Toolkit for creating plots and computing stable equipotential surfaces of fluids orbiting a compact stellar object (see Zarotti: Relativistic Hydrodynamics))
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Inverse effective potential for Erez-Rosen metric #4
There is, as far as I know, no analytical way to compute the inverse effective potential, or polar dependency, so to speak.
Thus, this issue is discarded, to solve for someone smarter than current me.
For the next feature, implement the inverse effective potential for the Q metric Also, give theoretical analysis in BoyerLindquist coordinates