% If you are using CVS use this line to give version information % $Header$ \documentclass{article} % Use the Cactus ThornGuide style file % (Automatically used from Cactus distribution, if you have a % thorn without the Cactus Flesh download this from the Cactus % homepage at www.cactuscode.org) \usepackage{../../../../doc/latex/cactus} \begin{document} \title{IDScalarWave} \author{Gabrielle Allen \\ Horst Beyer} \date{$ $Date$ $} \maketitle % Do not delete next line % START CACTUS THORNGUIDE \begin{abstract} Initial Data for the 3D Scalar Wave Equation \end{abstract} \section{Purpose} This thorn provides different initial data for the 3D scalar wave equation. \section{Spherically Symmetric Solutions} The general spherically symmetric solution can be written \begin{equation} \Psi(r,t) = \frac{1}{r}\left(f(r+t)+g(r-t)\right) \end{equation} where the functions $f$ and $g$ can be freely chosen. Making the additional requirement of time symmetry at $t=0$, forces \begin{equation} f(r)=g(r) \end{equation} Thus if the solution at t=0 is given by $\phi(r)$, the general solution will be \begin{equation} \Psi(r,t) = \frac{1}{2r}\left( (r+t)\phi(r+t)+(r-t)\phi(r-t) \right) \end{equation} \section{Gaussian} The gaussian solution is {\it spherically symmetric} about the origin of the Cartesian coordinate system, and is {\it time symmetric}. The initial profile is \begin{equation} \phi(r) = A \exp (- r^2/\sigma) \end{equation} with the solution at the origin being \begin{equation} \Psi(r=0,t) = \left(1-2\frac{t^2}{\sigma}\right)\exp(-t^2/\sigma) \end{equation} The Gaussian solution is set with the parameters \begin{itemize} \item {\tt amplitude} = $A$ \item {\tt sigma} = $\sigma$ \end{itemize} % Do not delete next line % END CACTUS THORNGUIDE \end{document}