FORECASTS OF DARK ENERGY CONSTRAINTS FROM BARYON ACOUSTIC OSCILLATIONS
From MaRDI portal
Publication:3086193
DOI10.1142/S0217732310034316zbMath1208.83135arXiv0904.2218OpenAlexW2952842088MaRDI QIDQ3086193
Publication date: 30 March 2011
Published in: Modern Physics Letters A (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/0904.2218
Cites Work
- Cardassian expansion: a model in which the universe is flat, matter dominated, and accelerating
- Cosmological constant -- the weight of the vacuum
- The cosmological constant and dark energy
- DYNAMICS OF DARK ENERGY
- RECONSTRUCTING DARK ENERGY
- Dark energy, gravitation and supernovae
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- Cosmological Imprint of an Energy Component with General Equation of State
- Model-independent determination of the cosmic expansion rate
- 4D gravity on a brane in 5D Minkowski space
- Cosmology on a brane in Minkowski bulk
This page was built for publication: FORECASTS OF DARK ENERGY CONSTRAINTS FROM BARYON ACOUSTIC OSCILLATIONS