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\input{mystyle_beamer.tex}
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\usetikzlibrary{arrows.meta}
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\usetikzlibrary{decorations.pathmorphing}
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\tikzset{zigzag/.style={decorate, decoration=zigzag}}
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\def \L {2.}
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\title{Towards Moving Picture Simulations in a Discontinuous Galerkin Framework}
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\author{Yingjie Wang}
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\institute{FAU}
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\addbibresource{ref.bib}
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\begin{document}
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\maketitle
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@@ -40,8 +49,83 @@
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\end{itemize}
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\end{frame}
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\begin{frame}{Methods on evolving black holes}
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\subsection{Methods on evolving black holes}
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There are two main methods to evolve black holes in numerical relativity:
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\begin{itemize}
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\item Excision method: excise the black hole interior from the computational domain, and impose boundary conditions on the excision surface
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\item Moving puncture method: evolve the black hole as a puncture, and use a suitable gauge condition to avoid the singularity.
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\end{itemize}
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\end{frame}
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\begin{frame}{Methods on evolving black holes: excision}
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\begin{figure}
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\centering
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\includegraphics[width=0.7\textwidth]{imgs/black_hole_excision_mesh.png}
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\caption{An example mesh using excision method from \cite{Hemberger_2013}.}
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\end{figure}
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\end{frame}
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\begin{frame}{Methods on evolving black holes}
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\begin{tikzpicture}[>=Latex, line cap=round, line join=round]
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% causal diamond
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\draw[thick,red,zigzag] (-\L,\L) coordinate(stl) -- (\L,\L) coordinate (str);
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\draw[thick,black] (\L,-\L) coordinate (sbr)
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-- (0,0) coordinate (bif) -- (stl);
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\draw[thick,black,fill=blue, fill opacity=0.2,text opacity=1]
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(bif) -- (str) -- (2*\L,0) node[right] (io) {$i^0$} -- (sbr);
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% null labels
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\draw[black] (1.4*\L,0.7*\L) node[right] (scrip) {$\mathcal{I}^+$}
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(1.5*\L,-0.6*\L) node[right] (scrip) {$\mathcal{I}^-$}
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(0.2*\L,-0.6*\L) node[right] (scrip) {$\mathcal{H}^-$}
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(0.5*\L,0.85*\L) node[right] (scrip) {$\mathcal{H}^+$};
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% singularity label
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\draw[thick,red,<-] (0,1.05*\L)
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-- (0,1.2*\L) node[above] {\color{red} singularity};
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% % Scwharzschild surface
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% \draw[thick,blue] (bif) .. controls (1.*\L,-0.35*\L) .. (2*\L,0);
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% \draw[thick,blue,<-] (1.75*\L,-0.1*\L) -- (1.9*\L,-0.5*\L)
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% -- (2*\L,-0.5*\L) node[right,align=left]
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% {$t=$ constant\\in Schwarzschild\\coordinates};
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% excision surface
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\draw[thick,dashed,red] (-0.3*\L,0.3*\L) -- (0.4*\L,\L);
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\draw[thick,red,<-] (-0.33*\L,0.3*\L)
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-- (-0.5*\L,0.26*\L) node[left,align=right] {excision\\surface};
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% Kerr-Schild surface
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\draw[green,thick] (0.325*\L,0.325*\L) .. controls (\L,0) .. (2*\L,0);
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\draw[green,dashed,thick] (0.325*\L,0.325*\L) -- (-0.051*\L,0.5*\L);
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% Kerr-Schild label
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\draw[green,thick,<-] (0.95*\L,0.15*\L) -- (1.2*\L,0.5*\L)
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-- (2*\L,0.5*\L) node[right,align=left]
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{time slice};
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\end{tikzpicture}
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\end{frame}
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\begin{frame}{Methods on evolving black holes: moving puncture}
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\begin{figure}
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\centering
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\includegraphics[width=0.42\textwidth]{imgs/moving_puncture_init.png}
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\includegraphics[width=0.45\textwidth]{imgs/moving_puncture_stable.png}
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\caption{The embedding of the initial slice (left) and the final slice (right) in the moving puncture method, from \cite{Hannam_2008}.}
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\end{figure}
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\end{frame}
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\begin{frame}{Methods on evolving black holes: moving puncture}
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\begin{figure}
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\centering
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\includegraphics[width=0.7\textwidth]{imgs/moving_puncture_penrose.png}
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\caption{The numerical time slices in the moving puncture method in the Penrose diagram, from \cite{Hannam_2008}.}
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\end{figure}
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\end{frame}
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\begin{frame}{Discontinuous Galerkin method and \texttt{nmesh}}
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\subsection{Discontinuous Galerkin method and \texttt{nmesh}}
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\end{frame}
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\begin{frame}{References}
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\printbibliography
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\end{frame}
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\end{document}
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