notes

uni notes
git clone git://popovic.xyz/notes.git
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commit 962b6aae46913eb88f7f4d2cd790ea544f27ccd0
parent 34433435cdf448e98fc98f08f68aa0a889f62fc8
Author: miksa <milutin@popovic.xyz>
Date:   Thu, 30 Jun 2022 16:35:48 +0200

done app pde

Diffstat:
Aapp_pde/build/main.bbl | 164+++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++
Mapp_pde/build/main.pdf | 0
Aapp_pde/build/main.run.xml | 85+++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++
Mapp_pde/chap1.tex | 4++--
Aapp_pde/pres/build/main.bbl | 208+++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++
Aapp_pde/pres/build/main.nav | 48++++++++++++++++++++++++++++++++++++++++++++++++
Mapp_pde/pres/build/main.pdf | 0
Aapp_pde/pres/build/main.run.xml | 85+++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++
Aapp_pde/pres/build/main.snm | 0
Mapp_pde/pres/main.tex | 65+++++++++++++++++++++++++++++++++++------------------------------
10 files changed, 627 insertions(+), 32 deletions(-)

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\field{sortinithash}{4f6aaa89bab872aa0999fec09ff8e98a} + \field{labelnamesource}{author} + \field{labeltitlesource}{title} + \field{series}{Cambridge Texts in Applied Mathematics} + \field{title}{A Modern Introduction to the Mathematical Theory of Water Waves} + \field{year}{1997} + \verb{doi} + \verb 10.1017/CBO9780511624056 + \endverb + \endentry + \entry{constantin_tsunami}{article}{} + \name{author}{1}{}{% + {{hash=11842dc817348c4beac10afc990ea158}{% + family={Constantin}, + familyi={C\bibinitperiod}, + given={Adrian}, + giveni={A\bibinitperiod}}}% + } + \strng{namehash}{11842dc817348c4beac10afc990ea158} + \strng{fullhash}{11842dc817348c4beac10afc990ea158} + \strng{bibnamehash}{11842dc817348c4beac10afc990ea158} + \strng{authorbibnamehash}{11842dc817348c4beac10afc990ea158} + \strng{authornamehash}{11842dc817348c4beac10afc990ea158} + \strng{authorfullhash}{11842dc817348c4beac10afc990ea158} + \field{sortinit}{2} + \field{sortinithash}{8b555b3791beccb63322c22f3320aa9a} + 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<provides type="dynamic"> + <file>main.bcf</file> + </provides> + <requires type="dynamic"> + <file>main.bbl</file> + </requires> + <requires type="static"> + <file>blx-dm.def</file> + <file>blx-compat.def</file> + <file>biblatex.def</file> + <file>standard.bbx</file> + <file>numeric.bbx</file> + <file>numeric.cbx</file> + <file>biblatex.cfg</file> + <file>english.lbx</file> + </requires> + </internal> + <external package="biblatex" priority="5" active="0"> + <generic>biber</generic> + <cmdline> + <binary>biber</binary> + <infile>main</infile> + </cmdline> + <input> + <file>main.bcf</file> + </input> + <output> + <file>main.bbl</file> + </output> + <provides type="dynamic"> + <file>main.bbl</file> + </provides> + <requires type="dynamic"> + <file>main.bcf</file> + </requires> + <requires type="editable"> + <file>uni.bib</file> + </requires> + </external> +</requests> diff --git a/app_pde/chap1.tex b/app_pde/chap1.tex @@ -199,8 +199,8 @@ Thereby the equations become For now we have separated two simplifications, that define an \textbf{idealized/perfect fluid} \begin{enumerate} - \item \textbf{incompressible} $\qquad \mu=0$ - \item \textbf{inviscid} $\quad \rho = \text{const.