DARK ENERGY AND THE FUTURE FATE OF THE UNIVERSE
From MaRDI portal
Publication:3507598
DOI10.1142/S021773230702292XzbMath1143.83323arXivgr-qc/0508053OpenAlexW3105264902MaRDI QIDQ3507598
Publication date: 20 June 2008
Published in: Modern Physics Letters A (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/gr-qc/0508053
Relativistic cosmology (83F05) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)
Cites Work
- Unifying phantom inflation with late-time acceleration: scalar phantom-non-phantom transition model and generalized holographic dark energy
- Observation of Cosmic Acceleration and Determining the Fate of the Universe
- Effective Field Theory, Black Holes, and the Cosmological Constant
- Cosmological parameters from supernova observations: A critical comparison of three data sets
- OBSERVATIONAL CONSTRAINTS ON DARK ENERGY MODEL
- Bayesian analysis of the (generalized) Chaplygin gas and cosmological constant models using the 157 gold SNe Ia data
- Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
- Model-independent analysis of dark energy: supernova fitting result
- Holography and holographic dark energy model
- Can we predict the fate of the Universe?
- An alternative to quintessence
This page was built for publication: DARK ENERGY AND THE FUTURE FATE OF THE UNIVERSE
