Talk:PlanetPhysics/Archimedes Principle

Original TeX Content from PlanetPhysics Archive
%%% This file is part of PlanetPhysics snapshot of 2011-09-01 %%% Primary Title: Archimedes' Principle %%% Primary Category Code: 47.85.Dh %%% Filename: ArchimedesPrinciple.tex %%% Version: 3 %%% Owner: joshsamani %%% Author(s): joshsamani %%% 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}

Archimedes' Principle states that

\emph{When a floating body of \htmladdnormallink{mass}{http://planetphysics.us/encyclopedia/CosmologicalConstant.html} $M$ is in \htmladdnormallink{equilibrium}{http://planetphysics.us/encyclopedia/InertialSystemOfCoordinates.html} with a fluid of constant density, then it displaces a mass of fluid $M_d$ equal to its own mass; $M_d = M$.}

Archimedes' principle can be justified via arguments using some elementary \htmladdnormallink{classical mechanics}{http://planetphysics.us/encyclopedia/NewtonianMechanics.html}. We use a Cartesian coordinate \htmladdnormallink{system}{http://planetphysics.us/encyclopedia/SimilarityAndAnalogousSystemsDynamicAdjointnessAndTopologicalEquivalence.html} oriented such that the $z$-axis is normal to the surface of the fluid.

Let $\mathbf{g}$ be \htmladdnormallink{The Gravitational Field}{http://planetphysics.us/encyclopedia/GravitationalField.html} (taken to be a constant) and let $\Omega$ denote the submerged region of the body. To obtain the net \htmladdnormallink{force}{http://planetphysics.us/encyclopedia/Thrust.html} of buoyancy $\mathbf{F}_B$ acting on the \htmladdnormallink{object}{http://planetphysics.us/encyclopedia/TrivialGroupoid.html}, we integrate the pressure $p$ over the \htmladdnormallink{boundary}{http://planetphysics.us/encyclopedia/GenericityInOpenSystems.html} of this region \[ \mathbf{F}_B = \int_{\partial\Omega}{-p\mathbf{n}\,dS} \] Where $\mathbf{n}$ is the outward pointing normal to the boundary of $\Omega$. The negative sign is there because pressure points in the direction of the \emph{inward} normal. It is a consequence of \htmladdnormallink{Stokes' theorem}{http://planetphysics.us/encyclopedia/StokesTheorem.html} that for a differentiable \htmladdnormallink{scalar}{http://planetphysics.us/encyclopedia/Vectors.html} \htmladdnormallink{field}{http://planetphysics.us/encyclopedia/CosmologicalConstant2.html} $f$ and for any $\Omega\subset\mathbb{R}^3$ a compact three-manifold with boundary, we have \[ \int_{\partial\Omega}{f\mathbf{n}\,dS} = \int_\Omega{\nabla f\,dV} \] therefore we can write \[ \mathbf{F}_B = -\int_\Omega{\nabla p\, dV} \] Now, it turns out that $\nabla p = \rho_f\mathbf{g}$ where $\rho_f$ is the \htmladdnormallink{volume}{http://planetphysics.us/encyclopedia/Volume.html} density of the fluid. Here is why. Imagine a cubical element of fluid whose height is $\Delta z$, whose top and bottom surface area is $\Delta A$ (in the $x-y$ plane), and whose mass is $\Delta m$. Let us consider the forces acting on the bottom surface of this fluid element. Let the z-coordinate of its bottom surface be $z$. Then, there is an upward force equal to $p(z)\Delta A\mathbf{e}_z$ on its bottom surface and a downward force of $-p(z + \Delta z)\Delta A\mathbf{e}_z + \Delta m\mathbf{g}$. These forces must balance so that we have \[ p(z)\Delta A = p(z + \Delta z)\Delta A - \Delta m|\mathbf{g}| \] a simple manipulation of this equation along with dividing by $\Delta z$ gives \[ \frac{p(z + \Delta z) - p(z)}{\Delta z} = \frac{\Delta m}{\Delta A\Delta z}|\mathbf{g}| = \frac{\rho_f \Delta A\Delta z}{\Delta A\Delta z}|\mathbf{g}| = \rho_f |\mathbf{g}| \] taking the limit $\Delta z \to 0$ gives \[ \frac{\partial p}{\partial z} = \rho_f|\mathbf{g}| \] Similar arguments for the $x$ and $y$ directions yield \[ \frac{\partial p}{\partial x} = \frac{\partial p}{\partial y} = 0 \] putting this all together we obtain $\nabla p = \rho_f\mathbf{g}$ as desired. Substituting this into the integral expression for the buoyant force obtained above using Stokes' theorem, we have \[ \mathbf{F}_B = -\int_\Omega{\rho_f\mathbf{g}\, dV} = -\rho_f\mathbf{g}\int_\Omega{dV} = -\rho_f\mathbf{g}\text{Vol}(\Omega) \] where we can pull $\rho_f$ and $\mathbf{g}$ outside of the integral since they are assumed to be constant. But notice that $\rho_f\text{Vol}(\Omega)$ is equal to $M_d$, the mass of the displaced fluid so that \[ \mathbf{F}_B = -M_d\mathbf{g} \] But by Newton's second law, the buoyant force must balance the weight of the object which is given by $M \mathbf{g}$. It follows from the above expression for the buoyant force that \[ M_d = M \] which is precisely the statement of Archimedes' Principle.

\end{document}