Energy Distribution in 2d Stringy Black Hole Backgrounds
arXiv:gr-qc/0303009 · doi:10.1142/S0217751X03015969
Abstract
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.
17 pages, LaTeX, v2: acknowledgements added, to appear in Int.J.Mod.Phys.A