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 5. Fitting results for the IΛCDM4+$\sum {m}_{\nu }$ ($Q=\beta {H}_{0}{\rho }_{{\rm{c}}}$) 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+$\sum {m}_{\nu }^{\mathrm{DH}}$
${{\rm{\Omega }}}_{{\rm{m}}}$0.299 ± 0.0160.297 ± 0.016${0.302}_{-0.017}^{+0.016}$0.272 ± 0.0130.269 ± 0.0130.275 ± 0.013
${H}_{0}$68.05 ± 0.80${68.07}_{-0.82}^{+0.83}$68.07 ± 0.8169.58 ± 0.7269.58 ± 0.73${69.58}_{-0.72}^{+0.71}$
β0.043 ± 0.047${0.058}_{-0.048}^{+0.047}$${0.024}_{-0.048}^{+0.047}$0.111 ± 0.0430.128 ± 0.0430.092 ± 0.044
${\sigma }_{8}$${0.814}_{-0.021}^{+0.019}$0.812 ± 0.019${0.820}_{-0.020}^{+0.019}$0.840 ± 0.0190.837 ± 0.0190.845 ± 0.019
$\sum {m}_{\nu }$ $\lt 0.202$$\lt 0.235$<0.156<0.202<0.239<0.162