LaTeX Exercise 1

The images of the equations on this page were taken from the Wikipedia pages referenced for each equation.

Imports


In [56]:
from IPython.display import Image

Typesetting equations

In the following cell, use Markdown and LaTeX to typeset the equation for the probability density of the normal distribution $f(x, \mu, \sigma)$, which can be found here. Following the main equation, write a sentence that defines all of the variable in the equation.


In [57]:
Image(filename='normaldist.png')


Out[57]:
\begin{equation*} f(x, \mu, \sigma) = \frac{1}{\sigma \sqrt{2\pi}} e^-\frac{(x-\mu)^2}{2\sigma^2} \end{equation*}

Here, $\mu$ is the mean or expectation of the distribution (and also its median and mode). The parameter $\sigma$ is its standard deviation. $x$ is the value in the normal distribution.

In the following cell, use Markdown and LaTeX to typeset the equation for the time-dependent Schrodinger equation for non-relativistic particles shown here (use the version that includes the Laplacian and potential energy). Following the main equation, write a sentence that defines all of the variable in the equation.


In [58]:
Image(filename='tdseqn.png')


Out[58]:
\begin{equation*} i \bar{h} \frac{\partial}{\partial t} \Psi(r,t) = \left[(\frac{{-\bar{h}^2}}{2 \mu} \nabla^2 + V(r,t) \right] \psi(r,t) \end{equation*}

$\mu$ is the particle's "reduced mass", $V$ is its potential energy, $\Delta$ is the Laplacian (a differential operator), and $\Psi$ is the wave function (more precisely, in this context, it is called the "position-space wave function").

In the following cell, use Markdown and LaTeX to typeset the equation for the Laplacian squared ($\Delta=\nabla^2$) acting on a scalar field $f(r,\theta,\phi)$ in spherical polar coordinates found here. Following the main equation, write a sentence that defines all of the variable in the equation.


In [59]:
Image(filename='delsquared.png')


Out[59]:
\begin{equation*} \Delta f = \frac{1}{r^2} \frac{\partial}{\partial r}\left(r^2 \frac{\partial f}{\partial r} \right) + \frac{1}{r^2 sin\theta}\frac{\partial}{\partial \theta} \left(sin\theta\frac{\partial f}{\partial \theta}\right) + \frac{1}{r^2sin^2\theta}\frac{\partial^2f}{\partial\varphi^2} \end{equation*}

In this equation, $\varphi$ represents the azimuthal angle and $\theta$ the zenith angle or co-latitude.


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