Constraining Cosmic Expansion and Gravity with Galaxy Redshift Surveys
arXiv:1212.0009 · doi:10.1088/1475-7516/2013/02/007
Abstract
We analyze the science reach of a next generation galaxy redshift survey such as BigBOSS to fit simultaneously for time varying dark energy equation of state and time- and scale-dependent gravity. The simultaneous fit avoids potential bias from assuming CDM expansion or general relativity and leads to only modest degradation in constraints. Galaxy bias, fit freely in redshift bins, is self calibrated by spectroscopic measurements of redshift space distortions and causes little impact. The combination of galaxy redshift, cosmic microwave background, and supernova distance data can deliver 5-10% constraints on 6 model independent modified gravity quantities.
5 pages, 5 figures
References in corpus (7)
- Distinguishing Modified Gravity from Dark Energy
- Testing cosmological structure formation using redshift-space distortions
- Probing cosmological parameters with the CMB: Forecasts from full Monte Carlo simulations
- Probing modifications of General Relativity using current cosmological observations
- Calibrating Dark Energy
- Confronting General Relativity with Further Cosmological Data
- By Dawn's Early Light: CMB Polarization Impact on Cosmological Constraints