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 |
Figure 7. The one-dimensional posterior distributions for the parameter H0 for the IΛCDM1+∑mν (NH, IH, and DH) model with Q=βHρde by using the CMB+BAO+SN and CMB+BAO+SN+H0 data combinations, respectively. The result of the local measurement of Hubble constant (H0=74.03±1.42kms−1Mpc−1) is shown by the hotpink band. |
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