Muir, J;
Baxter, E;
Miranda, V;
Doux, C;
Ferté, A;
Leonard, CD;
Huterer, D;
... Tucker, DL; + view all
(2021)
DES Y1 results: Splitting growth and geometry to test
Λ CDM.
Physical Review D
, 103
(2)
, Article 023528. 10.1103/PhysRevD.103.023528.
Preview |
Text
PhysRevD.103.023528.pdf - Published Version Download (3MB) | Preview |
Abstract
We analyze Dark Energy Survey (DES) data to constrain a cosmological model where a subset of parameters - focusing on ωm - are split into versions associated with structure growth (e.g., ωmgrow) and expansion history (e.g., ωmgeo). Once the parameters have been specified for the ΛCDM cosmological model, which includes general relativity as a theory of gravity, it uniquely predicts the evolution of both geometry (distances) and the growth of structure over cosmic time. Any inconsistency between measurements of geometry and growth could therefore indicate a breakdown of that model. Our growth-geometry split approach therefore serves both as a (largely) model-independent test for beyond-ΛCDM physics, and as a means to characterize how DES observables provide cosmological information. We analyze the same multiprobe DES data as [Phys. Rev. Lett. 122, 171301 (2019)PRLTAO0031-900710.1103/PhysRevLett.122.171301]: DES Year 1 (Y1) galaxy clustering and weak lensing, which are sensitive to both growth and geometry, as well as Y1 BAO and Y3 supernovae, which probe geometry. We additionally include external geometric information from BOSS DR12 BAO and a compressed Planck 2015 likelihood, and external growth information from BOSS DR12 RSD. We find no significant disagreement with ωmgrow=ωmgeo. When DES and external data are analyzed separately, degeneracies with neutrino mass and intrinsic alignments limit our ability to measure ωmgrow, but combining DES with external data allows us to constrain both growth and geometric quantities. We also consider a parametrization where we split both ωm and w, but find that even our most constraining data combination is unable to separately constrain ωmgrow and wgrow. Relative to ΛCDM, splitting growth and geometry weakens bounds on σ8 but does not alter constraints on h.
| Type: | Article |
|---|---|
| Title: | DES Y1 results: Splitting growth and geometry to test Λ CDM |
| Open access status: | An open access version is available from UCL Discovery |
| DOI: | 10.1103/PhysRevD.103.023528 |
| Publisher version: | https://doi.org/10.1103/PhysRevD.103.023528 |
| Language: | English |
| Additional information: | This version is the version of record. For information on re-use, please refer to the publisher’s terms and conditions. |
| Keywords: | Astrophysical studies of gravity, Cosmic microwave background, Cosmological constant, Cosmological parameters, Dark energy, Evolution of the Universe, Large scale structure of the Universe, Sky surveys |
| UCL classification: | UCL UCL > Provost and Vice Provost Offices > UCL BEAMS UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy |
| URI: | https://discovery.ucl.ac.uk/id/eprint/10120735 |
Loading...
Loading...Loading...| 1. |  Russian Federation | 2 |
| 2. |  United States | 1 |
| 3. |  China | 1 |
Archive Staff Only
 |
View Item |
