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The energy and momentum distributions in the dyadosphere of aReissner-Nordstrom black hole are evaluated. The Moller's energy-momentumcomplex is employed for this computation. The spacetime under study is modifieddue to the effects of vacuum fluctuations in the dyadosphere. Therefore, thecorrected Reissner-Nordstrom black hole metric takes into account the firstcontribution of the weak field limit of one-loop QED. Furthermore, a comparisonand a consequent connection between our results that those already existing inthe literature is provided. We hypothesize that when the energy distribution isof specific form there is a relation that connects the coefficients in theEinstein's prescription with those in the Moller's prescription.Comment: 12 pages, no figure, LaTe

ENERGY DISTRIBUTION IN THE DYADOSPHERE OF A REISSNER–NORDSTRÖM BLACK HOLE IN MØLLER'S PRESCRIPTION