LaTeX Exercise 1

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

Imports


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

The above equation is the probability density for x, where $\mu$ represents the mean of the distribution, and $\sigma$ is the standard deviation with $\sigma^{2}$ being the variance.

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{equation*} i\bar{h}\frac{\partial}{\partial t} \Psi (\mathbf{r},t) = \left[\frac{-h^{2}}{2\mu}\Delta^{2} + V(\mathbf{r},t)\right]\Psi(\mathbf{r},t) \end{equation*}

In the above equation i is an imaginary unit, $\bar{h}$ is placks constant divided by 2$\pi$, $\Psi$ is the quantum wave function of the system, $\mu$ is the reduced mass, $\Delta^{2}$ is the Laplace operator, and V is the potential energy.

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 [4]:
Image(filename='delsquared.png')


Out[4]:
\begin{equation*} \Delta f =\frac{1}{r^{2}}\frac{\partial}{\partial r} \left(r^{2} \frac{\partial}{\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{equation*}

In the above equation $\theta$ represents is the zenith angle and $\varphi$ is the azimuthal angle


In [ ]: