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authorschnetter <schnetter@f4913095-0e4f-0410-abea-a123d184f1f3>2005-03-17 19:04:54 +0000
committerschnetter <schnetter@f4913095-0e4f-0410-abea-a123d184f1f3>2005-03-17 19:04:54 +0000
commit749d52043c6199aa21bb24975c355b59eb9cd76b (patch)
tree0aa662185aec1f1ec75c0d912faa99c7f4153a5d
parent417e1eaf9555ed5fca925271f30010d340aea878 (diff)
More explanation.
git-svn-id: http://svn.cactuscode.org/arrangements/CactusNumerical/Norms/trunk@4 f4913095-0e4f-0410-abea-a123d184f1f3
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@@ -11,10 +11,16 @@ Purpose of the thorn:
Compute norms of the state vector, e.g. for Mexico tests. These are
special norms that make a difference between variables which have a
-second derivative taken and variables which have not; see gr-qc
-0503056.
+second derivative taken and variables which have not; see
+gr-qc/0503056. These norms include the gradients of those variables
+that have a second derivative taken. In doing so, they take all
+wavelenghts into account -- in contrast, a norm that would be based
+simply on using centered differences to calculate gradients would not.
-gr-qc 0503056: Calabrese, Hinder, Husa: Numerical stability for finite
-difference approximations of Einstein's equations
+References:
+
+Gioel Calabrese, Ian Hinder, Sascha Husa: Numerical stability for
+finite difference approximations of Einstein's equations,
+gr-qc/0503056 (2005)