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(DRAFT) feat: introduce 3-velocity grid variable to support relativistic transport #109
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Currently compute_dt runs every iteration. We may need to run compute_dt just once initially during production, since (rho,T,Ye) is static.
…density for mesh quantities
… antineutrino number densities
…tities to compute the correct time step
…rallel. This function will be used to compute the minimum trace of mesh quantities, and based on that, it will compute the optimum time step
…dary conditions and black holes.
… the minimum potential
…erse mean free paths in the grid center
…des a better representation of the time derivative of N than the previous 1/Opacity*c.
…and black holes in the function that computes the time step.
… it can be used when needed)
…ata generated by EMU
different to avoid repete code
…dat file that can be used as an initial condition for the Emu code.
…to make the process of writing data more efficient. Check points will not be permited for the output file.
…r cell optional. It run single boxes only if the input parameters are defined otherwise it splits particles in all cells
…mber bigger than 5 digits
… different from Fermi–Dirac. This will be useful for local simulations of CFI from NSM global cells, where the equilibrium is not necessarily Fermi–Dirac.
…al_instability_test
one that had the neutrino dir inside the plt file
…ir and just take the plt directories with data
…riables. MSW input test changed in order to initialize vup components as a parameter from the parameter class.
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implementation of 3-velocity to be stored in grid state multifab array. currently being read in through initial conditions file.