},\ \nabla \mathbf{u}= + \item \textbf{inviscid} $\qquad \mu=0$ + \item \textbf{incompressible} $\quad \rho = \text{const.},\ \nabla \mathbf{u}= 0$ \end{enumerate} \subsection{Vorticity and irrotational Flow} diff --git a/app_pde/pres/build/main.bbl b/app_pde/pres/build/main.bbl @@ -0,0 +1,208 @@ +% $ biblatex auxiliary file $ +% $ biblatex bbl format version 3.2 $ +% Do not modify the above lines! +% +% This is an auxiliary file used by the 'biblatex' package. +% This file may safely be deleted. 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<file>standard.bbx</file> + <file>numeric.bbx</file> + <file>numeric.cbx</file> + <file>biblatex.cfg</file> + <file>english.lbx</file> + </requires> + </internal> + <external package="biblatex" priority="5" active="0"> + <generic>biber</generic> + <cmdline> + <binary>biber</binary> + <infile>main</infile> + </cmdline> + <input> + <file>main.bcf</file> + </input> + <output> + <file>main.bbl</file> + </output> + <provides type="dynamic"> + <file>main.bbl</file> + </provides> + <requires type="dynamic"> + <file>main.bcf</file> + </requires> + <requires type="editable"> + <file>uni.bib</file> + </requires> + </external> +</requests> diff --git a/app_pde/pres/build/main.snm b/app_pde/pres/build/main.snm diff --git a/app_pde/pres/main.tex b/app_pde/pres/main.tex @@ -49,13 +49,20 @@ \title {Mathematical Modeling of Water-Wave Problems} \subtitle{Applied PDE Seminar} -\author[Popović Milutin] -{Popović Milutin} -\date{17. March 2021} +%\author[Popović Milutin] +%{Popović Milutin \inst{1}\\[1ex] {\small supervisor\inst{1,2}} + +\author[Popović Milutin]{Popović Milutin\\[10mm]{\small Supervisor: Sabine Hittmeir}} +\date{29. June 2022} \begin{document} \begin{frame} \titlepage + \nocite{johnson_1997} + \nocite{vallis_2017} + \nocite{constantin_tsunami} + \nocite{rupert_2009} + \nocite{mathe-physik} \end{frame} @@ -70,7 +77,6 @@ \item[$\circ$] Fluid density\\ $\rho(\vec{x}, t)$ \item[$\circ$] Velocity Field\\ $\vec{u}(\vec{x}, t) = (u, v, w)$ - \item[$\circ$] Pressure \\$P(\vec{x}, t)$ \end{itemize} \column{0.57\textwidth} @@ -122,7 +128,7 @@ conservation} \begin{align} \hspace{0.3\linewidth} \frac{\partial \rho}{\partial t} - \nabla \cdot (\rho \vec{u}) = + +\nabla \cdot (\rho \vec{u}) = 0 \nonumber \end{align} \end{itemize} @@ -192,6 +198,16 @@ \end{frame} \begin{frame} + \frametitle{Perfect Fluid} + \begin{itemize} + \item \textbf{inviscid} $\mu = 0$ + \item \textbf{incompressible} $\rho = \text{const}.$, then + $\nabla \vec{u} = 0$ + \end{itemize} + + \end{frame} + + \begin{frame} \frametitle{Boundary Conditions for Water Waves} \begin{center} \begin{tabular}{@{}l@{}} @@ -211,10 +227,10 @@ \begin{tabular}{@{}l@{}} \tabitem $h_0$ for the typical water depth\\ \tabitem $\lambda$ for the typical wavelength\\ - \tabitem $\frac{\lambda}{\sqrt{g h_0}}$ time scale - of wave propagation\\ \tabitem $\sqrt{g h_0}$ velocity scale of waves in $(x, y)$\\ + \tabitem $\frac{\lambda}{\sqrt{g