Journal
MODERN PHYSICS LETTERS A
Volume 15, Issue 11-12, Pages 803-807Publisher
WORLD SCIENTIFIC PUBL CO PTE LTD
DOI: 10.1142/S0217732300000785
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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.
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