From 156b00cbe78b1b269397577d47a6a11330c34103 Mon Sep 17 00:00:00 2001
From: Yingjie Wang <phywyj@gmail.com>
Date: Fri, 10 Apr 2026 03:40:25 -0400
Subject: [PATCH] update: auto commit

---
 report.tex | 2 +-
 1 file changed, 1 insertion(+), 1 deletion(-)

diff --git a/report.tex b/report.tex
index 0bce9af..9da00b7 100644
--- a/report.tex
+++ b/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}