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]:
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]:
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]:
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 [ ]: