[Commits] [svn:einsteintoolkit] Paper_EinsteinToolkit_2010/ (Rev. 254)

[diener at cct.lsu.edu]

User: diener
Date: 2012/03/05 12:40 PM

Modified:
 /
  ET.tex

Log:
 Cite Brandt:1996si when discussing Bowen-York initial data for a
 distorted spinning black hole.

File Changes:

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

File [modified]: ET.tex
Delta lines: +2 -2
===================================================================
--- ET.tex	2012-03-01 05:39:01 UTC (rev 253)
+++ ET.tex	2012-03-05 18:40:12 UTC (rev 254)
@@ -28,7 +28,7 @@
 \usepackage[all]{hypcap}
 
 \usepackage[sort&compress,numbers]{natbib}
-\renewcommand{\bibfont}{\footnotesize}
+%\renewcommand{\bibfont}{\footnotesize}
 
 \graphicspath{{figures/}
 {cactus-benchmarks/}
@@ -2241,7 +2241,7 @@
 resolution on the finest (coarsest) grid. The runs were performed using the tapering
 evolution scheme in \codename{Carpet} to avoid interpolation in
 time during prolongation. The initial data correspond to a rotating, stationary Kerr BH
-perturbed by a Brill wave and, as such, has a non-zero
+perturbed by a Brill wave\cite{Brandt:1996si} and, as such, has a non-zero
 gravitational wave content. We evolved the BH using 4th-order finite differencing from
 $T=0\mathrm{M}$ until it had settled down to a stationary state at $T=120\mathrm{M}$.