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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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Variables | |
| CLASS_ROOT = None | |
| string | PREFIX = "std" |
| int | NSAMP = 100 |
| int | SEED = 10 |
| ZVALS = np.arange(0., 3., 0.5) | |
| dictionary | param_dict |
| string | class_datadir = "%s/data/class" |
| string | ccl_datadir = "%s/data/ccl" |
| string | root = "%s/%s" |
| string | ccl_root = "%s/%s" |
| sample_points | |
| nonlinear | |
| False | |
| redshifts | |
| True | |
| fname_pattern | |
| class_root | |
| precision | |
| class_data_root | |
| zvals | |
| default_params | |
| mode | |
| nonlin | |
Generate a set of CLASS power spectra across a set of sample points in cosmological parameter space, and compare with CCL.
| string run_pk_param_space.ccl_datadir = "%s/data/ccl" |
Definition at line 31 of file run_pk_param_space.py.
| string run_pk_param_space.ccl_root = "%s/%s" |
Definition at line 37 of file run_pk_param_space.py.
| run_pk_param_space.class_data_root |
Definition at line 73 of file run_pk_param_space.py.
| string run_pk_param_space.class_datadir = "%s/data/class" |
Definition at line 30 of file run_pk_param_space.py.
| run_pk_param_space.CLASS_ROOT = None |
Definition at line 10 of file run_pk_param_space.py.
| run_pk_param_space.class_root |
Definition at line 62 of file run_pk_param_space.py.
| run_pk_param_space.default_params |
Definition at line 74 of file run_pk_param_space.py.
| run_pk_param_space.False |
Definition at line 48 of file run_pk_param_space.py.
| run_pk_param_space.fname_pattern |
Definition at line 61 of file run_pk_param_space.py.
| run_pk_param_space.mode |
Definition at line 74 of file run_pk_param_space.py.
| run_pk_param_space.nonlin |
Definition at line 83 of file run_pk_param_space.py.
| run_pk_param_space.nonlinear |
Definition at line 48 of file run_pk_param_space.py.
Referenced by ccl_cosmology_compute_power_class(), ccl_cosmology_compute_power_emu(), ccl_cosmology_write_power_class_z(), and ccl_get_class_As().
| int run_pk_param_space.NSAMP = 100 |
Definition at line 16 of file run_pk_param_space.py.
| dictionary run_pk_param_space.param_dict |
Definition at line 21 of file run_pk_param_space.py.
| run_pk_param_space.precision |
Definition at line 62 of file run_pk_param_space.py.
Referenced by ccl_cosmology_compute_power_class(), ccl_cosmology_compute_power_emu(), ccl_cosmology_write_power_class_z(), and ccl_get_class_As().
| string run_pk_param_space.PREFIX = "std" |
Definition at line 15 of file run_pk_param_space.py.
| run_pk_param_space.redshifts |
Definition at line 48 of file run_pk_param_space.py.
| run_pk_param_space.root = "%s/%s" |
Definition at line 36 of file run_pk_param_space.py.
Referenced by nlohmann::detail::json_sax_dom_parser< BasicJsonType >.handle_value(), and nlohmann::detail::json_sax_dom_callback_parser< BasicJsonType >.handle_value().
| run_pk_param_space.sample_points |
Definition at line 40 of file run_pk_param_space.py.
| int run_pk_param_space.SEED = 10 |
Definition at line 17 of file run_pk_param_space.py.
| run_pk_param_space.True |
Definition at line 54 of file run_pk_param_space.py.
| run_pk_param_space.ZVALS = np.arange(0., 3., 0.5) |
Definition at line 18 of file run_pk_param_space.py.
| run_pk_param_space.zvals |
Definition at line 74 of file run_pk_param_space.py.