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add a 3d inputs for the massive star problem (#2763)
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# ------------------ INPUTS TO MAIN PROGRAM ------------------- | ||
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amr.plot_files_output = 1 | ||
amr.checkpoint_files_output = 1 | ||
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max_step = 50 | ||
stop_time = 360000 | ||
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geometry.is_periodic = 0 0 | ||
geometry.coord_sys = 0 # r-z coordinates | ||
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geometry.prob_lo = 0. 0. 0. | ||
geometry.prob_hi = 1.6384e10 1.6384e10 1.6384e10 | ||
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amr.n_cell = 512 512 512 | ||
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amr.max_level = 3 # maximum level number allowed | ||
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castro.lo_bc = 2 2 2 | ||
castro.hi_bc = 2 2 2 | ||
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# >>>>>>>>>>>>> BC FLAGS <<<<<<<<<<<<<<<< | ||
# 0 = Interior 3 = Symmetry | ||
# 1 = Inflow 4 = SlipWall | ||
# 2 = Outflow 5 = NoSlipWall | ||
# >>>>>>>>>>>>> BC FLAGS <<<<<<<<<<<<<<<< | ||
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# GPU options | ||
castro.hydro_memory_footprint_ratio = 3 | ||
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castro.do_hydro = 1 | ||
castro.do_grav = 1 | ||
castro.do_react = 1 | ||
castro.do_sponge = 1 | ||
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castro.ppm_type = 1 | ||
castro.ppm_temp_fix = 0 | ||
castro.use_pslope = 1 | ||
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castro.use_flattening = 1 | ||
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castro.riemann_solver = 1 | ||
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gravity.gravity_type = MonopoleGrav | ||
gravity.drdxfac = 2 | ||
castro.grav_source_type = 4 | ||
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castro.sponge_upper_density = 1.e3 | ||
castro.sponge_lower_density = 1.e2 | ||
castro.sponge_timescale = 1.e-3 | ||
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castro.cfl = 0.4 # cfl number for hyperbolic system | ||
castro.init_shrink = 0.01 # scale back initial timestep by this factor | ||
castro.change_max = 1.2 # factor by which dt is allowed to change each timestep | ||
castro.sum_interval = 10 # timesteps between computing and printing volume averages | ||
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#castro.dtnuc_e = 0.25 | ||
#castro.dtnuc_X = 0.25 | ||
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amr.ref_ratio = 2 2 2 2 # refinement ratio | ||
amr.regrid_int = 10000 # how often to regrid | ||
amr.n_error_buf = 4 2 2 2 # number of buffer cells in error est | ||
amr.grid_eff = 0.7 # what constitutes an efficient grid | ||
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amr.check_file = massive_star_chk # root name of checkpoint file | ||
amr.check_int = 200 # number of timesteps between checkpoints | ||
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amr.plot_file = massive_star_plt # root name of plot file | ||
amr.plot_per = 5.0 | ||
amr.derive_plot_vars = ALL | ||
castro.store_burn_weights = 0 | ||
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amr.small_plot_file = massive_star_smallplt # root name of plot file | ||
amr.small_plot_per = 0.5 | ||
amr.small_plot_vars = density Temp in_nse\ | ||
amr.derive_small_plot_vars = abar Ye enuc MachNumber magvel magvort | ||
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fab.format = NATIVE_32 | ||
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castro.plot_per_is_exact = 0 | ||
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amr.max_grid_size = 64 # maximum grid size allowed -- used to control parallelism | ||
amr.blocking_factor = 32 # block factor in grid generation | ||
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amr.v = 1 # control verbosity in Amr.cpp | ||
castro.v = 1 # control verbosity in Castro.cpp | ||
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castro.small_dens = 1.0 | ||
castro.small_temp = 1.e6 | ||
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castro.time_integration_method = 3 | ||
castro.use_retry = 1 | ||
castro.max_subcycles = 16 | ||
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# problem initialization | ||
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problem.model_name = "15m_500_sec.aprox19.hse.5.00km" | ||
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problem.perturb_model = 1 | ||
problem.velpert_amplitude = 5.e6 | ||
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problem.interpolate_pres = 1 | ||
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# convection | ||
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castro.drive_initial_convection = 1 | ||
castro.drive_initial_convection_reinit_period = 2 | ||
castro.drive_initial_convection_tmax = 50 | ||
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# refinement | ||
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amr.refinement_indicators = denerr denerr2 denerr3 | ||
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amr.refine.denerr.max_level = 1 | ||
amr.refine.denerr.value_greater = 1.e3 | ||
amr.refine.denerr.field_name = density | ||
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amr.refine.denerr2.max_level = 2 | ||
amr.refine.denerr2.value_greater = 1.e4 | ||
amr.refine.denerr2.field_name = density | ||
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amr.refine.denerr3.max_level = 3 | ||
amr.refine.denerr3.value_greater = 1.e5 | ||
amr.refine.denerr3.field_name = density | ||
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# Microphysics | ||
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integrator.rtol_spec = 1.e-5 | ||
integrator.atol_spec = 1.e-5 | ||
integrator.rtol_enuc = 1.e-5 | ||
integrator.atol_enuc = 1.e-5 | ||
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integrator.jacobian = 1 | ||
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network.rho_nse = 1.e7 | ||
network.T_nse = 3.e9 | ||
network.Si_nse = 0.02 | ||
network.C_nse = 1.0 | ||
network.O_nse = 1.0 | ||
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integrator.ode_max_steps = 500000 | ||
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network.small_x = 1.e-10 | ||
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network.nse_relax_factor = 0.9 | ||
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# use cubic interpolation from the NSE table | ||
network.nse_table_interp_linear = 0 | ||
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# disable jacobian caching in VODE | ||
integrator.use_jacobian_caching = 0 | ||
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# do we include weak rate neutrino losses in the energy? | ||
integrator.nse_include_enu_weak = 0 |