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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 | |
| pcs = csm.PcsPar() | |
| int | lm_arr = 11 |
| int | m_arr = 10 |
| float | z_arr = 0.2 |
| nm_arr = np.array([[pcs.multiplicity_function(m,z,"Tinker200")/pcs.dlsigMdlM(m) for m in m_arr] for z in z_arr]) | |
| string | head = "[0]mass " |
| int | iz = 1 |
| header | |
| string mfunc_bm.head = "[0]mass " |
Definition at line 16 of file mfunc_bm.py.
| mfunc_bm.header |
Definition at line 21 of file mfunc_bm.py.
| int mfunc_bm.iz = 1 |
Definition at line 17 of file mfunc_bm.py.
Referenced by assign_to_grid(), Grid< NDIM, T >.Grid(), Grid< NDIM, T >.grid_index_3d(), anonymous_namespace{test_chameleon.cpp}.init_overdensity(), anonymous_namespace{chameleon.cpp}.transform_Grid_to_Mesh(), and anonymous_namespace{chameleon.cpp}.transform_Mesh_to_Grid().
| int mfunc_bm.lm_arr = 11 |
Definition at line 11 of file mfunc_bm.py.
| int mfunc_bm.m_arr = 10 |
Definition at line 12 of file mfunc_bm.py.
| mfunc_bm.nm_arr = np.array([[pcs.multiplicity_function(m,z,"Tinker200")/pcs.dlsigMdlM(m) for m in m_arr] for z in z_arr]) |
Definition at line 14 of file mfunc_bm.py.
| mfunc_bm.pcs = csm.PcsPar() |
Definition at line 5 of file mfunc_bm.py.
| float mfunc_bm.z_arr = 0.2 |
Definition at line 13 of file mfunc_bm.py.