First-order formalism for the quintom model of dark energy
From MaRDI portal
Publication:1008275
DOI10.1007/s10773-008-9757-3zbMath1161.83471arXiv0805.1117OpenAlexW2052828507MaRDI QIDQ1008275
Jafar Sadeghi, Mohammad R. Setare
Publication date: 24 March 2009
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/0805.1117
Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)
Related Items (2)
Multi-fluid cosmology in Einstein gravity: analytical solutions ⋮ Correspondence between Ricci and other dark energies
Cites Work
- Holographic tachyon model of dark energy
- Cardy-Verlinde formula and holographic dark energy
- First-order formalism and dark energy
- First-order formalism for bent brane
- Generalized second law of thermodynamics in quintom dominated universe
- Interacting holographic dark energy model in non-flat universe
- The holographic dark energy in non-flat Brans-Dicke cosmology
- Holographic Chaplygin gas model
- Shape invariance for the bent brane with two scalar fields
- de Sitter brane universe induced by phantom and quantum effects
- Quantum de Sitter cosmology and phantom matter
- Cosmological constant -- the weight of the vacuum
- Solitons in systems of coupled scalar fields
- The cosmological constant and dark energy
- Coupled quintessence and phantom based on a dilaton
- A TRACKER SOLUTION FOR A HOLOGRAPHIC DARK ENERGY MODEL
- 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
- Phantom cosmology with general potentials
- An alternative to quintessence
This page was built for publication: First-order formalism for the quintom model of dark energy