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author | allen <allen@a678b1cf-93e1-4b43-a69d-d43939e66649> | 1999-09-25 10:34:45 +0000 |
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committer | allen <allen@a678b1cf-93e1-4b43-a69d-d43939e66649> | 1999-09-25 10:34:45 +0000 |
commit | 8448c19709c000e089723e276c871563f278b2dd (patch) | |
tree | 9ad226574a910f24367351a24226afb99937a9b8 /doc | |
parent | 46976958af59db7a29d02472721dc2d281181e34 (diff) |
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/IDBrillData/trunk@3 a678b1cf-93e1-4b43-a69d-d43939e66649
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-rw-r--r-- | doc/documentation.tex | 142 |
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diff --git a/doc/documentation.tex b/doc/documentation.tex new file mode 100644 index 0000000..59a7721 --- /dev/null +++ b/doc/documentation.tex @@ -0,0 +1,142 @@ +% Thorn documentation template +\documentclass{article} +\begin{document} + +\title{IDBrillData} +\author{Carsten Gundlach} +\date{6 September 1999} +\maketitle + +\abstract{This thorn creates initial data for Brill wave spacetimes. +It can create both axisymmetric data (in a 3D cartesian grid), as +well as data with an angular dependency.} + +\section{Purpose} + +The purpose of this thorn is to create initial data for a Brill wave +spacetime. It does so by starting from a three--metric of the form +originally considered by Brill +\begin{equation} +ds^2 = \Psi^4 \left[ e^{2q} \left( d\rho^2 + dz^2 \right) ++ \rho^2 d\phi^2 \right] =\Psi^4 \hat{ds}^{2}, +\label{eqn:brillmetric} +\end{equation} +where $q$ is a free function subject to certain regularity and +fall-off conditions and $Psi$ is a conformal factor to be solved for. + +The thorn considers several different forms of the function $q$ +depending on certain parameters that will be described below. +Substituting the metric above into the Hamiltonian constraint results +in an elliptic equation for the conformal factor $Psi$ that can be +solved numerically once the function $q$ has been specified. The +initial data is also assumed to be time-symmetric, so the momentum +constraints are trivially satisfied. + +The thorn is activated by choosing the standard Cactus parameter +``initial\_data'' in one of the following two ways: + +\begin{itemize} + +\item initial\_data = ``brilldata'': Axisymmetric Brill wave initial data + (but calculated in a cartesian grid!). + +\item initial\_data = ``brilldata3D'': Brill wave initial data with an + angular dependency. + +\end{itemize} + + +\section{Parameters for the thorn} + +The thorn is controlled by the following parameters: + +\begin{itemize} + +\item brill\_q (INT): Form of the function $q$ [0,1,2] (default 2): + +\begin{itemize} + +\item brill\_q = 0: +\[ +q = a \; \frac{\rho^{2+b}}{r^2} \left( \frac{z}{\sigma_z} \right)^2 +e^{-(\rho - \rho_0^2)} +\] + +\item brill\_q = 1: +\[ +q = a \left( \frac{\rho}{\sigma_\rho} \right)^b \frac{1}{1 + \left[ +\left( r^2 - r_0^2 \right) / \sigma_r^2 \right]^{c/2}} +\] + +\item brill\_q = 2: +\[ +q = a \left( \frac{\rho}{\sigma_\rho} \right)^b e^{-\left[ +\left( r^2 - r_0^2 \right) / \sigma_r^2 \right]^{c/2}} +\] + +\item If one specifies 3D data (see above), the function $q$ is multiplied +by an additional factor with an angular dependency: +\[ +q \rightarrow q \left[ 1 + d \frac{\rho^m}{1 + e \rho^m} +\cos^2 \left( n \phi + \phi_0 \right) \right] +\] + +\end{itemize} + +\item brill\_a (REAL): Amplitude (default 0.0). + +\item brill\_b (REAL): $b$ in above expressions (default 2.0). + +\item brill\_c (REAL): $c$ in above expressions (default 2.0). + +\item brill\_d (REAL): $d$ in above expressions (default 0.0). + +\item brill\_e (REAL): $e$ in above expressions (default 1.0). + +\item brill\_m (REAL): $m$ in above expressions (default 2.0). + +\item brill\_n (REAL): $n$ in above expressions (default 2.0). + +\item brill\_r0 (REAL): $r_0$ in above expressions (default 0.0). + +\item brill\_rho0 (REAL): $\rho_0$ in above expressions + (default 0.0). + +\item brill\_phi0 (REAL): $\phi_0$ in above expressions + (default 0.0). + +\item brill\_sr (REAL): $\sigma_r$ in above expressions + (default 1.0). + +\item brill\_srho (REAL): $\sigma_\rho$ in above + expressions (default 1.0). + +\item savepsi (KEYWORD): Save conformal factor for output? + [``yes'',''no''] Normally, the conformal factor is calculated in the + grid function ``psi'', but this is set back to 1 at the end once the + physical metric has been constructed. Setting this parameter to + ``yes'' copies the conformal factor to the grid function + ``brillpsi0'' before resetting it to 1 (default ``no''). + +\end{itemize} + +The elliptic solver is controlled by additional the parameters: + +\begin{itemize} + +\item solver (KEYWORD): Elliptic solver used to solve the + hamiltonian constraint [sor/petsc/bam] (default ``sor''). + +\item thresh (REAL): Threshold for elliptic solver (default + 0.00001). + +\end{itemize} + +% Automatically created from the ccl files +% Do not worry for now. + +\include{interface} +\include{param} +\include{schedule} + +\end{document} |