Talk:PlanetPhysics/Examples of Lamellar Field

Original TeX Content from PlanetPhysics Archive

%%% This file is part of PlanetPhysics snapshot of 2011-09-01
%%% Primary Title: examples of lamellar field
%%% Primary Category Code: 02.30.-f
%%% Filename: ExamplesOfLamellarField.tex
%%% Version: 1
%%% Owner: pahio
%%% Author(s): pahio
%%% 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 PlanetPhysics 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

\begin{document}

 In the examples that follow, show that the given \htmladdnormallink{vector field}{http://planetphysics.us/encyclopedia/NeutrinoRestMass.html} $\vec{U}$ is lamellar everywhere in $\mathbb{R}^3$ and determine its \htmladdnormallink{scalar}{http://planetphysics.us/encyclopedia/Vectors.html} potential $u$.\\

\textbf{Example 1.}\, Given
\begin{align*}
\vec{U} \,:=\, y\,\vec{i}+(x+\sin{z})\,\vec{j}+y\cos{z}\,\vec{k}.
\end{align*}
For the rotor (\htmladdnormallink{curl}{http://planetphysics.us/encyclopedia/Curl.html}) of the field we obtain
$\displaystyle\nabla\!\times\!\vec{U} =   \left|\begin{matrix}
\vec{i} & \vec{j} & \vec{k}\\
\frac{\partial}{\partial{x}} & \frac{\partial}{\partial{y}} & \frac{\partial}{\partial{z}}\\
y & x\!+\!\sin{z} & y\cos{z}
\end{matrix}\right| \\=
\left(\frac{\partial(y\cos{z})}{\partial{y}}-\frac{\partial(x\!+\!\sin{z})}{\partial{z}}\right)\vec{i}
+\left(\frac{\partial{y}}{\partial{z}}-\frac{\partial(y\cos{z})}{\partial{x}}\right)\vec{j}
+\left(\frac{\partial(x\!+\!\sin{z})}{\partial{x}}-\frac{\partial{y}}{\partial{y}}\right)\vec{k}$,\\
which is identically $\vec{0}$ for all $x$, $y$, $z$.\, Thus, by the definition given in the parent entry, $\vec{U}$ is lamellar.\\
Since \,$\nabla{u} = \vec{U}$,\, the scalar potential \,$u = u(x,\,y,\,z)$\, must satisfy the conditions
$$\frac{\partial{u}}{\partial{x}} = y,\quad \frac{\partial{u}}{\partial{y}} = x\!+\!\sin{z},\quad \frac{\partial
{u}}{\partial{z}} = y\cos{z}.$$
Thus we can write
$$u = \int y\,dx = xy+C_1,$$
where $C_1$ may depend on $y$ or $z$. Differentiating this result with respect to $y$ and comparing to the second
condition, we get
$$\frac{\partial{u}}{\partial{y}} = x+\frac{\partial{C_1}}{\partial{y}} = x+\sin{z}.$$
Accordingly,
$$C_1 = \int\sin{z}\,dy = y\sin{z}+C_2,$$
where $C_2$ may depend on $z$.\, So
$$u = xy+y\sin{z}+C_2.$$
Differentiating this result with respect to $z$ and comparing to the third condition yields
$$\frac{\partial{u}}{\partial{z}} \,=\, y\cos{z}+\frac{\partial{C_2}}{\partial{z}} \,=\, y\cos{z}.$$
This means that $C_2$ is an arbitrary constant. Thus the form
$$u = xy+y\sin{z}+C$$
expresses the required potential \htmladdnormallink{function}{http://planetphysics.us/encyclopedia/Bijective.html}.\\

\textbf{Example 2.}\, This is a particular case in $\mathbb{R}^2$:
\begin{align*}
\vec{U}(x,\,y,\,0) \,:=\, \omega y \,\vec{i}+ \omega x \,\vec{j}, \quad \omega = \mbox{constant}
\end{align*}
Now,\; $\displaystyle\nabla\!\times\!\vec{U} = \left|\begin{matrix}
\vec{i} & \vec{j} & \vec{k}\\
\frac{\partial}{\partial{x}} & \frac{\partial}{\partial{y}} & \frac{\partial}{\partial{z}}\\
\omega y & \omega x & 0
\end{matrix}\right| =
\left(\frac{\partial(\omega x)}{\partial{x}}-\frac{\partial(\omega y)}{\partial{y}}\right)\vec{k}=\vec{0}$,\, and so $\vec{U}$ is lamellar.