h_0}}$ time scale + of wave propagation\\ \tabitem $\frac{h_0 \sqrt{g h_0} }{\lambda}$ velocity scale in $z$ \end{tabular} \end{center} @@ -223,7 +239,7 @@ \frac{h_0}{\lambda}$ \\ \centering - $\rightarrow$ \textbf{Amplitude Parameter} + $\rightarrow$ \textbf{Amplitude parameter} $\varepsilon=\frac{a}{h_0}$ \end{frame} @@ -302,28 +318,27 @@ \begin{frame} \frametitle{History of the Soliton} \begin{itemize} + \item[$\circ$] John Scott Russell discovered the solitary wave in 1834, + firstly calling it the \textbf{wave of translation} \item[$\circ$] a \textbf{soliton} is a solitary wave that resists dispersion, maintaining its shape while it propagates at constant velocity\\ - \item[$\circ$] John Scott Russell discovered the solitary wave in 1834, - firstly calling it the \textbf{wave of translation} \end{itemize} \end{frame} \begin{frame} \frametitle{Korteweg-de Vries equation (KdV)} - Korteweg-de Vries equation: nonlinear, dispersive PDE + Korteweg-de Vries equation: nonlinear PDE \begin{ceqn} \begin{align} - 2\eta_t + 3 \eta \eta_\xi + \frac{K}{3} \eta_{\xi\xi\xi} = - 0\qquad \left(\xi = x-ct, \tau = \varepsilon t\right)\nonumber + \eta_t + 6K \eta \eta_{x} + \eta_{x x x} = 0\nonumber \end{align} \end{ceqn} With Solution \begin{ceqn} \begin{align} - \eta(\xi, \tau) = 2c^2 \text{sech}^2\left( \sqrt{\frac{3}{2K}} - \left(\xi- \tau\right) \right)\nonumber + \eta(x, t) = 2c^2 \text{sech}^2\Big( c + \left(x - 4c^2t\right) \Big)\nonumber \end{align} \end{ceqn} \end{frame} @@ -347,13 +362,8 @@ \centering \includegraphics[width=0.35\textwidth]{./pics/water-surface.png} \caption{Earthquake generating a tsunami with $\lambda = 100\ - \text{km},\;\; a = 1\ \text{m}$} + \text{km},\;\; a = 1\ \text{m}$ (found in \cite{graph_meter})} \end{figure} - \begin{ceqn} - \begin{align} - \end{align} - \end{ceqn} - \end{frame} \begin{frame} @@ -361,17 +371,17 @@ \begin{itemize} \item[$\circ$] $\varepsilon = \frac{a}{h_0}$ and $\delta = - \frac{h_0}{\lambda}$ need to ender the regime + \frac{h_0}{\lambda}$ need to enter the regime $\varepsilon=O(\delta^2)$ for the KdV equation to become relevant \item[$\circ$] But also the geophysical scales need to be $\xi = O(1)$ and $\tau = - O(1)$ for the KdV-balance to become relevant, that is + O(1)$ for the KdV dynamics to become relevant, that is \begin{ceqn} \begin{align} x = O\left(\varepsilon^{-1} \lambda \right) \end{align} \end{ceqn} - \item[$\circ$] KdV balance is when the waves are ordered with the + \item[$\circ$] KdV dynamics is when the waves are ordered with the highest in front following an oscillatory tale \item[$\circ$] This happens because wave amplitude is proportional to wave speed @@ -383,7 +393,7 @@ \frametitle{2004 Tsunami: Regime of Validity} \begin{ceqn} \begin{align} - \lambda = 10\ \text{km}\qquad a = 1\ \text{m}\nonumber + \lambda = 100\ \text{km}\qquad a = 1\ \text{m}\nonumber \end{align} \end{ceqn} \begin{columns} @@ -440,11 +450,6 @@ \end{frame} \begin{frame}{Bibliography} - \nocite{johnson_1997} - \nocite{vallis_2017} - \nocite{constantin_tsunami} - \nocite{rupert_2009} - \nocite{mathe-physik} \printbibliography \end{frame} \end{document}