LaTeX Exercise 1

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

Imports


In [2]:
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 [3]:
Image(filename='normaldist.png')


Out[3]:
\begin{equation*} f(x,\mu,\sigma)=\frac{1}{\sigma \sqrt{2 \pi}}e^{-\frac{(x-\mu)^2}{2\sigma^2}} \end{equation*}

This function defines the normal distribution where $\mu$ represents the mean value, $\sigma$ represents the standard of deviation, and x is a variable

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 [4]:
Image(filename='tdseqn.png')


Out[4]:
\begin{equation*} i\hbar \frac{\delta}{\delta t}\psi(r,t) = [\frac{-\hbar^2}{2\mu}\bigtriangledown^2 + V(r,t)] \psi(r,t) \end{equation*}

This function represents the time dependent Schrodinger equation for non-relativistic particles. $\mu$ is the reduced mass, V is potential energy $\bigtriangledown^2$ is the laplacian, $\psi$ is the 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 [5]:
Image(filename='delsquared.png')


Out[5]:
\begin{equation*} \bigtriangleup f = \frac{1}{r^2}\frac{\delta}{\delta r}\Biggr(r^2 \frac{\delta f}{\delta r} \Biggr) + \frac{1}{r^2 sin \theta} \frac {\delta}{\delta \theta} \Biggr( sin \theta \frac{\delta f}{\delta \theta} \Biggr) + \frac{1}{r^2 sin^2 \theta} \frac {\delta^2 f}{\delta \varphi ^2} \end{equation*}

This is the equation of the Laplacian squared acting on a scalar field in spherical polar coordinates. $ \theta$ represents the andgle, r represents the distance in the polar coordinate system


In [ ]: