  In this paper, we investigate effects of the minimal length on quantum
tunnelling from spherically symmetric black holes using the Hamilton-Jacobi
method incorporating the minimal length. We first derive the deformed
Hamilton-Jacobi equations for scalars and fermions, both of which have the same
expressions. The minimal length correction to the Hawking temperature is found
to depend on the black hole's mass and the mass and angular momentum of emitted
particles. Finally, we calculate a Schwarzschild black hole's luminosity and
find the black hole evaporates to zero mass in infinite time.
