Energy of a regular charged black hole solution in Einstein-nonlinear electrodynamics

In this paper we calculate the energy-momentum for a (3+1)-dimensional spherically symmetric, static and charged, regular black hole solution recently constructed in the context of general relativity coupled to nonlinear electrodynamics. The calculations are performed by applying the Einstein and M{\o}ller energy-momentum complexes. It is shown that the expressions for the energy distribution depend on the mass M of the regular black hole, the charge q and the radial coordinate r. Further, all the momenta vanish. In the absence of electric charge the energy expressions for the Schwarzschild space-time geometry are obtained.