Table 3
Bayesian evidence for the cosmological models tested.
| Cosmology | Bayesian evidence |
|---|---|
| ΛCDM | −11419.6 ± 0.7 |
| ΛCDM with ∑ mv = 0.06 eV | −11418.3 ± 0.5 |
| vCDM | −11418.8 ± 0.8 |
| wCDM | −11419.5 ± 0.5 |
| vwCDM | −11421.2 ± 0.6 |
Notes. To interpret this table, we need the Jeffreys scale (Jeffreys 1961): if the difference between the two is greater than 5, then there is significant evidence to prefer the model with the largest Bayesian evidence; if the difference between the two is between 2.5 and 5, then there is weak preference for the model with the largest Bayesian evidence; otherwise, the models are statistically indistinguishable.
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