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\documentclass[aspectratio=169]{beamer}
\usepackage{amsmath,unicode-math,physics,tensor}
\useoutertheme{metropolis}
\useinnertheme{metropolis}
\usecolortheme{metropolis}
\usefonttheme{professionalfonts}
\setbeamerfont{title}{size=\Large, series=\bfseries}
\setbeamerfont{author}{size=\small}
\setbeamerfont{date}{size=\small}
\setbeamertemplate{footline}{\vspace*{0.3cm}}
\unimathsetup{math-style=ISO, bold-style=ISO, mathrm=sym}
\setsansfont{FiraGO}[BoldFont=* SemiBold, Numbers=Monospaced]
\setmathfont{Fira Math Regular}
\title{Fira Math}
\subtitle{Sans-serif font with Unicode math support}
\author{Xiangdong Zeng}
\date{2018/10/26\quad v0.3.1}
\begin{document}
\maketitle
\begin{frame}[noframenumbering]{General relativity}
\begin{itemize}
\item Covariant derivative:
\[
\nabla \symbf{X} = \tensor{X}{^\alpha_{;\beta}} \pdv{x^\alpha} \otimes \dd{x^\beta}
= \qty(\tensor{X}{^\alpha_{,\beta}} + \Gamma^{\alpha}_{\beta\gamma} \, X^\gamma) \,
\pdv{x^\alpha} \otimes \dd{x^\beta}
\]
\item Einstein's field equations:
\[ G_{\mu\nu} \equiv R_{\mu\nu} - \frac{1}{2} R g_{\mu\nu} = \frac{8\pi G}{c^4} T_{\mu\nu} \]
%\item Conservation of energy and momentum:
% \[ \nabla_\beta T^{\alpha\beta} = \tensor{T}{^{\alpha\beta}_{;\,\beta}} = 0 \]
\item Schwarzschild metric:
\[
c^2 \dd{\tau}^2 = \qty(1-\frac{r_{\mathrm{s}}}{r}) \, c^2 \dd{t}^2
- \qty(1-\frac{r_{\mathrm{s}}}{r})^{-1} \dd{r}^2
- r^2 \underbrace{\qty(\dd{\theta}^2 + \sin^2 \theta \dd{\varphi}^2)}_{\dd{\Omega}^2}
\]
\item Einstein--Hilbert action:
\[ S = \frac{1}{2\kappa} \int R \sqrt{-g} \dd[4]{x} \]
\end{itemize}
\end{frame}
\end{document}
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