  Primordial Black Holes (PBHs) are candidates for dark matter as well as
ultra-high energy cosmic rays. PBHs are speculated to exist over a large range
of masses, from below $10^{15}$ g to $10^3$ M$_\odot$. Here we search for PBHs
with an initial mass of $\sim 10^{15}$ g. Hawking radiation by black holes of
this initial mass predicts their evaporation at present time. PBHs are expected
to produce copious amounts of high-energy neutrinos and gamma rays right before
evaporating. Gamma-ray instruments such as Fermi, VERITAS, HAWC, HESS, and
Milagro have conducted searches for evaporating PBHs during their last second
to a year of existence. They are able to detect bursts from PBHs in a range of
$10^{-3}$ to $0.1$ pc. We present sensitivity to PBH evaporation using one year
of neutrino data by IceCube. In these proceedings, we detail the changes to
adapt IceCube's standard neutrino flare search, aka time-dependent point source
search, into one that is appropriate for evaporating BHs. These proceedings
serve as proof of concept for a first-ever search for evaporating PBHs using
neutrinos that can use 10 years of IceCube data.
