  We investigate the effects of a modified dispersion relation proposed by
Majhi and Vagenas on the Reissner-Nordstrom black hole thermodynamics in a
universe with large extra dimensions. It is shown that entropy, temperature and
heat capacity receive new corrections and charged black holes in this framework
have less degrees of freedom and decay faster compared to black holes in the
Hawking picture. We also study the emission rate of black hole and compare our
results with other quantum gravity approaches. In this regard, the existence of
the logarithmic prefactor and the relation between dimensions and charge are
discussed. This procedure is not only valid for a single horizon spacetime but
it is also valid for the spacetimes with inner and outer horizons.
