Constraints on neutrino mass in the scenario of vacuum energy interacting with cold dark matter after Planck 2018
Hai-Li Li,Jing-Fei Zhang,Xin Zhang
Table 2. Fitting results for the IΛCDM1+$\sum {m}_{\nu }$ ($Q=\beta H{\rho }_{\mathrm{de}}$) model by using the CMB+BAO+SN and CMB+BAO+SN+H0 data combinations, respectively. Here, H0 and $\sum {m}_{\nu }$ are in units of km s−1 Mpc−1 and eV, respectively.
DataCMB+BAO+SNCMB+BAO+SN+H0
ModelIΛCDM+$\sum {m}_{\nu }^{\mathrm{NH}}$IΛCDM+$\sum {m}_{\nu }^{\mathrm{IH}}$IΛCDM+$\sum {m}_{\nu }^{\mathrm{DH}}$IΛCDM+$\sum {m}_{\nu }^{\mathrm{NH}}$IΛCDM+$\sum {m}_{\nu }^{\mathrm{IH}}$IΛCDM+$\sum {m}_{\nu }^{\mathrm{DH}}$
Ωm0.285 ± 0.0290.279 ± 0.030${0.292}_{-0.030}^{+0.029}$0.235 ± 0.0270.229 ± 0.027${0.243}_{-0.027}^{+0.028}$
${H}_{0}$68.08 ± 0.81${68.08}_{-0.82}^{+0.83}$68.14 ± 0.83${69.64}_{-0.72}^{+0.73}$${69.62}_{-0.73}^{+0.75}$${69.67}_{-0.75}^{+0.74}$
β${0.10}_{-0.11}^{+0.10}$0.13 ± 0.11${0.07}_{-0.11}^{+0.10}$${0.257}_{-0.097}^{+0.096}$0.286 ± 0.0980.215 ± 0.099
${\sigma }_{8}$${0.870}_{-0.088}^{+0.058}$${0.884}_{-0.094}^{+0.061}$${0.859}_{-0.085}^{+0.056}$${1.013}_{-0.123}^{+0.076}$${1.031}_{-0.131}^{+0.081}$${0.987}_{-0.117}^{+0.073}$
$\sum {m}_{\nu }$ <0.189<0.218<0.151<0.177<0.209<0.138