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Fast Methods for Cosmological Simulations
FastSim serves as a tool for quick N-body simulations in modified gravity.
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#include <ccl_core.h>
Public Attributes | |
| double | growth0 |
| gsl_spline * | chi |
| gsl_spline * | growth |
| gsl_spline * | fgrowth |
| gsl_spline * | E |
| gsl_spline * | achi |
| gsl_interp_accel * | accelerator |
| gsl_interp_accel * | accelerator_achi |
| gsl_interp_accel * | accelerator_m |
| gsl_interp_accel * | accelerator_d |
| gsl_interp_accel * | accelerator_k |
| gsl_spline * | logsigma |
| gsl_spline * | dlnsigma_dlogm |
| gsl_spline * | alphahmf |
| gsl_spline * | betahmf |
| gsl_spline * | gammahmf |
| gsl_spline * | phihmf |
| gsl_spline * | etahmf |
| gsl_spline2d * | p_lin |
| gsl_spline2d * | p_nl |
| double | k_min_lin |
| double | k_min_nl |
| double | k_max_lin |
| double | k_max_nl |
Struct containing references to gsl splines for distance and acceleration calculations
Definition at line 77 of file ccl_core.h.
| gsl_interp_accel* ccl_data::accelerator |
Definition at line 91 of file ccl_core.h.
Referenced by ccl_comoving_angular_distance(), ccl_comoving_radial_distance(), ccl_cosmology_compute_distances(), ccl_cosmology_compute_growth(), ccl_cosmology_compute_power_emu(), ccl_cosmology_create(), ccl_data_free(), ccl_growth_factor(), ccl_growth_rate(), ccl_h_over_h0(), ccl_omega_x(), and h_over_h0().
| gsl_interp_accel* ccl_data::accelerator_achi |
Definition at line 92 of file ccl_core.h.
Referenced by ccl_cosmology_create(), ccl_data_free(), and ccl_scale_factor_of_chi().
| gsl_interp_accel* ccl_data::accelerator_d |
Definition at line 94 of file ccl_core.h.
Referenced by ccl_cosmology_compute_hmfparams(), ccl_cosmology_create(), ccl_data_free(), and massfunc_f().
| gsl_interp_accel* ccl_data::accelerator_k |
Definition at line 96 of file ccl_core.h.
Referenced by ccl_cosmology_create(), and ccl_data_free().
| gsl_interp_accel* ccl_data::accelerator_m |
Definition at line 93 of file ccl_core.h.
Referenced by ccl_cosmology_compute_sigma(), ccl_cosmology_create(), ccl_data_free(), ccl_dlninvsig_dlogm(), and ccl_sigmaM().
| gsl_spline* ccl_data::achi |
Definition at line 86 of file ccl_core.h.
Referenced by ccl_cosmology_compute_distances(), ccl_cosmology_create(), ccl_data_free(), and ccl_scale_factor_of_chi().
| gsl_spline* ccl_data::alphahmf |
Definition at line 104 of file ccl_core.h.
Referenced by ccl_cosmology_compute_hmfparams(), ccl_cosmology_create(), ccl_data_free(), and massfunc_f().
| gsl_spline* ccl_data::betahmf |
Definition at line 105 of file ccl_core.h.
Referenced by ccl_cosmology_compute_hmfparams(), ccl_cosmology_create(), ccl_data_free(), and massfunc_f().
| gsl_spline* ccl_data::chi |
Definition at line 82 of file ccl_core.h.
Referenced by ccl_comoving_angular_distance(), ccl_comoving_radial_distance(), ccl_cosmology_compute_distances(), ccl_cosmology_create(), and ccl_data_free().
| gsl_spline* ccl_data::dlnsigma_dlogm |
Definition at line 101 of file ccl_core.h.
Referenced by ccl_cosmology_compute_sigma(), ccl_cosmology_create(), ccl_data_free(), and ccl_dlninvsig_dlogm().
| gsl_spline* ccl_data::E |
Definition at line 85 of file ccl_core.h.
