Renormalization group improved black hole space-time in large extra dimensions
arXiv:0912.4517 · doi:10.1134/S0021364010160010
Abstract
By taking into account a running of the gravitational coupling constant with an ultra violet fixed point, an improvement of classical black hole space-times in extra dimensions is studied. It is found that the thermodynamic properties in this framework allow for an effective description of the black hole evaporation process. Phenomenological consequences of this approach are discussed and the LHC discovery potential is estimated.
13 pages, 6 figures
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- Black hole shadow of a rotating scale--dependent black hole
- A scale dependent black hole in three-dimensional space-time
- Scale-dependent (2+1) - dimensional electrically charged black holes in Einstein-power-Maxwell theory
- Scale-dependent rotating BTZ black hole
- Non-Singular Black Holes, the Cosmological Constant and Asymptotic Safety
- Black Holes in Asymptotically Safe Gravity
- Cosmological constant problem: deflation during inflation
- Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes