Uncertainties in limits on TeV-gravity from neutrino-induced showers
arXiv:hep-ph/0312249 · doi:10.1016/j.astropartphys.2004.06.008
Abstract
In models with TeV-scale gravity, ultrahigh energy cosmic rays can generate microscopic black holes in the collision with atmospheric and terrestrial nuclei. It has been proposed that stringent bounds on TeV-scale gravity can be obtained from the absence of neutrino cosmic ray showers mediated by black holes. However, uncertainties in the cross section of black hole formation and, most importantly, large uncertainties in the neutrino flux affects these bounds. As long as the cosmic neutrino flux remains unknown, the non-observation of neutrino induced showers implies less stringent limits than present collider limits.
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References in corpus (4)
Cited by in corpus (22)
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- Exact Results for Evaporating Black Holes in Curvature-Squared Lovelock Gravity: Gauss-Bonnet Greybody Factors
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- Brane Decay of a (4+n)-Dimensional Rotating Black Hole. III: spin-1/2 particles
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- TeV gravity at neutrino telescopes
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- Black Holes at the IceCube Neutrino Telescope
- Hawking evaporation of cosmogenic black holes in TeV-gravity models
- Bounds on Low Scale Gravity from RICE data and Cosmogenic Neutrino Flux Models
- Discriminating Supersymmetry and Black Holes at the Large Hadron Collider
- QCD and spin effects in black hole airshowers
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