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author | hawke <hawke@a4c7b220-a359-4231-b37a-efab6cb7d3ee> | 2002-05-03 14:41:55 +0000 |
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committer | hawke <hawke@a4c7b220-a359-4231-b37a-efab6cb7d3ee> | 2002-05-03 14:41:55 +0000 |
commit | bfd7ae0ce72db0b8c327a986ab50d8792d592ad7 (patch) | |
tree | e3d7241500ec8287b67475e490c4b053659d4c05 /doc/documentation.tex | |
parent | 273fb8a893d785ed02dd15bd58ce07147d2af3a2 (diff) |
This commit was generated by cvs2svn to compensate for changes in r2, which
included commits to RCS files with non-trunk default branches.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinBase/ADMCoupling/trunk@3 a4c7b220-a359-4231-b37a-efab6cb7d3ee
Diffstat (limited to 'doc/documentation.tex')
-rw-r--r-- | doc/documentation.tex | 30 |
1 files changed, 30 insertions, 0 deletions
diff --git a/doc/documentation.tex b/doc/documentation.tex new file mode 100644 index 0000000..bc570bd --- /dev/null +++ b/doc/documentation.tex @@ -0,0 +1,30 @@ +\documentclass{article} + +\begin{document} + +\title{ADMCoupling} +\author{Ian Hawke} +\date{03/05/2002} +\maketitle + +\abstract{ADMCoupling} + +\section{Purpose} +\label{sec:aux} + +This thorn is completely trivial (there's already more words in the +documentation than in the code). The point is to allow clean coupling +of matter thorns and spacetime evolution thorns. By making a spacetime +thorn (such as BSSN) a friend of ADMCoupling it can know about the +variables of the matter thorns (such as Whisky) as long as they are +also friends of ADMCoupling, and then the appropriate stress energy +tensor terms can be included through the {\tt CalcTmunu} interface. +This avoids explicit dependencies between the spacetime and matter +evolution thorns. Note that we need to do the same for certain +analysis thorns, such as ADMConstraints. + +\include{interface} +\include{param} +\include{schedule} + +\end{document} |