arXiv · hep-th/9611189
Radiation from a class of string theoretic black holes
Abstract
The emission of a scalar with low energy $ω$, from a $D (4\le D\le 8 )$ dimensional black hole with n charges is studied in both string and semiclassical calculations. In the lowest order in $ω$, the weak coupling string and semiclassical calculations agree provided that the Bekenstein--Hawking formula is valid and the effective central charge $c_{eff}=6$ for any D. When the next order in $ω$ is considered however, there is no agreement between the two schemes unless D=5, n=3 or D=4, n=4.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
S. P. de Alwis, K. Sato. 1996-11-22. Radiation from a class of string theoretic black holes. https://doi.org/10.1103/physrevd.55.6181
Cite the original work for its findings. Save a collection to share your selection of sources.