Energy of a Regular Black Hole

Abstract

We use Einstein, Landau-Lifshitz, Papapetrou and Weinberg energy-momentum complexes to evaluate energy distribution of a regular black hole. It is shown that for a regular black hole, these energy-momentum complexes give the same energy distribution. This supports Cooperstock hypothesis and also Aguirregabbiria et al. conclusions. Further, we evaluate energy distribution using M$\ddot{o}$ller's prescription. This does not exactly coincide with ELLPW energy expression but, at large distances, they become same.