|
Fast Methods for Cosmological Simulations
FastSim serves as a tool for quick N-body simulations in modified gravity.
|
#include "ccl_constants.h"

Go to the source code of this file.
Classes | |
| struct | ccl_spline_params |
| struct | ccl_gsl_params |
Typedefs | |
| typedef CCL_BEGIN_DECLS struct ccl_spline_params | ccl_spline_params |
| typedef struct ccl_gsl_params | ccl_gsl_params |
Variables | |
| ccl_spline_params * | ccl_splines |
| ccl_gsl_params * | ccl_gsl |
| typedef struct ccl_gsl_params ccl_gsl_params |
Struct that contains parameters that control the accuracy of various GSL routines.
| typedef CCL_BEGIN_DECLS struct ccl_spline_params ccl_spline_params |
Struct that contains all the parameters needed to create certain splines. This includes splines for the scale factor, masses, and power spectra.
| ccl_gsl_params* ccl_gsl |
Definition at line 48 of file ccl_core.c.
Referenced by a_of_chi(), calculate_nu_phasespace_spline(), ccl_angular_cl_native(), ccl_cosmology_compute_growth(), ccl_dNdz_tomog(), ccl_norm_integrand(), ccl_sigmaR(), ccl_sigmaV(), ccl_tracer_corr_bessel(), clt_init_nz(), compare_cls(), compare_corr(), compute_chi(), growth_factor_and_growth_rate(), window_lensing(), and window_magnification().
| ccl_spline_params* ccl_splines |
Definition at line 47 of file ccl_core.c.
Referenced by calculate_nu_phasespace_spline(), ccl_correlation_3d(), ccl_cosmology_compute_distances(), ccl_cosmology_compute_growth(), ccl_cosmology_compute_power_bbks(), ccl_cosmology_compute_power_class(), ccl_cosmology_compute_power_eh(), ccl_cosmology_compute_power_emu(), ccl_cosmology_compute_sigma(), ccl_dNdz_tomog(), ccl_fill_class_parameters(), ccl_linear_matter_power(), ccl_nonlin_matter_power(), ccl_norm_integrand(), ccl_sigmaR(), ccl_sigmaV(), ccl_tracer_corr_bessel(), ccl_tracer_corr_fftlog(), ccl_tracer_corr_legendre(), get_k_interval(), and main().