Energy Distribution in 2d Stringy Black Hole Backgrounds

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