Table 3.

Model selection results with four current data sets including Planck, assuming a Gaussian prior centred on w0 = −1 with a prior width of 0.5. Most of the data favour ΛCDM. A combination of Planck, WP and H0 data shows positive evidence for dynamical dark energy. Note that this calculation uses a rather restrictive prior. This model of dynamical dark energy would have an equation-of-state parameter in the range −1.5 < w0 < −0.5.

Current dataw0σln B01Evidence
Planck+WP+BAO−1.130.1200.900Positive for ΛCDM
Planck+WP+Union2.1−1.090.0851.241Positive for ΛCDM
Planck+WP+SNLS−1.130.0650.082Inconclusive to weak for ΛCDM
Planck+WP+H0−1.240.090−1.713Positive for wCDM
Current dataw0σln B01Evidence
Planck+WP+BAO−1.130.1200.900Positive for ΛCDM
Planck+WP+Union2.1−1.090.0851.241Positive for ΛCDM
Planck+WP+SNLS−1.130.0650.082Inconclusive to weak for ΛCDM
Planck+WP+H0−1.240.090−1.713Positive for wCDM
Table 3.

Model selection results with four current data sets including Planck, assuming a Gaussian prior centred on w0 = −1 with a prior width of 0.5. Most of the data favour ΛCDM. A combination of Planck, WP and H0 data shows positive evidence for dynamical dark energy. Note that this calculation uses a rather restrictive prior. This model of dynamical dark energy would have an equation-of-state parameter in the range −1.5 < w0 < −0.5.

Current dataw0σln B01Evidence
Planck+WP+BAO−1.130.1200.900Positive for ΛCDM
Planck+WP+Union2.1−1.090.0851.241Positive for ΛCDM
Planck+WP+SNLS−1.130.0650.082Inconclusive to weak for ΛCDM
Planck+WP+H0−1.240.090−1.713Positive for wCDM
Current dataw0σln B01Evidence
Planck+WP+BAO−1.130.1200.900Positive for ΛCDM
Planck+WP+Union2.1−1.090.0851.241Positive for ΛCDM
Planck+WP+SNLS−1.130.0650.082Inconclusive to weak for ΛCDM
Planck+WP+H0−1.240.090−1.713Positive for wCDM
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