Braneworld Black Holes and Entropy Bounds
arXiv:1706.04434 · doi:10.1016/j.physletb.2017.11.061
Abstract
The Bousso's D-bound entropy for the various possible black hole solutions on a 4-dimensional brane is checked. It is found that the D-bound entropy here is apparently different from that of obtained for the 4-dimensional black hole solutions. This difference is interpreted as the extra loss of information, associated to the extra dimension, when an extra-dimensional black hole is moved outward the observer's cosmological horizon. Also, it is discussed that N-bound entropy is hold for the possible solutions here. Finally, by adopting the recent Bohr-like approach to black hole quantum physics for the excited black holes, the obtained results are written also in terms of the black hole excited states.
13 pages, accepted for publication in Physics Letters B
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- D-bound and Bekenstein bound for McVittie solution surrounded by dark energy cosmological fields
- Massive gravity solution of Black Holes and Entropy Bounds
- Thermodynamic Topology and Photon Spheres Analysis of Black Holes in Brane-World: Insights from Barrow Entropy
- (2+1)-dimensional f(R) gravity solutions via Hojman symmetry
- D-bound and Bekenstein Bound for the Surrounded Vaidya Black Hole
- Scalar field propagation in braneworld black hole scenario obtained from Nash theorem