  The original derivation of Hawking radiation shows the complete evaporation
of black holes. However, theories of quantum gravity predict the existence of
the minimal observable length. In this paper, we investigate the tunneling
radiation of the scalar particles by introducing quantum gravity effects
influenced by the generalized uncertainty principle. The Hawking temperatures
are not only determined by the properties of the black holes, but also affected
by the quantum numbers of the emitted particles. The quantum gravity
corrections slow down the increase of the temperatures. The remnants are found
during the evaporation.
