Stability of dark energy models on the brane universes
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Publication:379239
DOI10.1007/s10773-013-1560-0zbMath1274.83175OpenAlexW1987546806MaRDI QIDQ379239
Publication date: 11 November 2013
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10773-013-1560-0
Relativistic cosmology (83F05) String and superstring theories; other extended objects (e.g., branes) in quantum field theory (81T30)
Cites Work
- Unnamed Item
- Holographic Ricci dark energy model
- Hubble expansion parameter in a new model of dark energy
- Holographic dark energy model with interaction and cosmological constant in the flat space-time
- Time-dependent dark energy density and holographic DE model with interaction
- Holographic dark energy density
- The ds/CFT correspondence and the big smash
- Holographic Chaplygin gas model
- Holographic dark energy density and JBP parametrization
- Quantum de Sitter cosmology and phantom matter
- Bouncing braneworlds
- Viscous generalized Chaplygin gas with arbitrary \(\alpha\)
- Viscous Chaplygin gas in non-flat universe
- Holography Stabilizes the Vacuum Energy
- A TRACKER SOLUTION FOR A HOLOGRAPHIC DARK ENERGY MODEL
- Large Mass Hierarchy from a Small Extra Dimension
- SUPERQUINTESSENCE
- SELF-INTERACTING HOLOGRAPHIC DARK ENERGY
- 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
- An alternative to quintessence