update: auto commit

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2026-04-10 03:40:25 -04:00
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@@ -293,7 +293,7 @@
\begin{frame}{Methods on evolving black holes: moving puncture}
In the isotropic coordinate for Schwarzschild black hole, the spical metric
In the isotropic coordinate for Schwarzschild black hole, the spacial metric
\begin{equation}
\dd{l^2} = \left( 1+\frac{M}{2r} \right)^4 (\dd{r^2} + r^2 \dd{\Omega^2})
\end{equation}