Implications of a transition in the dark energy equation of state for the H0 and σ8 tensions

Journal article

We explore the implications of a rapid appearance of dark energy between the redshifts (z) of one and two on the expansion rate and growth of perturbations. Using both Gaussian process regression and a parametric model, we show that this is the preferred solution to the current set of low-redshift (z<3) distance measurements if H0=73 km s−1 Mpc−1 to within 1% and the high-redshift expansion history is unchanged from the ΛCDM inference by the Planck satellite. Dark energy was effectively non-existent around z=2, but its density is close to the ΛCDM model value today, with an equation of state greater than −1 at z<0.5. If sources of clustering other than matter are negligible, we show that this expansion history leads to slower growth of perturbations at z<1, compared to ΛCDM, that is measurable by upcoming surveys and can alleviate the σ8 tension between the Planck CMB temperature and low-redshift probes of the large-scale structure.

Authors: Keeley, RE; Joudaki, S; Kaplinghat, M; Kirkby, D

• Publication status: Published
• Peer review status: Peer reviewed
• Publisher: IOP Publishing
• Journal: Journal of Cosmology and Astroparticle Physics
• Volume: 2019
• Issue: 12
• Article number: 35
• Publication date: 2019-12-11
• Acceptance date: 2019-11-25
• DOI: 10.1088/1475-7516/2019/12/035
• EISSN: 1475-7516
• ISSN: 1475-7516
• Language: English
• Keywords: supernova type Ia; baryon acoustic oscillations; FFR; cosmological parameters from CMBR; dark energy theory; standard candles