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| | [No title] (Site not responding. Last check: 2007-10-09) |
 | | The eigenfunctions obtained in these coordinate systems are each a suitable basis set in the absence of an electric field, but only the parabolic states, the Stark eigenfunctions, retain their character in the presence of a weak field. |
 | | The principal quantum number n and the magnetic quantum number m that are ``good" in spherical coordinates are common to both solutions; k is, however, unique to the parabolic coordinate solution. |
 | | Upon application of the field F, the parabolic quantum numbers are still good but the energy is now given by \begin{equation} E(n,\ k)\ =\ -\,\,{\frac{1}{2\,{n}^{2}}}\ -\ {\frac{3}{2}}\,n\,k\,F\ \end{equation} We note that, customarily, the opposite sign convention has been used for the electric quantum number k in equations (1) and (2). |
| newton.umsl.edu /~atomic/ajp4/ajp4.tex.txt (3063 words) |
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