Table 1.
Open in new tab

Baseline ΛCDM cosmological parameters for the three simulation suites used in this work. The first column refers to the extension investigated within that particular suite. Ωm and Ωb are, respectively, the present-day background total matter and baryon density in units of the critical density, h = H0/100 is the dimensionless Hubble constant, As and ns are the amplitude and slope of the primordial power spectrum, and |$\sigma _8^\Lambda$| is the amplitude of mass fluctuations for the baseline ΛCDM cosmology.

ΩmΩbhnsAs × 109|$\sigma _8^\Lambda$|
DGP0.30720.04810.680.96452.0850.821
f(R)0.313150.04920.67370.96522.0970.822
DE0.260.0440.720.962.0820.79
ΩmΩbhnsAs × 109|$\sigma _8^\Lambda$|
DGP0.30720.04810.680.96452.0850.821
f(R)0.313150.04920.67370.96522.0970.822
DE0.260.0440.720.962.0820.79
Table 1.
Open in new tab

Baseline ΛCDM cosmological parameters for the three simulation suites used in this work. The first column refers to the extension investigated within that particular suite. Ωm and Ωb are, respectively, the present-day background total matter and baryon density in units of the critical density, h = H0/100 is the dimensionless Hubble constant, As and ns are the amplitude and slope of the primordial power spectrum, and |$\sigma _8^\Lambda$| is the amplitude of mass fluctuations for the baseline ΛCDM cosmology.

ΩmΩbhnsAs × 109|$\sigma _8^\Lambda$|
DGP0.30720.04810.680.96452.0850.821
f(R)0.313150.04920.67370.96522.0970.822
DE0.260.0440.720.962.0820.79
ΩmΩbhnsAs × 109|$\sigma _8^\Lambda$|
DGP0.30720.04810.680.96452.0850.821
f(R)0.313150.04920.67370.96522.0970.822
DE0.260.0440.720.962.0820.79
Close
This Feature Is Available To Subscribers Only

Sign In or Create an Account

Close

This PDF is available to Subscribers Only

View Article Abstract & Purchase Options

For full access to this pdf, sign in to an existing account, or purchase an annual subscription.

Close