Table 1
Cosmological parameters used in our analysis.
Parameter | Prior range | Baseline | Definition |
|
|||
ωb ≡ Ωbh2 ........ | [0.005,0.1] | ... | Baryon density today |
ωc ≡ Ωch2 ........ | [0.001,0.99] | ... | Cold dark matter density today |
100θMC ........ | [0.5,10.0] | ... | 100 × approximation to r∗/DA (CosmoMC) |
τ ........ | [0.01,0.8] | ... | Thomson scattering optical depth due to reionization |
ΩK ........ | [− 0.3,0.3] | 0 | Curvature parameter today with Ωtot = 1 − ΩK |
∑ mν ........ | [0,5] | 0.06 | The sum of neutrino masses in eV |
![]() |
[0,3] | 0 | Effective mass of sterile neutrino in eV |
w0 ........ | [−3.0, −0.3] | −1 | Dark energy equation of statea, w(a) = w0 + (1 − a)wa |
wa ........ | [− 2,2] | 0 | As above (perturbations modelled using PPF) |
Neff ........ | [0.05,10.0] | 3.046 | Effective number of neutrino-like relativistic degrees of freedom (see text) |
YP ........ | [0.1,0.5] | BBN | Fraction of baryonic mass in helium |
AL ........ | [0,10] | 1 | Amplitude of the lensing power relative to the physical value |
ns ........ | [0.9,1.1] | ... | Scalar spectrum power-law index (k0 = 0.05 Mpc-1) |
nt ........ | nt = − r0.05/ 8 | Inflation | Tensor spectrum power-law index (k0 = 0.05 Mpc-1) |
dns/ dlnk ........ | [−1,1] | 0 | Running of the spectral index |
ln(1010As) ........ | [2.7,4.0] | ... | Log power of the primordial curvature perturbations (k0 = 0.05 Mpc-1) |
r0.05 ........ | [0,2] | 0 | Ratio of tensor primordial power to curvature power at k0 = 0.05 Mpc-1 |
|
|||
ΩΛ ........ | ... | Dark energy density divided by the critical density today | |
t0 ........ | ... | Age of the Universe today (in Gyr) | |
Ωm ........ | ... | Matter density (inc. massive neutrinos) today divided by the critical density | |
σ8 ........ | ... | RMS matter fluctuations today in linear theory | |
zre ........ | ... | Redshift at which Universe is half reionized | |
H0 ........ | [20,100] | ... | Current expansion rate in km s-1Mpc-1 |
r0.002 ........ | 0 | Ratio of tensor primordial power to curvature power at k0 = 0.002 Mpc-1 | |
109As ........ | ... | 109 × dimensionless curvature power spectrum at k0 = 0.05 Mpc-1 | |
ωm ≡ Ωmh2 ........ | ... | Total matter density today (inc. massive neutrinos) | |
|
|||
z∗ ........ | ... | Redshift for which the optical depth equals unity (see text) | |
r∗ = rs(z∗) ........ | ... | Comoving size of the sound horizon at z = z∗ | |
100θ∗ ........ | ... | 100 × angular size of sound horizon at z = z∗ (r∗/DA) | |
zdrag ........ | ... | Redshift at which baryon-drag optical depth equals unity (see text) | |
rdrag = rs(zdrag) ........ | ... | Comoving size of the sound horizon at z = zdrag | |
kD ........ | ... | Characteristic damping comoving wavenumber (Mpc-1) | |
100θD ........ | ... | 100 × angular extent of photon diffusion at last scattering (see text) | |
zeq ........ | ... | Redshift of matter-radiation equality (massless neutrinos) | |
100θeq ........ | ... | 100 × angular size of the comoving horizon at matter-radiation equality | |
rdrag/DV(0.57) ........ | ... | BAO distance ratio at z = 0.57 (see Sect. 5.2) |
Notes. For each, we give the symbol, prior range, value taken in the base ΛCDM cosmology (where appropriate), and summary definition (see text for details). The top block contains parameters with uniform priors that are varied in the MCMC chains. The ranges of these priors are listed in square brackets. The lower blocks define various derived parameters.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.