<?xml version="1.0" encoding="UTF-8"?>

<record version="4" id="100">
 <title>Laplacian in Spherical Coordinates</title>
 <name>LaplacianInSphericalCoordinates</name>
 <created>2005-12-30 20:39:07</created>
 <modified>2005-12-31 00:03:14</modified>
 <type>Definition</type>
 <creator id="1" name="bloftin"/>
 <modifier id="1" name="bloftin"/>
 <author id="1" name="bloftin"/>
 <classification>
	<category scheme="msc" code="02.40.Dr"/>
 </classification>
 <preamble>% this is the default PlanetMath preamble.  as your knowledge
% of TeX increases, you will probably want to edit this, but
% it should be fine as is for beginners.

% almost certainly you want these
\usepackage{amssymb}
\usepackage{amsmath}
\usepackage{amsfonts}

% used for TeXing text within eps files
%\usepackage{psfrag}
% need this for including graphics (\includegraphics)
\usepackage{graphicx}
% for neatly defining theorems and propositions
%\usepackage{amsthm}
% making logically defined graphics
%\usepackage{xypic}

% there are many more packages, add them here as you need them

% define commands here</preamble>
 <content>The Laplacian operator in spherical coordinates is 

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

The derivation is fairly straight forward and begins with locating a vector {\bf r} in spherical coordinates as shown in the figure.

\begin{figure}
\includegraphics[scale=.698]{SphericalCoordinates.eps}
\caption{Spherical Coordinates}
\end{figure}

The z component of the unit vector in direction of {\bf r} is given from the simple right triangle

$$ cos \theta = \frac{z}{| \hat{r} |} $$

Since a unit vector has a length of 1, the z component is

$$ z = cos \theta $$

To get the x component, we need to get the $\hat{r}$ projected onto the xy-plane

$$ cos( 90 - \theta) = \frac{ |\hat{r}_{xy}|}{ |\hat{r}| } $$

using the trig identity

$$ cos( 90 - \theta ) = sin \theta $$

so the projected unit vector is

$$ |\hat{r}_{xy}| = sin \theta $$

Finally, the x component is reached through the right triangle 

$$ cos \phi = \frac{x}{|\hat{r}_{xy}| }$$

giving 

$$ x = cos \phi \, sin \theta $$</content>
</record>
