The images of the equations on this page were taken from the Wikipedia pages referenced for each equation.
In [2]:
from IPython.display import Image
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]:
Where $\mu$ is the mean or expectaion 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 [4]:
Image(filename='tdseqn.png')
Out[4]:
where $r$ is radius, $t$ is time, $\hbar$ is plank's constant divided by 2$\pi$, $\mu$ is the particle's reduced mass, $V(r,t)$ is the particle's potential energy, $\nabla^2$ is the Laplacian (differential opperator), and $\Psi(r,t)$ 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]:
Where $\Delta = \nabla^2$ acting on a scalar field in spherical cooridnates, $r$ represents the radius, $\psi$ is the azimuthal angle and $\theta$ is the zenith angle/co-latitude.