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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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Public Attributes | |
| int | il |
| ccl_cosmology * | cosmo |
| CCL_ClWorkspace * | w |
| CCL_ClTracer * | clt1 |
| CCL_ClTracer * | clt2 |
| int * | status |
| int | l |
| RunParams * | par |
| char * | tr1 |
| char * | tr2 |
| CCL_ClTracer* IntClPar::clt1 |
Definition at line 817 of file ccl_cls.c.
Referenced by ccl_angular_cl_native(), and cl_integrand().
| CCL_ClTracer* IntClPar::clt2 |
Definition at line 818 of file ccl_cls.c.
Referenced by ccl_angular_cl_native(), and cl_integrand().
| ccl_cosmology* IntClPar::cosmo |
Definition at line 815 of file ccl_cls.c.
Referenced by ccl_angular_cl_native(), cl_integrand(), and cl_cmblx_bm.Power_Spectra::DZ_int().
| int IntClPar::il |
Definition at line 814 of file ccl_cls.c.
Referenced by ccl_angular_cl_native(), and cl_integrand().
| int IntClPar::l |
Definition at line 4 of file spectra.c.
Referenced by cl_integrand(), and spectra().
| RunParams* IntClPar::par |
Definition at line 5 of file spectra.c.
Referenced by cl_integrand(), and spectra().
| int* IntClPar::status |
Definition at line 819 of file ccl_cls.c.
Referenced by ccl_angular_cl_native(), and cl_integrand().
| char* IntClPar::tr1 |
Definition at line 6 of file spectra.c.
Referenced by cl_integrand(), and spectra().
| char* IntClPar::tr2 |
Definition at line 7 of file spectra.c.
Referenced by cl_integrand(), and spectra().
| CCL_ClWorkspace* IntClPar::w |
Definition at line 816 of file ccl_cls.c.
Referenced by ccl_angular_cl_native(), and cl_integrand().