[Commits] [svn:einsteintoolkit] Paper_EinsteinToolkit_2010/ (Rev. 151)
knarf at cct.lsu.edu
knarf at cct.lsu.edu
Mon Oct 17 00:27:25 CDT 2011
User: knarf
Date: 2011/10/17 12:27 AM
Modified:
/
ET.tex, plot_defaults.py
Log:
include new plots in paper
File Changes:
Directory: /
============
File [modified]: ET.tex
Delta lines: +6 -3
===================================================================
--- ET.tex 2011-10-17 05:21:57 UTC (rev 150)
+++ ET.tex 2011-10-17 05:27:24 UTC (rev 151)
@@ -2709,19 +2709,22 @@
than second order, but higher than first order.
\begin{figure}
\label{fig:tov_collapse_rho_central}
- \includegraphics{examples/collapse/tov_collapse_rho_central}
+ %\includegraphics{examples/collapse/tov_collapse_rho_central}
+ \includegraphics[width=0.9\textwidth]{examples/collapse/rho_max}
\caption{Evolution of the central density for the collapsing TOV star.}
\end{figure}
\begin{figure}
\label{fig:tov_collapse_radii}
- \includegraphics{examples/collapse/tov_collapse_radii}
+ %\includegraphics{examples/collapse/tov_collapse_radii}
+ \includegraphics[width=0.9\textwidth]{examples/collapse/radii}
\caption{Location on x axis where $\rho = 100\,\mathtt{whisky\_rho\_min}$ and
the areal radius of the apparent horizon ($R_g = 2\,M_\star =
2\,1.63\,M_{\mathord\odot}$).}
\end{figure}
\begin{figure}
\label{fig:tov_collapse_rho_maximum_convergence}
- \includegraphics{examples/collapse/rho_maximum_convergence}
+ %\includegraphics{examples/collapse/rho_maximum_convergence}
+ \includegraphics[width=0.9\textwidth]{examples/collapse/rho_max_conv}
\caption{Convergence factor (based on three runs) for the central density.}
\end{figure}
In Figure~\ref{fig:tov_collapse_radii} we plot on the same graph the
File [modified]: plot_defaults.py
Delta lines: +5 -5
===================================================================
--- plot_defaults.py 2011-10-17 05:21:57 UTC (rev 150)
+++ plot_defaults.py 2011-10-17 05:27:24 UTC (rev 151)
@@ -33,11 +33,11 @@
ax.xaxis.LABELPAD=10.
ax.xaxis.OFFSETTEXTPAD=10.
-# constants
-G = 6.673e-11
-c = 299792458
-M_sol = 1.98892e30
+# constants, in SI
+G = 6.673e-11 # m^3/(kg s^2)
+c = 299792458 # m/s
+M_sol = 1.98892e30 # kg
# convertion factors
M_to_ms = 1./(1000*M_sol*G/(c*c*c))
# fix this - what is 7e10?
-M_to_rho_g_cm3 = M_sol*1000/7e10/7e10/7e10
+M_to_density = c*c*c*c*c*c / (G*G*G * M_sol*M_sol) # kg/m^3
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