Therefore there exists a potential field $u$ with\, $\vec{U}=\nabla{u}$.\, We deduce successively:
$$\frac{\partial{u}}{\partial{x}} = \omega y; \;\; u(x,y,0) =
\omega xy+f(y); \;\; \frac{\partial{u}}{\partial{y}}=
\omega x+f'(y)\equiv \omega x; \;\; f'(y)=0; \;\; f(y)=C$$
Thus we get the result
$$u(x,\,y,\,0) = \omega xy+C,$$
which corresponds to a particular case in $\mathbb{R}^2$.\\

\textbf{Example 3.}\, Given
\begin{align*}
\vec{U} \,:=\, ax\vec{i}+by\vec{j}-(a+b)z)\vec{k}.
\end{align*}
The rotor is now\, $\displaystyle\nabla\!\times\!\vec{U} =
\left|\begin{matrix}
\vec{i} & \vec{j} & \vec{k}\\
\frac{\partial}{\partial{x}} & \frac{\partial}{\partial{y}} & \frac{\partial}{\partial{z}}\\
ax & by & -(a+b)z
\end{matrix}\right|= \vec{0}.$\; From\, $\nabla u=\vec{U}$\, we obtain
$$\frac{\partial u}{\partial x} = ax \; \implies \; u = \frac{ax^2}{2}+f(y,z) \quad(1)$$
$$\frac{\partial u}{\partial y} = by \; \implies \; u = \frac{by^2}{2}+g(z,x) \quad(2)$$
$$\frac{\partial u}{\partial z} = -(a+b)z \; \implies \;u = -(a+b)\frac{z^2}{2}+h(x,y) \quad(3)$$
Differentiating (1) and (2) with respect to $z$ and using (3) give
$$-(a+b)z = \frac{\partial f(y,z)}{\partial z} \; \implies \; f(y,z) = -(a+b)\frac{z^2}{2}+F(y) \quad(1');$$
$$-(a+b)z=\frac{\partial g(z,x)}{\partial z} \; \implies \; g(z,x) = -(a+b)\frac{z^2}{2}+G(x) \quad (2').$$
We substitute $(1')$ and $(2')$ again into (1) and (2) and deduce as follows:
$$u = \frac{ax^2}{2}-(a+b)\frac{z^2}{2}+F(y); \;\; \frac{\partial u}{\partial y} = F'(y) = by;
\;\; F(y) = \frac{by^2}{2}+C_1; \;\; f(y,z) = \frac{by^2}{2}-(a+b)\frac{z^2}{2}+C_1 \quad (1'');$$
$$u = \frac{by^2}{2}-(a+b)\frac{z^2}{2}+G(x); \;\; \frac{\partial u}{\partial x} = G'(x) = ax;
\;\; G(x) = \frac{ax^2}{2}+C_2; \;\; g(z,x) = \frac{ax^2}{2}-(a+b)\frac{z^2}{2}+C_2\quad (2'');$$
putting $(1'')$, $(2'')$ into (1), (2) then gives us
$$u = \frac{ax^2}{2}+\frac{by^2}{2}-(a+b)\frac{z^2}{2}+C_1, \quad
u = \frac{ax^2}{2}+\frac{by^2}{2}-(a+b)\frac{z^2}{2}+C_2,$$
whence, by comparing,\, $C_1 = C_2 = C$,\, so that by (3), the expression $h(x,y)$ and $u$ itself have been found, that is,
$$u = \frac{ax^2}{2}+\frac{by^2}{2}-(a+b)\frac{z^2}{2}+C.$$

Unlike Example 1, the last two examples are also \htmladdnormallink{solenoidal}{http://planetphysics.us/encyclopedia/SolenoidalVectorField.html}, i.e.\, $\nabla\cdot\vec{U}=0$,\, which physically may be interpreted as the \htmladdnormallink{continuity equation}{http://planetphysics.us/encyclopedia/ContinuityEquation.html} of an incompressible fluid flow.\\

\textbf{Example 4.}\, An additional example of a \htmladdnormallink{lamellar field}{http://planetphysics.us/encyclopedia/LamellarField.html} would be
$$\vec{U} \,:=\, -\frac{ay}{x^2+y^2}\vec{i}+\frac{ax}{x^2+y^2}\vec{j}+v(z)\vec{k}$$
with a differentiable function \,$v:\mathbb{R}\to\mathbb{R}$;\, if $v$ is a constant, then $\vec{U}$ is also solenoidal.

\end{document}