ENERGY MODEL
• FIELD THEORY OF TACHYON MATTER
• Braneworld cosmological solutions and their stability
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• Black Holes and Entropy
• Entropy-Corrected Holographic Dark Energy
• 4D gravity on a brane in 5D Minkowski space
• \(k\)-inflation

This page was built for publication: Anisotropic cosmology with a dilaton field coupled to ghost dark energy