Autori: I. Radinschi

Editorial: Modern Physics Letters A, 15, p.803-807, 2000.

Rezumat:

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 be equal to zero at origin. We get the same result as obtained by Y-Ching Yang by using the Einstein’s and Weinberg’s prescriptions.

Cuvinte cheie: distributie de energie, gaura neagra // energy distribution, black hole

URL: http://xxx.lanl.gov