[Commits] [svn:einsteintoolkit] Paper_EinsteinToolkit_2010/ (Rev. 269)

[bcmsma at astro.rit.edu]

User: bmundim
Date: 2012/03/07 03:14 PM

Modified:
 /
  ET.tex

Log:
 Fixes related to the ID table.

File Changes:

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

File [modified]: ET.tex
Delta lines: +6 -5
===================================================================
--- ET.tex	2012-03-07 18:11:55 UTC (rev 268)
+++ ET.tex	2012-03-07 21:14:00 UTC (rev 269)
@@ -1023,7 +1023,7 @@
 {\tt Lorene} is often used to generate initial data involving neutron stars,
 where the initial data problem is sufficiently hard that finding a numerical
 solution requires a significant amount of computer time as well as some human
-vversight in order to guide the routine to the correct solution. 
+oversight in order to guide the routine to the correct solution. 
 Therefore, recommended practice is to let Lorene output 
 data into files, and then read those into the Einstein Toolkit at the beginning of a run.
 
@@ -2478,10 +2478,11 @@
 \hline
 QC3 & 3.0 & -3.0 & 0.0 & 0.13808 & 0.47656 &  0.984618  \\
 \end{tabular}\\}
-\caption{Initial data parameters for a non-spinning equal mass 
-BH binary. The punctures are located on the
-$x$-axis at positions $x_1$ and $x_2$, with puncture bare 
-mass parameters $m_1 = m_2 = m$, and momenta $\pm\vec p$.
+\caption{Initial data parameters and initial ADM mass
+for a non-spinning equal mass BH binary system. The punctures are located 
+on the $x$-axis at positions $x_1$ and $x_2$, with puncture bare 
+mass parameters $m_1 = m_2 = m$, and momenta %$\pm\vec p$.
+$\vec p_1 = -\vec p_2 = \vec p$.
 }
 \end{table}