The images of the equations on this page were taken from the Wikipedia pages referenced for each equation.
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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.
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Image(filename='normaldist.png')
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$\mu$ 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.
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Image(filename='tdseqn.png')
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$\hbar$ 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.
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Image(filename='delsquared.png')
Out[5]:
$r$ 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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