LaTeX Exercise 1

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

Imports


In [4]:
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 [2]:
Image(filename='normaldist.png')


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

$\mu$ is the mean of the distribution and $\sigma$ is the standard deviation.

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 [3]:
Image(filename='tdseqn.png')


Out[3]:
$$\begin{align} i\hbar\frac{\partial}{\partial{t}}\Psi(r,t)=\left[\frac{-\hbar^2}{2\mu}\nabla^2+V(r,t)\right]\Psi(r,t) \end{align}$$

$\hbar$ is Planck's constant over $2\pi$. This is multiplied by the partial derivitave of the wave function $\Psi$ with respect to time. $\mu$ is the particle's mass. $V$ is the potential energy and $\nabla^2$ is the Laplacian

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 [5]:
Image(filename='delsquared.png')


Out[5]:
$$\begin{align} \Delta f=\frac{1}{r^2}\frac{\partial}{\partial r}\left(r^2 \frac{\partial f}{\partial r}\right) +\frac{1}{r^2 \sin\theta}\frac{\partial}{\partial \theta}\left(\sin\theta\frac{\partial f}{\partial\theta}\right)+\frac{1}{r^2\sin^2\theta}\frac{\partial^2 f}{\partial\varphi^2} \end{align}$$

$r$ is the distance from the origin, radius, $\theta$ is the angle in the xy plane from the x axis, and $\varphi$ is the angle from the z axis.


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