[Commits] [svn:einsteintoolkit] Paper_EinsteinToolkit_2010/ (Rev. 294)

[bcmsma at astro.rit.edu]

User: bmundim
Date: 2012/03/12 03:37 PM

Modified:
 /
  ET.tex

Log:
 link to sec. 5.6.3

File Changes:

Directory: /
============

File [modified]: ET.tex
Delta lines: +3 -1
===================================================================
--- ET.tex	2012-03-12 20:31:14 UTC (rev 293)
+++ ET.tex	2012-03-12 20:37:30 UTC (rev 294)
@@ -2077,6 +2077,7 @@
 matter field.
 
 \subsubsection{Gravitational Waves} 
+\label{sec:gw}
 One of the main goals of numerical relativity to date is 
 modeling  gravitational waveforms that may 
 be used in template generation to help analyze 
@@ -2686,7 +2687,8 @@
 calculated by the \codename{QuasiLocalMeasures} module, 
 and were found to be $0.884 \mathrm{M}$ and $0.625 \mathrm{M}^{2}$, respectively.
 
-Two modules are necessary to perform the waveform extraction.
+Two modules are necessary to perform the waveform extraction
+(see Sec.~\ref{sec:gw} for details).
 The first one, \codename{WeylScal4}, calculates the Weyl scalar
 $\Psi_4$ in term of the metric components and its derivatives;
 these were computed to be $4$-th order accurate in this example.