Referenced by ccl_cosmology_compute_distances(), ccl_cosmology_create(), ccl_data_free(), and ccl_h_over_h0().
| gsl_spline* ccl_data::etahmf |
Definition at line 108 of file ccl_core.h.
Referenced by ccl_cosmology_compute_hmfparams(), ccl_cosmology_create(), ccl_data_free(), and massfunc_f().
| gsl_spline* ccl_data::fgrowth |
Definition at line 84 of file ccl_core.h.
Referenced by ccl_cosmology_compute_growth(), ccl_cosmology_create(), ccl_data_free(), and ccl_growth_rate().
| gsl_spline* ccl_data::gammahmf |
Definition at line 106 of file ccl_core.h.
Referenced by ccl_cosmology_compute_hmfparams(), ccl_cosmology_create(), ccl_data_free(), and massfunc_f().
| gsl_spline* ccl_data::growth |
Definition at line 83 of file ccl_core.h.
Referenced by ccl_cosmology_compute_growth(), ccl_cosmology_create(), ccl_data_free(), and ccl_growth_factor().
| double ccl_data::growth0 |
Definition at line 81 of file ccl_core.h.
Referenced by ccl_cosmology_compute_growth(), ccl_cosmology_create(), and ccl_growth_factor_unnorm().
| double ccl_data::k_max_lin |
Definition at line 115 of file ccl_core.h.
Referenced by ccl_cosmology_compute_power_bbks(), ccl_cosmology_compute_power_class(), ccl_cosmology_compute_power_eh(), ccl_cosmology_compute_power_emu(), and ccl_linear_matter_power().
| double ccl_data::k_max_nl |
Definition at line 116 of file ccl_core.h.
Referenced by ccl_cosmology_compute_power_bbks(), ccl_cosmology_compute_power_class(), ccl_cosmology_compute_power_eh(), ccl_cosmology_compute_power_emu(), and ccl_nonlin_matter_power().
| double ccl_data::k_min_lin |
Definition at line 113 of file ccl_core.h.
Referenced by ccl_cosmology_compute_power_bbks(), ccl_cosmology_compute_power_class(), ccl_cosmology_compute_power_eh(), ccl_cosmology_compute_power_emu(), and ccl_linear_matter_power().
| double ccl_data::k_min_nl |
Definition at line 114 of file ccl_core.h.
Referenced by ccl_cosmology_compute_power_bbks(), ccl_cosmology_compute_power_class(), ccl_cosmology_compute_power_eh(), ccl_cosmology_compute_power_emu(), and ccl_nonlin_matter_power().
| gsl_spline* ccl_data::logsigma |
Definition at line 100 of file ccl_core.h.
Referenced by ccl_cosmology_compute_sigma(), ccl_cosmology_create(), ccl_data_free(), and ccl_sigmaM().
| gsl_spline2d* ccl_data::p_lin |
Definition at line 111 of file ccl_core.h.
Referenced by ccl_cosmology_compute_power_bbks(), ccl_cosmology_compute_power_class(), ccl_cosmology_compute_power_eh(), ccl_cosmology_compute_power_emu(), ccl_cosmology_create(), ccl_data_free(), and ccl_linear_matter_power().
| gsl_spline2d* ccl_data::p_nl |
Definition at line 112 of file ccl_core.h.
Referenced by ccl_cosmology_compute_power_bbks(), ccl_cosmology_compute_power_class(), ccl_cosmology_compute_power_eh(), ccl_cosmology_compute_power_emu(), ccl_cosmology_create(), ccl_data_free(), and ccl_nonlin_matter_power().
| gsl_spline* ccl_data::phihmf |
Definition at line 107 of file ccl_core.h.
Referenced by ccl_cosmology_compute_hmfparams(), ccl_cosmology_create(), ccl_data_free(), and massfunc_f().