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Energy Distribution in 2d Stringy Black Hole Backgrounds

Elias C. Vagenas
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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.

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BibTeXRIS

Elias C. Vagenas. 2003-06-12. Energy Distribution in 2d Stringy Black Hole Backgrounds. https://doi.org/10.1142/s0217751x03015969

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