Brane-world black hole entropy from modified dispersion relations
arXiv:1007.4904 · doi:10.1016/j.physletb.2010.07.051
Abstract
The entropy of the Reissner-Nördstrom black hole is studied within the context of a brane-world scenario. Such a black hole is a solution of the Einstein field equations on the brane, possessing a tidal charge which is a reflection of the extra dimension. We use the modified dispersion relation to obtain the entropy of such brane-world black holes. The resulting entropy differs from that of the standard Bekenstein-Hawking's and contains information on the extra dimension.
9 pages, 4 figures, to appear in PLB
References in corpus (6)
- Modified dispersion relations and black hole physics
- Entropy of the Randall-Sundrum brane world with the generalized uncertainty principle
- On the Existence of the Logarithmic Correction Term in Black Hole Entropy-Area Relation
- Brane-World Black Hole Solutions via a Confining Potential
- The Physics of Information
- Entropy of the Randall-Sundrum black brane world to all orders in the Planck length
Cited by in corpus (9)
- Modified dispersion relations in extra dimensions
- Black Holes with MDRs and Bekenstein-Hawking and Perelman Entropies for Finsler-Lagrange-Hamilton Spaces
- Physical Properties of Brane-World Black Hole Solutions via a Confining Potential
- Corrections to the Cardy-Verlinde formula from the modified dispersion relation in extra dimensions
- Radiation of Charged Black Holes and Modified Dispersion Relation
- A possible cosmological application of some thermodynamic properties of the black body radiation in dimensional Euclidean spaces
- Quantum corrections for a black hole in an asymptotically safe gravity with higher derivatives
- Quantum Corrections for a Braneworld Black Hole
- Probing dynamical embeddings in a five-dimensional spacetime in light of DESI BAO