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 3. Observational constraints (68.3% and 95.4% confidence level) on the IΛCDM3+$\sum {m}_{\nu }$ ($Q=\beta {H}_{0}{\rho }_{\mathrm{de}}$) model by using the CMB+BAO+SN (left) and CMB+BAO+SN+H0 (right) data combinations, respectively. |