Energy Distribution in 2d Stringy Black Hole Backgrounds

Details Energy Distribution in 2d Stringy Black Hole Backgrounds Energy Distribution in 2d Stringy Black Hole Backgrounds

2003-03-03

arxiv.org/abs/gr-qc/0303009v2

Int.J.Mod.Phys. A18 (2003) 5781-5794

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

17 pages, LaTeX, v2: acknowledgements added, to appear in Int.J.Mod.Phys.A

Scientific paper

10.1142/S0217751X03015969

We utilize Moller's and Einstein's energy-momentum complexes in order to explicitly evaluate the energy distributions associated with the two-dimensional "Schwarzschild" and "Reissner-Nordstrom" black hole backgrounds. While Moller's prescription provides meaningful physical results, Einstein's prescription fails to do so in the aforementioned gravitational backgrounds. These results hold for all two-dimensional static black hole geometries. The results obtained within this context are exploited in order Seifert's hypothesis to be investigated.

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