  In the tunneling framework of Hawking radiation, charged massive particle's
tunneling in charged non-rotating TeV-Scale black hole is investigated. To this
end, we consider natural cutoffs as a minimal length, a minimal momentum, and a
maximal momentum through a generalized uncertainty principle. We focus on the
role played by these natural cutoffs on the luminosity of charged non-rotating
micro black hole by taking into account the full implications of energy and
charge conservation as well as the back- scattered radiation.
