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Devlin:
<math>let \xi = \sqr [(mx\omega}/\hbar)] </math> and <math> K=(2E)/(\hbar\omega). </math>
Then we can use the dimensionless form of the Schrodinger <math> \frac{\partial^2}{\partial x^2}=(\xi^2-K)\psi(x) </math>
We can think of <math> \xi </math> as approximately <math> x </math> and also <math> \psi </math> as approximately <math> e^-(\xi)^2/2) </math>.
<math> \psi\approx h(\xi)e^(-\xi^2/2) </math>
We use this and hope that <math> h(\xi) </math> is simpler than <math> \psi(\xi) </math>
<math> \frac{\partial^2}{\partial x^2}=(\xi^2-K)\psi(x). </math>
Differentiate and then Schrodinger's equation becomes
<math> \frac{\partial^2h(\xi)}{\partial \xi^2}=-2h\xi(\xi)+(K-1)(h(\xi)=0 </math> (A)
Assume the solution can be found in the form <math> h(\xi)=\sum a_j \xi^j. </math>.
Differentiate each term: <math> \frac{\partial h}{partial\xi}=\sum a_j\xi^j </math>
Differentiate once more:
<math> \frac{\partial^2h}{partial\xi^2}=\sum (j+1)(j+2)a_j+2\xi^j </math>
Plug equation into (A) and we get a recursive equation that can be illustrated like this:
<math> (blah)(\xi)^0+ (blahblah)(\xi)^1 +(moreblah)(\xi)^2+…=0. </math>
Since the equation needs to hold true for all <math> \xi </math>, the 'blahs' must equal zero. We now have this equation
<math> a_j+2 = (2j+1-K)a_j/[(j+1)(j+2)] </math>
Now all we need to know is a_0 and a_1 and we can find all a.
This is good, but not all the solutions that are found are normalizable. For example, at very large j, the formula is <math> a_j+2 \approx 2a_j/j.
Then the solution is <math> a_j\approx \frac{C}{(j/2)!}. </math> Which makes <math> h(\xi)\approx Ce^\xi^2. </math>
The solution blows up. To get normalizable solutions, we need the power series to terminate. To do this, we need the numerator to go to zero. That is <math> 2j+1-K=0, </math> so <math>K=2j+1.</math>
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