Talk:PlanetPhysics/Lamellar Field

From Wikiversity
Jump to navigation Jump to search

Original TeX Content from PlanetPhysics Archive[edit source]

%%% This file is part of PlanetPhysics snapshot of 2011-09-01 %%% Primary Title: lamellar field %%% Primary Category Code: 02.30.Em %%% Filename: LamellarField.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}

A \htmladdnormallink{vector field}{http://planetphysics.us/encyclopedia/NeutrinoRestMass.html} \,$\vec{F} = \vec{F}(x,\,y,\,z)$,\, defined in an open set $D$ of $\mathbb{R}^3$, is\, {\em lamellar}\, if the condition

$$\nabla\!\times\!\vec{F} = \vec{0}$$ is satisfied in every point \,$(x,\,y,\,z)$\, of $D$.

Here, $\nabla\!\times\!\vec{F}$ is the \htmladdnormallink{curl}{http://planetphysics.us/encyclopedia/Curl.html} or {\em rotor} of $\vec{F}$.\, The condition is equivalent with both of the following: \begin{itemize} \item The line integrals $$\oint_s \vec{F}\cdot d\vec{s}$$ taken around any closed contractible curve $s$ vanish. \item The vector field has a {\em scalar potential}\, $u = u(x,\,y,\,z)$\, which has continuous partial derivatives and which is up to a constant term unique in a simply connected \htmladdnormallink{domain}{http://planetphysics.us/encyclopedia/Bijective.html}; the \htmladdnormallink{scalar}{http://planetphysics.us/encyclopedia/Vectors.html} potential means that $$\vec{F} = \nabla u.$$ \end{itemize} The scalar potential has the expression $$u = \int_{P_0}^P\vec{F}\cdot d\vec{s},$$ where the point $P_0$ may be chosen freely,\, $P = (x,\,y,\,z)$.\\

\textbf{Note.}\, In physics, $u$ is in general replaced with\, $V = -u$.\, If the $\vec{F}$ is interpreted as a force, then the potential $V$ is equal to the \htmladdnormallink{work}{http://planetphysics.us/encyclopedia/Work.html} made by the force when its point of application is displaced from $P_0$ to infinity.

\end{document}