Talk:PlanetPhysics/Example of Solving the Heat Equation

Original TeX Content from PlanetPhysics Archive

%%% This file is part of PlanetPhysics snapshot of 2011-09-01
%%% Primary Title: example of solving the heat equation
%%% Primary Category Code: 44.
%%% Filename: ExampleOfSolvingTheHeatEquation.tex
%%% Version: 1
%%% Owner: bloftin
%%% Author(s): bloftin
%%% PlanetPhysics is released under the GNU Free Documentation License.
%%% You should have received a file called fdl.txt along with this file.        
%%% If not, please write to gnu@gnu.org.
\documentclass[12pt]{article}
\pagestyle{empty}
\setlength{\paperwidth}{8.5in}
\setlength{\paperheight}{11in}

\setlength{\topmargin}{0.00in}
\setlength{\headsep}{0.00in}
\setlength{\headheight}{0.00in}
\setlength{\evensidemargin}{0.00in}
\setlength{\oddsidemargin}{0.00in}
\setlength{\textwidth}{6.5in}
\setlength{\textheight}{9.00in}
\setlength{\voffset}{0.00in}
\setlength{\hoffset}{0.00in}
\setlength{\marginparwidth}{0.00in}
\setlength{\marginparsep}{0.00in}
\setlength{\parindent}{0.00in}
\setlength{\parskip}{0.15in}

\usepackage{html}

% this is the default PlanetMath preamble. as your knowledge
% of TeX increases, you will probably want to edit this, but
% it should be fine as is for beginners.

% almost certainly you want these
\usepackage{amssymb}
\usepackage{amsmath}
\usepackage{amsfonts}

% used for TeXing text within eps files
%\usepackage{psfrag}
% need this for including graphics (\includegraphics)
\usepackage{graphicx}
% for neatly defining theorems and propositions
\usepackage{amsthm}
% making logically defined graphics
%\usepackage{xypic}

% there are many more packages, add them here as you need them

% define commands here

\theoremstyle{definition}
\newtheorem*{thmplain}{Theorem}

\begin{document}

 Let a thin square-formed plate of heat conducting homogeneous material be in the $xy$-plane with sides on the $x$-axis (isolated), on the line\, $y = \pi$ (held at the constant temperature\, $u = C$), and on the vertical lines\, $x = 0$\, and\, $x = \pi$ (both held at the constant temperature\, $u = 0$).\, Determine the \htmladdnormallink{temperature}{http://planetphysics.us/encyclopedia/BoltzmannConstant.html} \htmladdnormallink{function\,}{http://planetphysics.us/encyclopedia/Bijective.html} $(x,\,y)\mapsto u(x,\,y)$\, on the plate, when the faces of the plate are isolated.

