WKB in Spherical Coordinates: Difference between revisions
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where | where | ||
<math>T=\frac{\hbar^2(l+\tfrac{1}{2})^2}{2mE} | <math>T=\frac{\hbar^2(l+\tfrac{1}{2})^2}{2mE},\,V=-\frac{e^2}{E},</math> | ||
and the integral, | and <math>r_1\!</math> and <math>r_2\!</math> are the classical turning points of the (effective) potential appearing in the WKB approximation for this problem, and the integral, | ||
<math>\int_{r_1}^{r_2}\sqrt{{\frac{(x-a)(x-b)}{x^{2}}}}\,dx=\frac{\pi }{2}(\sqrt {b} -\sqrt {a} )^{2} </math> | <math>\int_{r_1}^{r_2}\sqrt{{\frac{(x-a)(x-b)}{x^{2}}}}\,dx=\frac{\pi }{2}(\sqrt {b} -\sqrt {a} )^{2}.</math> | ||
[[Phy5645/WKBenergyspectrum|Solution]] | [[Phy5645/WKBenergyspectrum|Solution]] |
Revision as of 02:30, 13 January 2014
It is possible to apply the WKB approximation to the radial equation using a method by R. E. Langer (1937).
Recall that
and that satisfies the effective one-dimensional Schrödinger equation,
We now perform the following transformations:
Note that, for The radial equation becomes
In this case the Bohr-Sommerfeld quantization rule becomes:
Problems
(1) Use the WKB approximation to estimate energy spectrum for a Hydrogen atom.
Hint:
Use the relation,
where
and and are the classical turning points of the (effective) potential appearing in the WKB approximation for this problem, and the integral,