  The energy and momentum distributions in the dyadosphere of a
Reissner-Nordstrom black hole are evaluated. The Moller's energy-momentum
complex is employed for this computation. The spacetime under study is modified
due to the effects of vacuum fluctuations in the dyadosphere. Therefore, the
corrected Reissner-Nordstrom black hole metric takes into account the first
contribution of the weak field limit of one-loop QED. Furthermore, a comparison
and a consequent connection between our results that those already existing in
the literature is provided. We hypothesize that when the energy distribution is
of specific form there is a relation that connects the coefficients in the
Einstein's prescription with those in the Moller's prescription.
