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add subchandra subch_base input files (#2657)
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input files for subch_base. Used for NSE_NET runs.
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zhichen3 authored Mar 13, 2024
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148 changes: 148 additions & 0 deletions Exec/science/subchandra/inputs_2d.NSE
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# ------------------ INPUTS TO MAIN PROGRAM -------------------
amr.plot_files_output = 1
amr.checkpoint_files_output = 1

max_step = 1000000
stop_time = 10.0

geometry.is_periodic = 0 0
geometry.coord_sys = 1 # r-z coordinates

geometry.prob_lo = 0. 0.
geometry.prob_hi = 5.12e9 1.024e10

amr.n_cell = 1280 2560

amr.max_level = 1 # maximum level number allowed

castro.lo_bc = 3 2
castro.hi_bc = 2 2

# >>>>>>>>>>>>> BC FLAGS <<<<<<<<<<<<<<<<
# 0 = Interior 3 = Symmetry
# 1 = Inflow 4 = SlipWall
# 2 = Outflow 5 = NoSlipWall
# >>>>>>>>>>>>> BC FLAGS <<<<<<<<<<<<<<<<

castro.do_hydro = 1
castro.do_grav = 1
castro.do_react = 1
castro.do_sponge = 1

castro.react_rho_min = 1.0
castro.react_T_min = 5.e7

castro.ppm_type = 1
castro.ppm_temp_fix = 0

castro.use_flattening = 1

castro.riemann_solver = 1

# Full self-gravity with the Poisson equation
gravity.gravity_type = PoissonGrav

# Multipole expansion includes terms up to r**(-max_multipole_order)
gravity.max_multipole_order = 6

# Tolerance for multigrid solver for phi solves
gravity.abs_tol = 1.e-10

# Use sync solve for gravity after refluxing
#gravity.no_sync = 0

# Disable the use of the lagged composite correction for the potential
gravity.do_composite_phi_correction = 0

castro.sponge_upper_density = 1.e4
castro.sponge_lower_density = 1.e2
castro.sponge_timescale = 1.e-3

castro.cfl = 0.2 # cfl number for hyperbolic system
castro.init_shrink = 0.05 # scale back initial timestep by this factor
castro.change_max = 1.025 # factor by which dt is allowed to change each timestep
castro.sum_interval = 0 # timesteps between computing and printing volume averages
castro.update_sources_after_reflux = 0
castro.time_integration_method = 3

castro.use_retry = 1
castro.retry_subcycle_factor = 0.5
castro.max_subcycles = 32

castro.abundance_failure_rho_cutoff = 1.0

#castro.dtnuc_e = 0.25
#castro.dtnuc_X = 0.25

amr.ref_ratio = 2 2 2 2 # refinement ratio
amr.regrid_int = 2 # how often to regrid
amr.n_error_buf = 2 2 2 2 # number of buffer cells in error est
amr.grid_eff = 0.7 # what constitutes an efficient grid

amr.check_file = subch_chk # root name of checkpoint file
amr.check_int = 50 # number of timesteps between checkpoints
amr.plot_file = subch_plt # root name of plot file
amr.plot_int = -1 # number of timesteps between plotfiles
amr.plot_per = 2.e-3

amr.max_grid_size = 256 # maximum grid size allowed -- used to control parallelism
amr.blocking_factor = 32 # block factor in grid generation

amr.v = 1 # control verbosity in Amr.cpp
castro.v = 1 # control verbosity in Castro.cpp

amr.derive_plot_vars = ALL
castro.store_burn_weights = 1

castro.small_dens = 1.e-5
castro.small_temp = 1.e5

# problem parameters

problem.model_name = "sub_chandra.M_WD-1.10.M_He-0.050.hse.CO.10.00km"

problem.pert_temp_factor = 20.0
problem.pert_rad_factor = 0.5
problem.R_pert = 1.e7

problem.mu_p = -5.0
problem.mu_n = -12.0

# tagging

amr.refinement_indicators = tempgrad denerr temperr

amr.refine.tempgrad.relative_gradient = 2.0
amr.refine.tempgrad.field_name = Temp
amr.refine.tempgrad.max_level = 1

amr.refine.denerr.value_greater = 1.0
amr.refine.denerr.field_name = density
amr.refine.denerr.max_level = 1

amr.refine.temperr.value_greater = 1.e8
amr.refine.temperr.field_name = Temp
amr.refine.temperr.max_level = 3

# Microphysics

network.small_x = 1.e-10
integrator.SMALL_X_SAFE = 1.e-10

integrator.rtol_spec = 1.e-5
integrator.atol_spec = 1.e-5
integrator.rtol_enuc = 1.e-5
integrator.atol_enuc = 1.e-8
integrator.jacobian = 1

integrator.X_reject_buffer = 4.0

# disable jacobian caching in VODE
integrator.use_jacobian_caching = 0

integrator.ode_max_steps = 500000

nse.nse_dx_independent = 1
nse.nse_molar_independent = 0
nse.ase_tol = 0.1
nse.nse_skip_molar = 0
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