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diff --git a/mindmap/electrostatics.org b/mindmap/electrostatics.org new file mode 100644 index 0000000..e71a05e --- /dev/null +++ b/mindmap/electrostatics.org @@ -0,0 +1,97 @@ +:PROPERTIES: +:ID: 32f0b8b1-17bc-4c91-a824-2f2a3bbbdbd1 +:END: +#+title: electrostatics +#+author: Preston Pan +#+html_head: <link rel="stylesheet" type="text/css" href="../style.css" /> +#+html_head: <script src="https://polyfill.io/v3/polyfill.min.js?features=es6"></script> +#+html_head: <script id="MathJax-script" async src="https://cdn.jsdelivr.net/npm/mathjax@3/es5/tex-mml-chtml.js"></script> +#+options: broken-links:t + +* What is Electricity? +Because this is an introduction and not a lesson in quantum mechanics, I will say that electricity is broadly +defined by the charge that an object has that corresponds the force that it both feels and also gives +to other objects. Charge is measured in coulombs and can be negative or positive, which leads us to the man himself: + +* Coulomb's Law +In order to define the phenomena of electric force in the real world, we use +this experimentally verified law known as Coulomb's Law. Let \( \vec{r_{1}} \) be the displacement +of a charge \( Q \), and let \( \vec{r_{2}} \) be the displacement of a charge \( q \), where these two charges are named \( P_{1}\) and \( P_{2} \) respectively. +Then let \( \vec{r} = \vec{r_{1}} - \vec{r_{2}} \) be the distance between the charges. For simplicity, we assume +these charges have no mass or volume; we call these /point charges/. The equation for the force +on \( P_{1} \) is as follows: + +\begin{align*} +\vec{F(\vec{r})} = \frac{1}{4\pi\epsilon_{0}}\frac{qQ}{r^{2}} \hat{r}. +\end{align*} + +Where \( \hat{r} \) is the unit vector pointing in the direction of \( P_{2} \). Note that there are a +couple of interesting things about this force. First, it is an inverse square law, and the formula looks a lot like the one for gravitation, +only charge can be negative and mass cannot. Second, it is symmetrical, +in the sense that the force felt by \( P_{2} \) is going to be the same, only \( \hat{r} \) +is pointing in the other direction. Also, note that due to linearity, this force calculation follows the /superposition principle/. +That is, if we have different electrostatic forces acting on one particle: + +\begin{align*} +\vec{F_{tot}} = \vec{F_{1}} + \vec{F_{2}} + … = \sum_{i=1}^{n} \vec{F_{i}}. +\end{align*} + +Wait, where does the \( \frac{1}{4\pi\epsilon_{0}} \) term come from? Well, the surface area of a sphere +is \( 4\pi r^{2}\) , which explains both the inverse square law and this \( 4\pi \) term in the denominator, +but what about \( \epsilon_{0} \), what does it even mean? + +Well, it is simply a conversion of units from /speed of light/ terms to /SI unit terms/. If you +think of it like that, you will never need to know what the units actually are, although I'm +sure you can find that online. Just know that it is called the permeability of free space, and +it is defined in terms of the speed of light and a constant relating to magnetism: + +\begin{align*} +\epsilon_{0}\mu_{0} = \frac{1}{c^{2}} +\end{align*} + +but since this is electrostatics and not electrodynamics, you will not have to worry about +magnetic constants. Again, it is just a shift from speed of light units to our mortal units. + +** Electric Field +Okay, now we can continue to defining the /electric field/ of a particle. Let's call \( P_{1} \) our +/test charge/, and \( P_{2} \) our /source charge/. If we now want to measure the force on \( P_{1} \), +our equation is going to be the same. However, we can define a field \( \vec{E(\vec{r})} \) such that: + +\begin{align*} +\vec{F} = Q\vec{E} +\end{align*} + +Where: + +\begin{align*} +\vec{E} = \frac{\vec{F}}{Q} +\end{align*} + +Therefore, the value of \( \vec{E} \) for a point charge must be: + +\begin{align*} +\vec{E} := \frac{1}{4\pi\epsilon_{0}}\frac{q}{r^{2}}\hat{r}. +\end{align*} + +The result is we find a way to express force in a /test charge independent way/. This is useful +because we often want to find the force if an arbitrary object with an arbitrary charge is next +to the particle in question, instead of focusing specifically on two charges. + +Note that it is trivial to prove that \( \vec{E} \) also follows the superposition principle. + + +** Continuous Charge Distributions +Now that we have a working definition of \( \vec{E} \), we can now find the electric field of an object +that has a continuous charge distribution. Note that there aren't actually infinite charges in real +world objects which is what we are assuming by taking an integral over some space of charge, but +it's close enough because there are so many individual charges in real world objects. Assuming we are in +three dimensions: + +\begin{align*} +\vec{E(\vec{r})} = \frac{1}{4\pi\epsilon_{0}} \int_{space} \frac{\sigma(\vec{r_{2}})}{r^{2}}\hat{r}d\tau +\end{align*} + +Where \( \tau \) is the patch of volume we are integrating over, and \( \sigma \) is the charge density function, +which takes a position vector and returns the charge at that vector. Of course, surface and line integrals +have their own analogues -- simply replace \( d\tau \) with \( da \) or \( dl \), and make sure your charge +distribution is in the correct amount of dimensions. |