  We consider the Hawking radiation by the tunneling of charged fermions and
charged scalar particles from the five-dimensional charged static squashed
Kaluza-Klein black hole based on the generalized uncertainty principle. We
derive corrections of the Hawking temperature to general relativity, which are
related to the energy of the emitted particle, the size of the extra dimension,
the charge of the black hole and the quantum effect predicted by the
generalized uncertainty principle. It is shown that the quantum correction may
slow down the increase of the Hawking temperature, which may lead to the
thermodynamic stable remnant after the evaporation of the squashed Kaluza-Klein
black hole.
