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