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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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Go to the source code of this file.
Classes | |
| class | cl_cmblx_bm.Power_Spectra |
Namespaces | |
| cl_cmblx_bm | |
Variables | |
| cl_cmblx_bm.c = c.to(u.km/u.second) | |
| cl_cmblx_bm.cosmo_fid | |
| cl_cmblx_bm.cosmo | |
| cl_cmblx_bm.cosmo_h = cosmo.clone(H0=100) | |
| dictionary | cl_cmblx_bm.pk_params = {'non_linear':0,'kmax':1E3,'kmin':5.e-5,'nk':5000} |
| cl_cmblx_bm.PS = Power_Spectra() | |
| cl_cmblx_bm.zg | |
| cl_cmblx_bm.l | |
| cl_cmblx_bm.cl_g_cmb | |
| cl_cmblx_bm.pk_func | |
| cl_cmblx_bm.ccl_pk_bbks | |
| cl_cmblx_bm.zs | |
| cl_cmblx_bm.p_zs | |
| cl_cmblx_bm.p_zg | |
| cl_cmblx_bm.bias_g | |
| cl_cmblx_bm.fmt | |
| float | cl_cmblx_bm.sigz1 = 0.15 |
| cl_cmblx_bm.zav = np.linspace(0,10.,10000) | |
| int | cl_cmblx_bm.pza = 1 |
| dictionary | cl_cmblx_bm.za = {'z':zav,'pz':pza} |
| cl_cmblx_bm.n_zl | |
| cl_cmblx_bm.zs2 | |
| cl_cmblx_bm.p_zs2 | |
| cl_cmblx_bm.zl_max | |