The energy distribution in a static spherically symmetric nonsingular black hole space-time

We calculate the energy distribution in a static spherically symmetric nonsingular black hole space-time by using the Tolman's energy-momentum complex. All the calculations are performed in quasi-Cartesian coordinates. The energy distribution is positive everywhere and equal to zero at the origin. Mie get the same result as obtained by I.-C. Yang by using the Einstein's and Weinberg's prescriptions.