The Energy Distribution in a Static Spherically Symmetric Nonsingular Black Hole Space-Time

Details The Energy Distribution in a Static Spherically Symmetric Nonsingular Black Hole Space-Time The Energy Distribution in a Static Spherically Symmetric Nonsingular Black Hole Space-Time

2000-08-14

arxiv.org/abs/gr-qc/0008029v1

Mod.Phys.Lett. 15 (2000) 803-807

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

5 pages, no figures

Scientific paper

10.1142/S0217732300000785

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.

Affiliated with

Also associated with

No associations

Rating

The Energy Distribution in a Static Spherically Symmetric Nonsingular Black Hole Space-Time does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The Energy Distribution in a Static Spherically Symmetric Nonsingular Black Hole Space-Time, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Energy Distribution in a Static Spherically Symmetric Nonsingular Black Hole Space-Time will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-395052