@Article{DiValentino_etal2020,
author="Di Valentino, E.
and Melchiorri, A.
and Mena, O.
and Vagnozzi, S.",
title="Interacting dark energy in the early 2020s: A promising solution to the H-0 and cosmic shear tensions",
journal="Physics of the Dark Universe",
year="2020",
publisher="Elsevier",
volume="30",
pages="100666--12pp",
optkeywords="Hubble tension; Cosmological parameters; Dark matter; Dark energy; Interacting dark energy",
abstract="We examine interactions between dark matter and dark energy in light of the latest cosmological observations, focusing on a specific model with coupling proportional to the dark energy density. Our data includes Cosmic Microwave Background (CMB) measurements from the Planck 2018 legacy data release, late-time measurements of the expansion history from Baryon Acoustic Oscillations (BAO) and Supernovae Type Ia (SNeIa), galaxy clustering and cosmic shear measurements from the Dark Energy Survey Year 1 results, and the 2019 local distance ladder measurement of the Hubble constant H-0 from the Hubble Space Telescope. Considering Planck data both in combination with BAO or SNeIa data reduces the H-0 tension to a level which could possibly be compatible with a statistical fluctuation. The very same model also significantly reduces the Omega(m) -- sigma(8) tension between CMB and cosmic shear measurements. Interactions between the dark sectors of our Universe remain therefore a promising joint solution to these persisting cosmological tensions.",
optnote="WOS:000595300400037",
optnote="exported from refbase (https://references.ific.uv.es/refbase/show.php?record=4646), last updated on Wed, 06 Jan 2021 10:44:06 +0000",
issn="2212-6864",
doi="10.1016/j.dark.2020.100666",
opturl="https://arxiv.org/abs/1908.04281",
opturl="https://doi.org/10.1016/j.dark.2020.100666",
language="English"
}