Global parameters#
This block, called &RUN_PARAMS, contains the run global control
parameters. These parameters are now briefly described.
More thorough explanations will be given in dedicated sections of the wiki.
Variable name, syntax, default value |
Fortran type |
Description |
|---|---|---|
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Activate cosmological supercomoving cooordinates and computes the expansion factor |
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Activate Particle-In-Cell solver |
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Activate sink particles |
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Activate the clump finder |
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Use Monte Carlo tracer particles |
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Activate the particle unbinding for clumps |
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Make merger trees |
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Activate Poisson solver for self-gravity |
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Activate hydro or MHD solver. |
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Activate radiative transfer using CPU-based M1 solver. This solver works on the AMR grid. |
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Activate radiative transfer using GPU-based M1 solver. This solver works only on unigrid at |
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Activate verbose mode. |
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Load balancing based on computational cost, not memory. This is rather expensive in term of memory usage. For memory limited runs, using |
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Output file number from which the code loads backup data and resumes the simulation, The default value, zero, is for a fresh start from the beginning (time=0). |
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Restart with double precision Hilbert keys. Must be equal to |
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Maximum number of coarse time step. This can be used to terminate the simulation after a fixed amount of main steps. |
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Frequency of screen output for control lines (to stdout), usually redirected into a log file. |
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Frequency of call, in units of coarse time steps, for the load balancing routine, for MPI runs only. The default value, zero, means never. Load balancing is a slow operation, so use as high a value as possible. |
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Cell ordering method used in the domain decomposition of the grid, for MPI runs only. Possible values are |
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Number of fine level sub-cycling steps within one coarser level time step. Each value in the array corresponds to a given level of refinement, starting from the coarse grid at |
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Activate full static mode (RT post processing) |
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Activate static mode for DM particles only (isolated initial conditions relaxation) |
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Activate static mode for star particles only (isolated initial conditions relaxation) |
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Mapping for the passive scalars and non-thermal pressures. Value indicates in which variable the scalar from the restart should be loaded. [0 = ignore this scalar in the restart output, -N = do not read but initialise ivar=N to 0, N = read and initialise ivar=N from the restart output]. For example |