  We derive the Hawking spectrum of fermions emitted by a minimally geometric
deformed (MGD) black hole. The MGD naturally describes quantum effects on the
geometry in the form of a length scale related, for instance, to the existence
of extra dimensions. The dynamics of the emitted fermions is described in the
context of the generalised uncertainty principle and likewise contains a length
scale associated with the quantum nature of space-time. We then show that the
emission is practically indistinguishable from the Hawking thermal spectrum for
large black hole masses, but the total flux can vanish for small and finite
black hole mass. This suggests the possible existence of black hole remnants
with a mass determined by the two length scales.
