diff options
author | jthorn <jthorn@f88db872-0e4f-0410-b76b-b9085cfa78c5> | 2005-05-11 12:00:30 +0000 |
---|---|---|
committer | jthorn <jthorn@f88db872-0e4f-0410-b76b-b9085cfa78c5> | 2005-05-11 12:00:30 +0000 |
commit | 132ef4236ecbfe0539ad46d48450f70846635c6f (patch) | |
tree | f55c99d4e089d71b654820ff17a72b041817bd79 /doc | |
parent | e0904c944cfa784ca76dfc222072668defef921d (diff) |
standardize terminology: $\Theta$ = expansion of trial surface
(a long time ago I used $H$, and I missed a few places when I switched)
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinAnalysis/AHFinderDirect/trunk@1408 f88db872-0e4f-0410-b76b-b9085cfa78c5
Diffstat (limited to 'doc')
-rw-r--r-- | doc/documentation.tex | 18 |
1 files changed, 9 insertions, 9 deletions
diff --git a/doc/documentation.tex b/doc/documentation.tex index 9bace6c..5c6551f 100644 --- a/doc/documentation.tex +++ b/doc/documentation.tex @@ -153,7 +153,7 @@ There may be several such surfaces, some nested inside others; an In terms of the usual $3+1$ variables, an apparent horizon satisfies the equation \begin{equation} -H \equiv \del_i n^i + K_\ij n^i n^j - K = 0 +\Theta \equiv \del_i n^i + K_\ij n^i n^j - K = 0 \label{AHFinderDirect/eqn-horizon} \end{equation} where $n^i$ is the outward-pointing unit normal to the apparent horizon, @@ -446,8 +446,8 @@ section~\ref{AHFinderDirect/sect-examples} should make this clear. \item[\code{"algorithm highlights"}] \mbox{}\\ Also print a single line for each Newton iteration giving - the 2-norm and $\infty$-norm of the $H(h)$ function defined - by equation~\eqref{AHFinderDirect/eqn-horizon}. + the 2-norm and $\infty$-norm of the $\Theta(h)$ function + defined by equation~\eqref{AHFinderDirect/eqn-horizon}. This is the default. \item[\code{"algorithm details"}] \mbox{}\\ @@ -1639,7 +1639,7 @@ improved convergence). Computationally, this algorithm has 3 main parts: \begin{itemize} -\item Computation of the ``horizon function'' $H(h)$ given a trial +\item Computation of the ``horizon function'' $\Theta(h)$ given a trial surface defined by a trial horizon shape function $h$. This is done by interpolating the Cactus geometry fields $g_\ij$ and $K_\ij$ (and optionally $\psi$) from the 3-D $xyz$ grid to the @@ -1647,8 +1647,8 @@ Computationally, this algorithm has 3 main parts: $\partial_k g_\ij$ in the interpolation process), then doing all further computations with angular grid functions defined solely on $S^2$ (\ie{} at the horizon-surface grid points). -\item Computation of the Jacobian matrix $\Jac[H(h)]$ of $H(h)$. This - thorn incorporates the \defn{symbolic differentiation} technique +\item Computation of the Jacobian matrix $\Jac[\Theta(h)]$ of $\Theta(h)$. + This thorn incorporates the \defn{symbolic differentiation} technique described in \cite{AEIThorns/AHFinderDirect/Thornburg-1996-apparent-horizon-finding}, so this computation is quite fast. The Jacobian is a highly @@ -1656,9 +1656,9 @@ Computationally, this algorithm has 3 main parts: as either a dense matrix (for debugging purposes), or a sparse matrix (the default). Which option is used is determined by a compile-time configuration in \verb|src/include/config.h|. -\item Solving the nonlinear equations $H(h) = 0$ by a global Newton's - method or a variant. How this is done depends on how the Jacobian - is stored. At present, +\item Solving the nonlinear equations $\Theta(h) = 0$ by a global + Newton's method or a variant. How this is done depends on how + the Jacobian is stored. At present, \begin{itemize} \item If \thorn{AHFinderDirect} is configured to store the Jacobian as a dense matrix, then LAPACK is used to solve |