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

<record version="2" id="212">
 <title>gradient</title>
 <name>Gradient</name>
 <created>2006-07-25 20:30:50</created>
 <modified>2006-07-25 21:02:21</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."/>
 </classification>
 <synonyms>
	<synonym concept="gradient" alias="gradient operator"/>
 </synonyms>
 <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 gradient is the vector sum of the resultant rate of increase of a scalar funcion $V$ and is denoted $\nabla V$.  It represents a directed rate of change of $V$.  A directed derivative or vector derivative of $V$, so to speak.  In cartesian coordinates

\begin{equation}
\nabla V = \frac{ \partial V}{\partial x} {\bf \hat{i}} + \frac{ \partial V}{\partial y} {\bf \hat{j}} + \frac{ \partial V}{\partial z} {\bf \hat{k}}  
\end{equation}

It is common to regard $\nabla$ as the gradient operator which obtains a vector $\nabla V$ from a scalar function $V$ of position in space.

$$ \nabla V = \left ( \frac{ \partial }{\partial x} {\bf \hat{i}} + \frac{ \partial }{\partial y} {\bf \hat{j}} + \frac{ \partial }{\partial z} {\bf \hat{ik}} \right ) V $$

Thus it is easy to work with just the gradient operator

\begin{equation}
\nabla V = \frac{ \partial }{\partial x} {\bf \hat{i}} + \frac{ \partial }{\partial y} {\bf \hat{j}} + \frac{ \partial }{\partial z} {\bf \hat{k}}  
\end{equation}

This symbolic operator $\nabla$ was introduced by Sir W. R. Hamilton.  It has been found by experience that the monosyllable \emph{del} is so short and easy to pronounce that even in complicated formulas in which $\nabla$ occurs a number of times no inconvenience to the speaker or hearer arises from the repetition.  $\nabla V$ is read simply as "del $V$."

\subsection{Coordinate System Independence}

Although this operator $\nabla$ has been defined as 

$$\nabla V = \frac{ \partial }{\partial x} {\bf \hat{i}} + \frac{ \partial }{\partial y} {\bf \hat{j}} + \frac{ \partial }{\partial z} {\bf \hat{k}} $$

so that it appears to depend upon the choice of the axes, it is in reality independent of them.  This would be surmised from the interpretation of $\nabla$ as the magnitude and direction of the most rapid increase of $V$.  To demonstrate the independence take another set of axes, ${\bf \hat{i}'}$, ${\bf \hat{j}'}$, ${\bf \hat{k}'}$ and a new set of variables $x'$, $y'$, $z'$ referred to them.  Then $\nabla$ referred to this system is 

$$\nabla' = \frac{ \partial }{\partial x'} {\bf \hat{i'}} + \frac{ \partial }{\partial y'} {\bf \hat{j'}} + \frac{ \partial }{\partial z'} {\bf \hat{k'}} $$


(Please Insert PROOF here...)


Leaving behind the proof of coordinate system independence, here is the gradient opertor in the most common coordinate systems.

Cartesian Coordinates

\begin{equation}
\nabla V = \frac{ \partial V}{\partial x} {\bf \hat{i}} + \frac{ \partial V}{\partial y} {\bf \hat{j}} + \frac{ \partial V}{\partial z} {\bf \hat{k}}  
\end{equation}

Cylindrical Coordinates

\begin{equation}
\nabla V = \frac{ \partial V}{\partial r} {\bf \hat{r}} + \frac{1}{r}\frac{ \partial V}{\partial \theta} {\bf \hat{\theta}} + \frac{ \partial V}{\partial z} {\bf \hat{z}}  
\end{equation}                                  

Spherical Coordinates

\begin{equation}
\nabla V = \frac{ \partial V}{\partial r} {\bf \hat{r}} + \frac{1}{r}\frac{ \partial V}{\partial \phi} {\bf \hat{\phi}} + \frac{1}{r \sin \phi}\frac{ \partial V}{\partial \theta} {\bf \hat{\theta}}  
\end{equation}</content>
</record>
