Ricardo #3
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Ricardo #3
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Now takes accretion rate in terms of Eddington's. I just change the source code, it's not compiled.
Runs grmonty many times, creates a list of points that represent the grid in (logM, logMdot, theta, logNu) and another list with the corresponding values of logNuLnu. The script saves two separate files: "points" and "values" for the lists.
To see an interpolation: 1. Run iterate.py to create the support points. 2. Run interpolate.py on the desired point. compare.py does the same as interpolate.py but compares the result with an independent grmonty run. Plots both and shows the relative error. convergence.py computes the L1 norm for a point (M, Mdot, theta) over an array of photon numbers. convergence2.py does the same but compares each photon number with another run with same photon number.
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grmonty(N, dump,Mdot/MdotEdd,M/Msun,Tp/Te)