Impacts of dark energy on constraining neutrino mass after Planck 2018
Ming Zhang,Jing-Fei Zhang,Xin Zhang
Table 3. Fitting results of the cosmological parameters in the CPL+$\sum {m}_{\nu }$ model for three neutrino mass hierarchy cases, i.e. the DH case, the NH case, and the IH case, using the Planck+BAO+SNe and Planck+BAO+SNe+H0 data combinations.
DataPlanck+BAO+SNePlanck+BAO+SNe+H0
Mass orderingDHNHIHDHNHIH
w0−0.945 ± 0.087−0.933 ± 0.089−0.923 ± 0.089−1.003 ± 0.082−0.988 ± 0.086−0.978 ± 0.088
wa$-{0.41}_{-0.30}^{+0.44}$$-{0.52}_{-0.32}^{+0.46}$$-{0.61}_{-0.33}^{+0.46}$$-{0.38}_{-0.31}^{+0.41}$$-{0.50}_{-0.33}^{+0.44}$$-{0.60}_{-0.34}^{+0.45}$
H0 (km s−1 Mpc−1)68.22 ± 0.8368.19 ± 0.8368.14 ± 0.8469.78 ± 0.7369.71 ± 0.7469.69 ± 0.73
Ωm0.3087 ± 0.00820.3102 ± 0.00830.3113 ± 0.00830.2948 ± 0.00680.2965 ± 0.00700.2976 ± 0.0069
σ8${0.819}_{-0.015}^{+0.018}$${0.813}_{-0.015}^{+0.018}$${0.808}_{-0.015}^{+0.018}$${0.835}_{-0.015}^{+0.017}$${0.828}_{-0.014}^{+0.017}$${0.823}_{-0.014}^{+0.017}$
$\sum {m}_{\nu }$ (eV)<0.247<0.290<0.305<0.216<0.255<0.281

χ23804.6443805.9383806.5313816.7163817.8063818.809