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Black holes at the IceCube neutrino telescope

2006/10/31 by Luis A. Anchordoqui, Matthew M. Glenz, Leonard Parker
Physics and Astronomy · #Astrophysics #Astrophysics and Cosmic Phenomena #Black Holes and Theoretical Physics #Black hole (networking) #Cosmology and Gravitation Theories #Gravitational wave #Hawking radiation #Micro black hole #Neutrino #Particle physics #Physics #hep-ph

paper · pdf · doi:10.1103/physrevd.75.024011

published as Phys.Rev.D75:024011,2007 · Matching version to be published in Phys. Rev. D

arxiv created 2006/12/14 · openalex publication_date 2007/01/09 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

If the fundamental Planck scale is about a TeV and the cosmic neutrino flux is at the Waxman-Bahcall level, quantum black holes are created daily in the Antarctic ice cap. We reexamine the prospects for observing such black holes with the IceCube neutrino-detection experiment. To this end, we first revise the black hole production rate by incorporating the effects of inelasticty, i.e., the energy radiated in gravitational waves by the multipole moments of the incoming shock waves. After that we study in detail the process of Hawking evaporation accounting for the black hole's large momentum in the lab system. We derive the energy spectrum of the Planckian cloud which is swept forward with a large, O(106), Lorentz factor. (It is noteworthy that the boosted thermal spectrum is also relevant for the study of near-extremal supersymmetric black holes, which could be copiously produced at the Large Hadron Collider.) In the semiclassical regime, we estimate the average energy of the boosted particles to be less than 20% the energy of the \ensuremathν progenitor. Armed with such a constraint, we determine the discovery reach of IceCube by tagging on soft (relative to what one would expect from charged current standard model processes) muons escaping the electromagnetic shower bubble produced by the black hole's light descendants. The statistically significant 5\ensuremathσ excess extends up to a quantum gravity scale \ensuremath∼1.3 TeV.

Citations