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We give three different spherically symmetric spacetimes for the coupledgravitational and electromagnetic fields with charged source in the tetradtheory of gravitation. One of these, contains an arbitrary function andgenerates the others. These spacetimes give the Reissner Nordstr$\ddot{o}$mmetric black hole. We then, calculated the energy associated with thesespacetimes using the superpotential method. We find that unless the time-spacecomponents of the tetrad field go to zero faster than ${1/\sqrt{r}}$ atinfinity, one gets different results for the energy.Comment: 12 pages tex fil

REISSNER–NORDSTRÖM SOLUTIONS AND ENERGY IN TELEPARALLEL THEORY