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authorallen <allen@b7a48df3-cbbf-4440-997f-b4b717c9f7fc>2002-04-07 17:07:20 +0000
committerallen <allen@b7a48df3-cbbf-4440-997f-b4b717c9f7fc>2002-04-07 17:07:20 +0000
commit74d53c943c0566408cc47e0375c2465942864fd3 (patch)
treedad3ca41f6f8cc7364c57807718afb8ee30568aa /doc
parent0104991f6c58e19f02bb65e07ce6d4eecf0f3889 (diff)
Some basic documentation for thorn ADMConstraints ... it would be great
if someone could take this and add a few words of wisdom on how to interpret the results ... git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinAnalysis/ADMConstraints/trunk@58 b7a48df3-cbbf-4440-997f-b4b717c9f7fc
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+\documentclass{article}
+\begin{document}
+
+\title{ADMConstraints}
+\author{Gabrielle Allen}
+\date{April 2002}
+\maketitle
+
+\abstract{Calculate the values of the Hamiltonian and Momentum Constraints on the computational grid for output.}
+
+\section{Physics}
+
+This analysis thorn calculates the values of the Hamiltonian and
+momentum constraint equations on the computational grid during a spacetime
+evolution. The Hamiltonian Constraint (grid function: ham) is given by
+
+\begin{equation}
+ H = R - K^{i}_{\;\;j} K^{j}_{\;\;i} + trK^2 - 16 \pi \rho
+\end{equation}
+
+The Momentum Constraints (grid functions momx, momy, momz) are given by
+
+\begin{equation}
+M_i = \nabla_j K_i^{\;\;j} - \nabla_i trK - 8 \pi S_i
+\end{equation}
+
+where
+
+\begin{equation}
+S_i = -g_{ia} n_b T^{ab} = - g_i^a n^b T_{ab} = -\frac{1}{\alpha} (T_{i0} - \beta^j T_{ij})
+\end{equation}
+
+\section{Comments}
+
+\begin{itemize}
+
+\item Symmetry boundary conditions ({\tt CactusBase/CartGrid3D}) are implemented.
+
+\item Default behaviour is to apply so called flat boundary conditions to the calculated values of the constraint equations.
+
+\item Excision ({\tt Excision/LegoExcision}) is included.
+
+\item The 3-metric is only included through the Macros in {\tt CactusEinstein/Einstein} and as such the physical metric is used.
+
+\item Matter is included using the {\tt CalcTmuNu} mechanism.
+
+\item The constraint calculation is default performed at the ANALYSIS time bin, if the constraint values are needed at every iteration, the parameter {\tt constraints\_persist} should be used to schedule the calculation instead at POSTSTEP.
+
+\end{itemize}
+
+% Automatically created from the ccl files by using gmake thorndoc
+\include{interface}
+\include{param}
+\include{schedule}
+
+\end{document}