Constraints on neutrino mass in the scenario of vacuum energy interacting with cold dark matter after Planck 2018
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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 5. The one-dimensional posterior distributions for the parameter H0 for the ΛCDM+$\sum {m}_{\nu }$ (NH, IH, and DH) model and IΛCDM1+$\sum {m}_{\nu }$ (NH, IH, and DH) model with $Q=\beta H{\rho }_{\mathrm{de}}$ by using the CMB+BAO+SN data combination. The result of the local measurement of Hubble constant (${H}_{0}=74.03\pm 1.42\,\mathrm{km}\,{{\rm{s}}}^{-1}\,{\mathrm{Mpc}}^{-1}$) is shown by the hotpink band. |
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