\(Om\) diagnostic for two-parameter \(\omega _{\sigma }\) in dilaton dark energy
From MaRDI portal
Publication:763250
DOI10.1007/s10773-011-0765-3zbMath1235.85013OpenAlexW2023301404MaRDI QIDQ763250
Publication date: 9 March 2012
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10773-011-0765-3
Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Astrophysical cosmology (85A40)
Cites Work
- Cardy-Verlinde formula and holographic dark energy
- Prospects and problems of tachyon matter cosmology
- Inflation from a tachyon fluid?
- \(Om\) diagnostic for dilaton dark energy
- Coupled quintessence and phantom based on a dilaton
- DYNAMICS AND HOLOGRAPHIC DISCRETENESS OF TACHYONIC INFLATION
- PHANTOM COSMOLOGY WITH A NONLINEAR BORN–INFELD TYPE SCALAR FIELD
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
- Hessence: a new view of quintom dark energy
- STATEFINDER DIAGNOSTIC FOR HOLOGRAPHIC DARK ENERGY MODEL
- \(k\)-inflation
This page was built for publication: \(Om\) diagnostic for two-parameter \(\omega _{\sigma }\) in dilaton dark energy
