First, write out
.
![\begin{eqnarray*}
L^2&=&(\vec{r}\times\vec{p})^2 \\
&=&-\hbar^2\left[
\left...
...over\partial y}-y{\partial\over\partial x}\right)^2 \right] \\
\end{eqnarray*}](img1758.png)
![\begin{eqnarray*}
L^2=&-&\hbar^2\left[
x^2\left({\partial^2\over\partial z^2}...
...er\partial y}
+2z{\partial\over\partial z}\right) \right] \\
\end{eqnarray*}](img1759.png)
We expect to need to keep the radial derivatives
so lets identify those by dotting
into
.
This will also make the units match
.

By adding these two expressions, things simplify a lot.
We can now solve for
and we have something we can use in the Schrödinger equation.

The Schrödinger equation now can be written with only radial derivatives and
.
Jim Branson 2013-04-22