The \htmladdnormallink{equation of the heat flow}{http://planetphysics.us/encyclopedia/HeatEquation.html} in this stationary case is
\begin{align}
\nabla^2 u \equiv u''_{xx}+u''_{yy} = 0
\end{align}
under the \htmladdnormallink{boundary}{http://planetphysics.us/encyclopedia/PiecewiseLinear.html} conditions
$$u(0,\,y) = 0,\,\, u(\pi,\,y) = 0,\,\, u(x,\,\pi) = C,\,\, u'_y(x,\,0) = 0.$$
We first try to separate the variables, i.e. seek the solution of (1) of the form
$$u(x,\,y) := X(x)Y(y).$$
Then we get
$$u'_x = X'Y,\,\, u''_{xx} = X''Y,\,\, u'_y = XY',\,\, u''_{yy} = XY'',$$
and thus (1) gets the form
\begin{align}
X''Y+XY'' = 0
\end{align}
and the boundary conditions
$$X(0) = X(\pi) = 0,\,\,\, X(x) = \frac{C}{Y(\pi)},\,\,\, Y'(0) = 0.$$
We separate the variables in (2):
$$\frac{X''}{X} = -\frac{Y''}{Y}$$
This equation is not possible unless both sides are equal to a same negative constant $-k^2$, which implies for\, $X'' = -k^2X$\, the solution
$$X := C_1\cos{kx}+C_2\sin{kx}$$
and for\, $Y'' = k^2Y$\, the solution
$$Y := D_1\cosh{ky}+D_2\sinh{ky}.$$
The two first boundary conditions give\, $0 = X(0) = C_1$,\, $0 = X(\pi) = 0+C_2\sin{k\pi}$,\, and since\, $C_2 \ne 0$,\, we must have\, $\sin{k\pi} = 0$,\, i.e.
$$0 < k := n = 1,\,2,\,3,\,\ldots$$
Therefore
$$X(x) := C_2\sin{nx},\,\,\, Y'(y) \equiv nD_1\sinh{ny}+nD_2\cosh{ny}.$$
The fourth boundary condition now gives that\, $0 = Y'(0) = nD_2$;\,
thus\, $D_2 = 0$\, and\, $Y(y) := D_1\cosh{ny}.$\, So (1) has infinitely many solutions
\begin{align}
u_n := C_2D_1\sin{nx}\cosh{ny} = A_n\sin{nx}\cosh{ny}
\end{align}
with\, $n\in\mathbb{Z}_+$\, and they all satisfy the boundary conditions except the third.\, Because of the linearity of (1), also the sum
$$u := \sum_{n=1}^\infty A_n\sin{nx}\cosh{ny}$$
of the functions (3) satisfy (1) and those boundary conditions, provided that this series converges.\, The third boundary condition requires that
$$C = u(x,\,\pi) = \sum_{n=1}^\infty A_n\sin{nx}\cosh{n\pi} =
\sum_{n=1}^\infty(A_n\cosh{n\pi})\sinh{nx}$$
on the interval\, $0 \leqq x \leqq \pi$.\, But this is the Fourier sine series of the constant function\, $x \mapsto C$\, on the half-interval\, $[0,\,\pi]$,\, whence
$$A_n\cosh{n\pi} = \frac{2}{\pi}\int_0^\pi C\sin{nx}\,dx =
\frac{2C}{n\pi}(1\!-\!(-1)^n)\quad \forall n\in\mathbb{Z}_+.$$
The even $n$'s here give 0 and the odd give
$$A_{2m+1} := \frac{4C}{(2m\!+\!1)\pi\cosh(2m\!+\!1)\pi}
\quad (m = 0,\,1,\,2,\,\ldots)$$

Thus we obtain the solution
$$u(x,\,y) \,:=\,
\frac{4C}{\pi}\sum_{m=0}^\infty\frac{\sin(2m\!+\!1)x\cosh(2m\!+\!1)y}
{(2m\!+\!1)\cosh(2m\!+\!1)\pi}.$$
It can be shown that this series converges in the whole square of the plate.

\subsection*{Visualization of the solution}

\begin{figure}[!htb]
\begin{center}
\includegraphics{heat-surface.eps}
\caption{Surface plot of the solution $u(x,y)$, for $C=1$}
\end{center}
\end{figure}

\begin{figure}[!htb]
\begin{center}
\includegraphics{heat-color.eps}
\caption{Color-coded plot of the temperature $u(x,y)$}
\end{center}
\end{figure}

\textbf{Remark.} The function $u$ has been approximated in the plot by computing a partial sum of the true infinite-series solution.\, However,
there is substantial numerical error in the approximate solution near\,
$y = \pi$,\, evident in the small oscillations observed in the surface plot, that should not be there in theory.\,
This phenomenon is actually inevitable given that the boundary conditions are actually discontinuous at the corners\, $(0,\,\pi)$\, and\, $(\pi,\,\pi)$.

More precisely, observe that when\, $y = \pi$,\, the formula for\, $u(x,\,y)$\, reduces to the Fourier series
\[
\frac{4C}{\pi} \left( \sin{x}+\frac{\sin{3x}}{3}+\frac{\sin{5x}}{5}+\dotsb \right)
\]
for the discontinuous function on\, $[-\pi,\,\pi]$:

\[
x \mapsto \begin{cases}
C \, , & 0 < x < \pi\\
-C \, , & -\pi < x < 0
\end{cases} \,
\]





That means the Fourier expansion will necessarily be subject to the {\em Gibbs phenomenon}.\, Of course, the series also cannot converge absolutely; in other words, the terms of the series decay too slowly in \htmladdnormallink{magnitude}{http://planetphysics.us/encyclopedia/AbsoluteMagnitude.html}, adversely affecting the numerical solution.

\begin{itemize}
\item
\htmladdnormallink{Python program to compute\, $u(x,\,y)$\, and produce the two figures}{http://gold-saucer.afraid.org/math/planetmath/ExampleOfSolvingTheHeatEquation/heat.py}
\end{itemize}

\end{document}