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 <title>time independent Schr\"odinger equation in spherical coordinates</title>
 <name>TimeIndependentSchrodingerEquationInSphericalCoordinates</name>
 <created>2006-01-15 15:34:54</created>
 <modified>2006-10-30 21:50:45</modified>
 <type>Definition</type>
 <creator id="1" name="bloftin"/>
 <modifier id="390" name="invisiblerhino"/>
 <author id="1" name="bloftin"/>
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	<category scheme="msc" code="03.65.-w"/>
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	<object name="TimeIndependentSchrodingerEquation"/>
	<object name="RadialEquation"/>
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 <content>When writing the time independent Schr\"odinger equation in spherical coordinates, we need to 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 Schr\"odinger equation we then have


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

{\bf References}

[1] Griffiths, D. "Introduction to Quantum Mechanics" Prentice Hall, New Jersey, 1995.</content>
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