Wiki

Clone wiki

cosmosis / default_modules / Halofit_Takahashi_Camb-Nov-13

Halofit_Takahashi module

Compute non-linear matter power spectrum

Name: Halofit_Takahashi

File: cosmosis-standard-library/boltzmann/halofit_takahashi/halofit_interface.so

Version: Camb-Nov-13

Author(s):

  • Antony Lewis
  • Simeon Bird

URL: http://camb.info

Cite:

Rules:

Assumptions:

  • Fitting formula from Takahashi et al applies only to LCDM

Explanation

Halofit is a fitting function based on simulations which models
the non-linear matter-power spectrum by scaling the linear one.

This Takahashi et al version improves over previous versions.

##Parameters

These parameters can be set in the module's section in the ini parameter file.
If no default is specified then the parameter is required.

Parameter Description
kmin real, minimum k in Mpc/h to generate values for (default 1e-4)
kmax real, maximum k in Mpc/h to generate values for (default 100.0
nk integer, number of log-spaced k values to sample (default 200)

##Inputs

These parameters and data are inputs to the module, either supplied as parameters by the sampler or computed by some previous module. They are loaded from the data block.

Section Parameter Description
cosmological_parameters omega_m real, Total matter density fraction today
omega_lambda real, Dark energy density fraction today
omega_nu real, Neutrino density fraction today (default 0.0)
w real, Dark energy equation of state (default -1)
matter_power_lin k_h real 1D array, sample values of linear spectrum in Mpc/h
z real 1D array, redshift of linear spectrum samples
P_k real 2D array, linear spectrum in (Mpc/h)^{-3}

##Outputs

These parameters and data are computed as outputs from the module

Section Parameter Description
matter_power_nl k_h real 1D array, sample values of nonlinear spectrum in Mpc/h
z real 1D array, redshift of nonlinear spectrum samples
P_k real 2D array, nonlinear spectrum in (Mpc/h)^{-3}

Updated