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%
% Copyright © 2014 Peeter Joot. All Rights Reserved.
% Licenced as described in the file LICENSE under the root directory of this GIT repository.
%
%\input{../blogpost.tex}
%\renewcommand{\basename}{multiphysicsL17}
%\renewcommand{\dirname}{notes/ece1254/}
%\newcommand{\keywords}{ECE1254H}
%\input{../peeter_prologue_print2.tex}
%
%
%\beginArtNoToc
%\generatetitle{ECE1254H Modeling of Multiphysics Systems. Lecture 17: Stability. Taught by Prof.\ Piero Triverio}
%%\chapter{Stability}
%\label{chap:multiphysicsL17}
%
%\section{Disclaimer}
%
%Peeter's lecture notes from class. These may be incoherent and rough.
%
\section{Stability (continued).}
\index{stability}
%
Continuing with the simple continuous time test system
%
\begin{equation}\label{eqn:multiphysicsL17:20}
\dot{x}(t) = \lambda x(t)
\end{equation}
%
With the application of a trial solution \( x(t) = e^{s t} \), the resulting characteristic equation is
%
\begin{equation}\label{eqn:multiphysicsL17:40}
s = \lambda,
\end{equation}
%
and stability follows, provided that \( \Real(\lambda) < 0 \) as sketched in \cref{fig:lecture17:lecture17Fig1}.
%
\imageFigure{../figures/ece1254-multiphysics/lecture17Fig1}{Stability region.}{fig:lecture17:lecture17Fig1}{0.2}
%
Utilizing LMS methods, for example TR, the discrete time system results, such as
%
\begin{equation}\label{eqn:multiphysicsL17:60}
\gamma_{-1} x_{n+1} +
\gamma_{0} x_{n} +
\gamma_1 x_{n-1}
+ \cdots
= 0.
\end{equation}
%
% n+1 = k
% n = k-1
% n + j = k - 1 + j
With a substitution \( x_{n + j} = z^{k - 1 + j} \), a characteristic polynomial results
%
\begin{equation}\label{eqn:multiphysicsL17:80}
\gamma_{-1} z^{k} +
\gamma_{0} z^{k-1} +
\gamma_1 z^{k-2} + \cdots = 0.
\end{equation}
%
This is stable provided \( \Abs{z_l} < 1 \), as illustrated in \cref{fig:lecture17:lecture17Fig2}.
%
\imageFigure{../figures/ece1254-multiphysics/lecture17Fig2}{Stability region in z-domain.}{fig:lecture17:lecture17Fig2}{0.3}
%
... SWITCHED TO SLIDES.
%
\makedefinition{Stiff.}{dfn:multiphysicsL17:100}{
A \textAndIndex{stiff} system is one that has multiple timescales, as characterized by a significant range of eigenvalues.
}
%
\makedefinition{Lossless system.}{dfn:multiphysicsL17:120}{
Lossless \index{pole!lossless} poles are those that reside strictly on the imaginary axis.
}
%
\makedefinition{Lossly system.}{dfn:multiphysicsL17:140}{
Lossly poles \index{pole!lossly} are those that reside strictly to the left of the imaginary axis.
}
%
\makedefinition{Active system.}{dfn:multiphysicsL17:160}{
Active poles \index{pole!active} are those that reside strictly to the right of the imaginary axis.
}
%
\makedefinition{A-stable.}{dfn:multiphysicsL17:170}{
See slides.
}
%
\index{Dahlquist's theorem}
\maketheorem{Dahlquist's theorem.}{thm:multiphysicsL17:180}{
There are no LMS methods of order greater than 2 that are A-stable. Also known as the Dahlquist barrier. The TR method has the lowest error of the A-stable LMS methods.
}
%
\paragraph{Some recent developments}
\index{backward differentiation formula}
%
The backward differentiation formulas (BDF) are of \( \text{order} > 2 \). They are not A-stable, but can be sufficient with stability sketched in \cref{fig:lecture17:lecture17Fig3}.
%
\imageFigure{../figures/ece1254-multiphysics/lecture17Fig3}{BDF stability region.}{fig:lecture17:lecture17Fig3}{0.2}
%
Also available are the Obreshkov formulas \citep{butcherOrder}, which are both A-stable and of \( \text{order} > 2 \). There is a cost to both of these methods: computation of the derivatives at each step.
%