  The effect of Lorentz symmetry breaking (LSB) on the Hawking radiation of
Schwarzschild-like black hole found in the bumblebee gravity model (SBHBGM) is
studied in the framework of quantum gravity. To this end, we consider Hawking
radiation spin-0 (bosons) and spin-$\frac{1}{2}$ particles (fermions), which go
in and out through the event horizon of the SBHBGM. We use the modified
Klein-Gordon and Dirac equations, which are obtained from the generalized
uncertainty principle (GUP) to show how Hawking radiation is affected by the
GUP and LSB. In particular, we reveal that, independent of the spin of the
emitted particle, GUP causes a change in the Hawking temperature of the SBHBGM.
Furthermore, we compute the semi-analytic greybody factors (for both bosons and
fermions) of the SBHBGM. Thus, we reveal that LSB is effective on the greybody
factor of the SBHBGM such that its redundancy decreases the value of the
greybody factor. Our findings are graphically depicted.
