@Article{Yang_etal2021,
author="Yang, W. Q.
and Pan, S.
and Di Valentino, E.
and Mena, O.
and Melchiorri, A.",
title="2021-H-0 odyssey: closed, phantom and interacting dark energy cosmologies",
journal="Journal of Cosmology and Astroparticle Physics",
year="2021",
publisher="IOP Publishing Ltd",
volume="10",
number="10",
pages="008--21pp",
optkeywords="baryon acoustic oscillations; cosmological parameters from CMBR; cosmological perturbation theory; dark energy theory",
abstract="Up-to-date cosmological data analyses have shown that (sigma) a closed universe is preferred by the Planck data at more than 99{\%} CL, and (b) interacting scenarios offer a very compelling solution to the Hubble constant tension. In light of these two recent appealing scenarios, we consider here an interacting dark matter-dark energy model with a non-zero spatial curvature component and a freely varying dark energy equation of state in both the quintessential and phantom regimes. When considering Cosmic Microwave Background data only, a phantom and closed universe can perfectly alleviate the Hubble tension, without the necessity of a coupling among the dark sectors. Accounting for other possible cosmological observations compromises the viability of this very attractive scenario as a global solution to current cosmological tensions, either by spoiling its effectiveness concerning the H-0 problem, as in the case of Supernovae Ia data, or by introducing a strong disagreement in the preferred value of the spatial curvature, as in the case of Baryon Acoustic Oscillations.",
optnote="WOS:000711524000011",
optnote="exported from refbase (https://references.ific.uv.es/refbase/show.php?record=5012), last updated on Wed, 10 Nov 2021 08:44:38 +0000",
issn="1475-7516",
doi="10.1088/1475-7516/2021/10/008",
opturl="https://arxiv.org/abs/2101.03129",
opturl="https://doi.org/10.1088/1475-7516/2021/10/008",
language="English"
}