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<record version="2" id="820">
 <title>relativistic total energy</title>
 <name>RelativisticTotalEnergy</name>
 <created>2009-08-11 23:41:35</created>
 <modified>2009-09-06 02:29:13</modified>
 <type>Definition</type>
 <creator id="1" name="bloftin"/>
 <modifier id="441" name="bci1"/>
 <author id="441" name="bci1"/>
 <author id="1" name="bloftin"/>
 <classification>
	<category scheme="msc" code="03.30.+p"/>
 </classification>
 <defines>
	<concept>relativistic total energy</concept>
	<concept>energy-mass equivalence</concept>
 </defines>
 <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 relativistic total energy E of a particle is defined as 

\begin{equation}
E = \frac{mc^2}{\sqrt{1-v^2/c^2}}
\end{equation}

One often finds this relationship in the limit of low speeds $(v &lt;&lt; c)$ with the famous equation

\begin{equation}
E_0 = mc^2
\end{equation}</content>
</record>
