Interacting dark energy in Hořava-Lifshitz cosmology
From MaRDI portal
Publication:422284
DOI10.1007/s10509-011-0955-8zbMath1238.83089arXiv0909.0456OpenAlexW1537078899MaRDI QIDQ422284
S. K. Moayedi, Davood Momeni, Mohammad R. Setare
Publication date: 16 May 2012
Published in: Astrophysics and Space Science (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/0909.0456
Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
Related Items (4)
On Hořava-Lifshitz ``black holes ⋮ Horava-Lifshitz cosmology and quark-hadron phase transition ⋮ Cosmological evolution of pilgrim dark energy in \(f(G)\) gravity ⋮ Minimal-supersymmetric extended inflation field in Horava–Lifshitz gravity
Cites Work
- Holographic tachyon model of dark energy
- Hořava-Lifshitz cosmology
- Generalized second law of thermodynamics in quintom dominated universe
- de Sitter brane universe induced by phantom and quantum effects
- Quantum de Sitter cosmology and phantom matter
- Cosmological constant -- the weight of the vacuum
- Extended theories of gravity and their cosmological and astrophysical applications
- Unifying phantom inflation with late-time acceleration: scalar phantom-non-phantom transition model and generalized holographic dark energy
- The cosmological constant and dark energy
- Modified F ( R ) Hořava–Lifshitz gravity: a way to accelerating FRW cosmology
- INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
- QUINTOM COSMOLOGY WITH GENERAL POTENTIALS
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- Cosmological Imprint of an Energy Component with General Equation of State
- The cosmological constant problem
This page was built for publication: Interacting dark energy in Hořava-Lifshitz cosmology