Theoretical survey of tidal-charged black holes at the LHC
arXiv:0911.1884 · doi:10.1007/JHEP02(2010)079
Abstract
We analyse a family of brane-world black holes which solve the effective four-dimensional Einstein equations for a wide range of parameters related to the unknown bulk/brane physics. We first constrain the parameters using known experimental bounds and, for the allowed cases, perform a numerical analysis of their time evolution, which includes accretion through the Earth. The study is aimed at predicting the typical behavior one can expect if such black holes were produced at the LHC. Most notably, we find that, under no circumstances, would the black holes reach the (hazardous) regime of Bondi accretion. Nonetheless, the possibility remains that black holes live long enough to escape from the accelerator (and even from the Earth's gravitational field) and result in missing energy from the detectors.
RevTeX4, 12 pages, 4 figures, 5 tables, minor changes to match the accepted version in JHEP
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Cited by in corpus (13)
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- Large extra dimensions and small black holes at the LHC
- Minimum length effects in black hole physics
- Microcanonical description of (micro) black holes
- Circular Geodesics in Tidal Charged Black Hole
- Distorted 5-dimensional vacuum black hole
- Brane-world black holes and the scale of gravity
- Exploring the bulk of tidal charged micro-black holes
- Production of tidal-charged black holes at the Large Hadron Collider
- Quantum Black Holes from Cosmic Rays
- Affect of brane thickness on microscopic tidal-charged black holes
- Minimum black hole mass from colliding Gaussian packets
- Generalized three body problem and the instability of the core-halo objects in binary systems