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Constraints on neutrino mass in the scenario of vacuum energy interacting with cold dark matter after Planck 2018
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Hai-Li Li,Jing-Fei Zhang,Xin Zhang
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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.
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Data | CMB+BAO+SN | CMB+BAO+SN+H0 |
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Model | IΛCDM+$\sum {m}_{\nu }^{\mathrm{NH}}$ | 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+$\sum {m}_{\nu }^{\mathrm{DH}}$ |
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${{\rm{\Omega }}}_{{\rm{m}}}$ | 0.299 ± 0.016 | 0.297 ± 0.016 | ${0.302}_{-0.017}^{+0.016}$ | 0.272 ± 0.013 | 0.269 ± 0.013 | 0.275 ± 0.013 | ${H}_{0}$ | 68.05 ± 0.80 | ${68.07}_{-0.82}^{+0.83}$ | 68.07 ± 0.81 | 69.58 ± 0.72 | 69.58 ± 0.73 | ${69.58}_{-0.72}^{+0.71}$ | β | 0.043 ± 0.047 | ${0.058}_{-0.048}^{+0.047}$ | ${0.024}_{-0.048}^{+0.047}$ | 0.111 ± 0.043 | 0.128 ± 0.043 | 0.092 ± 0.044 | ${\sigma }_{8}$ | ${0.814}_{-0.021}^{+0.019}$ | 0.812 ± 0.019 | ${0.820}_{-0.020}^{+0.019}$ | 0.840 ± 0.019 | 0.837 ± 0.019 | 0.845 ± 0.019 | $\sum {m}_{\nu }$ | $\lt 0.202$ | $\lt 0.235$ | <0.156 | <0.202 | <0.239 | <0.162 |
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