arXiv:1810.02499·v2·Cosmology and Nongalactic Astrophysics
Dark Energy Survey Year 1 Results: Constraints on Extended Cosmological Models from Galaxy Clustering and Weak Lensing
DES Collaboration: T. M. C. Abbott🇨🇱 · F. B. Abdalla🇬🇧 · S. Avila🇬🇧 · M. Banerji🇬🇧 · E. Baxter🇺🇸 · K. Bechtol🇺🇸 · M. R. Becker🇺🇸 · E. Bertin🇫🇷 · J. Blazek🇺🇸 · S. L. Bridle🇬🇧 · D. Brooks🇬🇧 · D. Brout🇺🇸
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.
Comments: 22 pages, 7 figures, matches the published version