Supernova limits on brane world cosmology
arXiv:astro-ph/0511029 · doi:10.1016/j.physletb.2006.07.048
Abstract
By combining the first year data from the Supernova Legacy Survey (SN LS) and the recent detection of the baryon acoustic peak in the Sloan Digital Sky Survey data, we are able to place strong constraints on models where the cosmic acceleration is due to the leakage of gravity from the brane into the bulk on large scales. In particular, we are able to show that the DGP model is not compatible with a spatially flat universe. We generalize our analysis to phenomenological toy models where the curvature of the brane enters into the Friedmann equations in different ways.
comments added on baryon oscillations/typos fixed 8 pages, 3 figs
References in corpus (15)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- An Alternative to Compactification
- The Hierarchy Problem and New Dimensions at a Millimeter
- Type Ia Supernova Discoveries at z>1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
- 4D Gravity on a Brane in 5D Minkowski Space
- The Supernova Legacy Survey: Measurement of Omega_M, Omega_Lambda and w from the First Year Data Set
- New Constraints on , , and w from an Independent Set of Eleven High-Redshift Supernovae Observed with HST
- Non-conventional cosmology from a brane-universe
- Accelerated Universe from Gravity Leaking to Extra Dimensions
- Cosmology on a Brane in Minkowski Bulk
- Structure formation in the DGP cosmological model
- Supernovae, CMB, and Gravitational Leakage into Extra Dimensions
- Cosmological Challenges in Theories with Extra Dimensions and Remarks on the Horizon Problem
- SNOC: a Monte-Carlo simulation package for high-z supernova observations
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