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 $N_{\mathrm{eff}}$ 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, $M_{\nu }\sim 0.21_{-0.14}^{+0.15}\mathrm{eV}$ and $N_{\mathrm{eff}}=3.03\pm 0.32$ 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.

现象学上出现的暗能量模型，一种暗能量模型，其自由参数的数量与单位相同 $\Lambda$有人提出CDM作为最小模型的工作示例，它可以避免当前的宇宙学张力。一个直接的问题是，包含大量中微子和相对论物种是否会破坏这种吸引人的现象学选择。我们提出界限${\mathrm{中号}}_{\nu }$ 和 ${ñ}_{\mathrm{效}}$ 并评论长期存在 $H_0$ 和 ${\sigma }_8$在这个宇宙学框架内的紧张关系以及大量的宇宙学观察。有趣的是，我们发现置信水平为95％，并且通过最完整的宇宙学观测，${\mathrm{中号}}_{\nu }〜0。2{\mathrm{1个}}_{-0。14}^{+0。15}\mathrm{电子伏特}$ 和 ${ñ}_{\mathrm{效}}=3。03\pm 0。32$ 也就是说，具有高于上述意义的中微子质量为非零的指示 $2\sigma$。众所周知的哈勃恒张力已经大大减轻，其重要性始终低于$2\sigma$ 水平。