LaTex Template

LaTeX Template for writing lecture notes, thesis and more. Contains customs environments for quickly denoting theorems, lemmata and definitions in different colors.

Category

thesis

License

Free to use (MIT)

File

Test_document.tex

Test_document.texRead-only preview
\documentclass{yannick}

	%%%%%%%%%%%%%%%%
	% Titlepage %%%%
	%%%%%%%%%%%%%%%%

\title{LaTeX template for scripts } 
\author{by Yannick Kees \\  {\small University Bonn}}
\date{Summer 2021 }

	
	%%%%%%%%%%%%%%%%
	% Pagestyle %%%%
	%%%%%%%%%%%%%%%%	
	
\pagestyle{fancy}
\lhead{\textsc{Template file - Yannick Kees}}
\cfoot{\thepage }


\begin{document}

\maketitle
\newpage

	\section{Examples for using this class}
	% You can use 'dfn', 'satz', 'satzb', 'satzn', 'satznb', 'lem', 'lemn', 'lemnb', 'lemb', 'korollar'
	% 'yannick' & 'problem'
	\begin{dfn}
		We define the \textbf{Laplace-operator} as
			\begin{align*}
				\Delta f = \sum_{i=1}^n \frac{\partial^2 f}{\partial x_i^2}
			\end{align*}
	\end{dfn}

	\begin{satznb}{Fundamentallemma of calcus of variations}
		Let $\Omega$ be an open subset of $\mathbb{R}^2$ and $\Phi:\Omega\to\mathbb{R}$ be lokal integrable. If for any function $v:\Omega\to\mathbb{R}$ with compact support the integral 
		\begin{align*}
			\int\limits_{\Omega} \Phi(x)v(x)\,\mathrm{d}x
		\end{align*}
		vanishes, then $\Phi(x) = 0$ nearly everywhere.
	\end{satznb}

	\begin{satzn}{First green identity}
		{
			Let $\omega\subset \mathbb{R}^n$ be compact and $\phi$ and $\psi$ are two functions on $\Omega$, where $\phi$ is once and $\psi$ is twice differentable. Then
			\begin{align*}
				\int\limits_\Omega \phi \Delta(\psi)+\nabla\phi\cdot\nabla\psi\,\mathrm{d}m^d = \int\limits_{\partial \Omega}\phi \frac{\partial \psi}{\partial n}\,\mathrm{d}m^{d-1}
			\end{align*}
		}
		We use the gaußsche Integral formula to see that
		\begin{align*}
		 	\int\limits_{\partial \Omega}\phi \frac{\partial \psi}{\partial n}\,\mathrm{d}m^{d-1}&=  \int\limits_{\partial \Omega}(\phi\nabla\psi)\cdot \vec{n}\,\mathrm{d}m^{d-1}\\
		 	&= \int\limits_\Omega \nabla\mathrm{div}(\phi\nabla\psi)\\
		 	&= \int\limits_\Omega \phi \Delta(\psi)+\nabla\phi\cdot\nabla\psi\,\mathrm{d}m^d
		\end{align*}
	\end{satzn}
	
	\begin{korollar}
		If $\mathcal{L}u\geq 0$ in $\Omega$, then $u$ obtains its minimum in the boundary of $\Omega$.
	\end{korollar} 
	
	\begin{dfn}
		A problem is called \textbf{well posed}\index{well posed} if there exists a solution, that is unique and depends continuously on its data.
	\end{dfn}

	\begin{problem}{Laplace-Equation}{
		\begin{align*}
			\Delta u(x)&=0 && \text{for }x\in\Omega \\
			u(x)&=g(x) &&\text{for }x\in \Gamma
		\end{align*}
	}\end{problem}

	\begin{lem}
		{
			 Stability implies $\|A^{-1}_h\|_{\infty }\leq C_s$ and this bound is independent of $h$.
		}
		Let $\vec{v}_h$ be the coefficient vector of $v_h$ and $\vec{w}:= A_h\vec{v}_h $ is the coefficient vector of $\mathcal{L}_hv_h$
		\begin{align*}
			\|A^{-1}_h\vec{w}_h\|_{\infty }=\|\vec{v}_h \|_{\infty}=\|v_h \|_{\Omega}\leq C_s \|\mathcal{L}_hv_h \|_{\overline{\Omega_h}} = C_s\|A_h\vec{v}_h \|_{\infty}=C_s\|\vec{w}_h \|_{\infty}
		\end{align*}			 
		Then $\|A^{-1}_h\|_{\infty }$ is the smallest number for which this inequality holds.
	\end{lem}
		 
	\begin{yannick}{
		In contrast to Dirichlet boundary conditions, Neumann boundary conditions are not directly built into the search space. Therefore they are also calles \textbf{natural boundary conditions}.
	}\end{yannick}	
	
	\begin{lemn}{Comparison Principle}
		{ 
			If $\mathcal{L}u\leq\mathcal{L}v$ in $\Omega$ and $u\leq v$ in the boundary, then $u\leq v$ in $\overline{\Omega}$.
		}
		We use the maximum principle for
		\begin{align*}
			\mathcal{L}(v-u)\leq 0
		\end{align*}
		Then $(v-u)\leq 0$ in $\overline{\Omega}$.
	\end{lemn}
	
	\begin{lemb}
		Let $\mathcal{L}$ be uniformly elliptic. Then there exists a constant $c:=c(\Omega,\alpha)$, such that
		\begin{align*}
			|u(\vec{x})|\leq \max_{\vec{z}\in\Gamma}|u(\vec{z})|+c\cdot\sup_{\vec{z}\in\Omega}|(\mathcal{L}u )(\vec{z})|   &&\forall u\in C^2(\Omega)\cap C(\overline{\Omega}),\ \vec{x}\in\Omega
		\end{align*}
	\end{lemb}
	
	\begin{satz}
		{
	 		The space $C^\infty$ is dense in $H^m(\Omega)$.
	 	}
	 This theorem was proofen in 1964 by Meyers and Serrin. ($H=W$).
	 \end{satz}
\end{document}
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