  In June 2015 the Large Hadron Collider was able to produce collisions with an
energy of 13TeV, where collisions at these energy levels may allow for the
formation of higher dimensional black holes. In order to detect these higher
dimensional black holes we require an understanding of their emission spectra.
One way of determining this is by looking at the absorption probabilities
associated with the black hole. In this proceedings we will look at the
absorption probability for spin-3/2 particles near $N$-dimensional
Schwarzschild black holes. We will show how the Unruh method is used to
determine these probabilities for low energy particles. We then use the
Wentzel-Kramers-Brillouin approximation in order to determine these absorption
probabilities for the entire possible energy range.
