update: auto commit

report.tex

@@ -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}