Dark Energy Survey Year 1 Results: Constraints on Extended Cosmological Models from Galaxy Clustering and Weak Lensing
arXiv:1810.02499 · doi:10.1103/PhysRevD.99.123505
Abstract
We present constraints on extensions of the minimal cosmological models dominated by dark matter and dark energy, CDM and CDM, by using a combined analysis of galaxy clustering and weak gravitational lensing from the first-year data of the Dark Energy Survey (DES Y1) in combination with external data. We consider four extensions of the minimal dark energy-dominated scenarios: 1) nonzero curvature , 2) number of relativistic species different from the standard value of 3.046, 3) time-varying equation-of-state of dark energy described by the parameters and (alternatively quoted by the values at the pivot redshift, , and ), and 4) modified gravity described by the parameters and that modify the metric potentials. We also consider external information from Planck CMB measurements; BAO measurements from SDSS, 6dF, and BOSS; RSD measurements from BOSS; and SNIa information from the Pantheon compilation. Constraints on curvature and the number of relativistic species are dominated by the external data; when these are combined with DES Y1, we find at the 68% confidence level, and at 68% (95%) confidence. For the time-varying equation-of-state, we find the pivot value at pivot redshift from DES alone, and at from DES Y1 combined with external data; in either case we find no evidence for the temporal variation of the equation of state. For modified gravity, we find the present-day value of the relevant parameters to be from DES Y1 alone, and from DES Y1 combined with external data, consistent with predictions from GR.
arXiv comment22 pages, 7 figures, matches the published version
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