Cosmological Constraints from Type Ia Supernovae Peculiar Velocity Measurements
arXiv:0705.1718 · doi:10.1103/PhysRevLett.99.081301
Abstract
We detect the correlated peculiar velocities of nearby type Ia supernovae (SNe), while highlighting an error in some of the literature. We find sigma_8=0.79 +/- 0.22 from SNe, and examine the potential of this method to constrain cosmological parameters in the future. We demonstrate that a survey of 300 low-z SNe (such as the nearby SNfactory) will underestimate the errors on w by about 35% if the coherent peculiar velocities are not included.
5 pages, 4 figures. V2: references added. V3: clarifying comments added in response to referee reports. V4: typo in eq. 6 corrected. V5: error in Fig. 1 corrected
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