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<record version="1" id="108">
 <title>time independent Schrödinger equation in spherical coordinates</title>
 <name>TimeIndependentSchrodingerEquationInSphericalCoordinates</name>
 <created>2006-01-15 15:34:54</created>
 <modified>2006-01-15 15:34:54</modified>
 <type>Definition</type>
 <creator id="1" name="bloftin"/>
 <modifier id="1" name="bloftin"/>
 <author id="1" name="bloftin"/>
 <classification>
	<category scheme="msc" code="03.65.-w"/>
 </classification>
 <related>
	<object name="TimeIndependentSchrodingerEquation"/>
 </related>
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 <content>When writing the time independent Schr\"odinger equation in spherical coordinates, we need plug the Laplacian in spherical coordinates into the time independent Schr\"odinger equation.  The Laplacian was found to be 

$$
\nabla _{sph}^{2} = \frac{1}{r^2} \frac{\partial}{\partial r}\left(r^2 \frac{\partial}{\partial r}\right) + \frac{1}{r^2 sin\theta} \frac{\partial}{\partial \theta} \left( sin \theta \frac{\partial}{\partial \theta}\right) + \frac{1}{r^2 sin^2 \theta} \frac{\partial^2}{\partial \phi^2}
$$

Using the three dimensional version of the S.E. we then have


$$ C \psi(r,\theta, \phi) = -\frac{\hbar^2}{2m} \left [ \frac{1}{r^2} \frac{\partial }{\partial r}\left(r^2 \frac{\partial \psi(r,\theta, \phi)}{\partial r}\right) \frac{1}{r^2 sin\theta} \frac{\partial}{\partial \theta} \left( sin \theta \frac{\partial \psi(r,\theta, \phi)}{\partial \theta}\right) + \frac{1}{r^2 sin^2 \theta} \frac{\partial^2 \psi(r,\theta, \phi)}{\partial \phi^2} \right ] + V(r,\theta, \phi) \psi(r,\theta, \phi)
$$</content>
</record>
