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 $T=120\mathrm{M}$.