TY  - JOUR
AU  - Yang, W. Q.
AU  - Di Valentino, E.
AU  - Pan, S.
AU  - Mena, O.
PY  - 2021
DA  - 2021//
TI  - Emergent Dark Energy, neutrinos and cosmological tensions
T2  - Phys. Dark Universe
JO  - Physics of the Dark Universe
SP  - 100762
EP  - 9pp
VL  - 31
PB  - Elsevier
AB  - The Phenomenologically Emergent Dark Energy model, a dark energy model with the same number of free parameters as the flat Lambda CDM, has been proposed as a working example of a minimal model which can avoid the current cosmological tensions. A straightforward question is whether or not the inclusion of massive neutrinos and extra relativistic species may spoil such an appealing phenomenological alternative. We present the bounds on M-nu and N-eff and comment on the long standing H-0 and sigma(8) tensions within this cosmological framework with a wealth of cosmological observations. Interestingly, we find, at 95% confidence level, and with the most complete set of cosmological observations, M-nu similar to 0.21(-0.14)(+0.15) eV and N-eff = 3.03 +/- 0.32 i.e. an indication for a non-zero neutrino mass with a significance above 2 sigma. The well known Hubble constant tension is considerably easened, with a significance always below the 2 sigma level. (C) 2020 Elsevier B.V. All rights reserved.
SN  - 2212-6864
UR  - https://arxiv.org/abs/2007.02927
UR  - https://doi.org/10.1016/j.dark.2020.100762
DO  - 10.1016/j.dark.2020.100762
LA  - English
N1  - WOS:000630235100022
ID  - Yang_etal2021
ER  -