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authorhawke <hawke@a4c7b220-a359-4231-b37a-efab6cb7d3ee>2002-05-03 14:41:55 +0000
committerhawke <hawke@a4c7b220-a359-4231-b37a-efab6cb7d3ee>2002-05-03 14:41:55 +0000
commitbfd7ae0ce72db0b8c327a986ab50d8792d592ad7 (patch)
treee3d7241500ec8287b67475e490c4b053659d4c05
parent273fb8a893d785ed02dd15bd58ce07147d2af3a2 (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
-rw-r--r--README9
-rw-r--r--doc/auto/documentation.el13
-rw-r--r--doc/documentation.tex30
-rw-r--r--interface.ccl4
-rw-r--r--param.ccl2
-rw-r--r--schedule.ccl2
-rw-r--r--src/make.code.defn9
7 files changed, 69 insertions, 0 deletions
diff --git a/README b/README
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--- /dev/null
+++ b/README
@@ -0,0 +1,9 @@
+Cactus Code Thorn ADMCoupling
+Authors : Ian Hawke
+CVS info : $Header$
+--------------------------------------------------------------------------
+
+Purpose of the thorn:
+
+The "friend of a friend" thorn to help matter / spacetime coupling. Does nothing itself.
+
diff --git a/doc/auto/documentation.el b/doc/auto/documentation.el
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--- /dev/null
+++ b/doc/auto/documentation.el
@@ -0,0 +1,13 @@
+(TeX-add-style-hook "documentation"
+ (function
+ (lambda ()
+ (LaTeX-add-labels
+ "sec:aux")
+ (TeX-run-style-hooks
+ "latex2e"
+ "art10"
+ "article"
+ "interface"
+ "param"
+ "schedule"))))
+
diff --git a/doc/documentation.tex b/doc/documentation.tex
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+++ 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}
diff --git a/interface.ccl b/interface.ccl
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--- /dev/null
+++ b/interface.ccl
@@ -0,0 +1,4 @@
+# Interface definition for thorn ADMCoupling
+# $Header$
+
+implements: ADMCoupling \ No newline at end of file
diff --git a/param.ccl b/param.ccl
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index 0000000..b280418
--- /dev/null
+++ b/param.ccl
@@ -0,0 +1,2 @@
+# Parameter definitions for thorn ADMCoupling
+# $Header$
diff --git a/schedule.ccl b/schedule.ccl
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--- /dev/null
+++ b/schedule.ccl
@@ -0,0 +1,2 @@
+# Schedule definitions for thorn ADMCoupling
+# $Header$
diff --git a/src/make.code.defn b/src/make.code.defn
new file mode 100644
index 0000000..b345f84
--- /dev/null
+++ b/src/make.code.defn
@@ -0,0 +1,9 @@
+# Main make.code.defn file for thorn ADMCoupling
+# $Header$
+
+# Source files in this directory
+SRCS =
+
+# Subdirectories containing source files
+SUBDIRS =
+