The Classical Schrodinger's Equation
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A non perturbative numerical method for determining the discrete spectra is deduced from the classical analogue of the Schrodinger's equation. The energy eigenvalues coincide with the bifurcation parameters for the classical orbits.
UUEncoded Postscript, 18 pages, 4 figures inserted in text
UUEncoded Postscript, 18 pages, 4 figures inserted in text