| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 8187941 | Physics Letters B | 2013 | 5 Pages |
Abstract
We propose a derivation for computing black hole entropy for spherical non-rotating isolated horizons from loop quantum gravity in four and higher dimensions. The state counting problem effectively reduces to the well studied 3+1-dimensional one based on an SU(2)-Chern-Simons theory, differing only in the precise form of the area spectrum.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
Authors
N. Bodendorfer,