QCD and spin effects in black hole airshowers

Simple item page
dc.creatorCavaglia, Marco
dc.creatorRoy, Arunava
dc.date2007-07-02
dc.date.accessioned2026-07-07T11:17:25Z
dc.date.available2026-07-07T11:17:25Z
dc.descriptionIn models with large extra dimensions, black holes may be produced in high-energy particle collisions. We revisit the physics of black hole formation in extensive airshowers from ultrahigh-energy cosmic rays, focusing on collisional QCD and black hole emissivity effects. New results for rotating black holes are presented. Monte Carlo simulations show that QCD effects and black hole spin produce no observable signatures in airshowers. These results further confirm that the main characteristics of black hole-induced airshowers do not depend on the fine details of micro black hole models.
dc.description6 pages, 2 figures, accepted for publication in Physical Review D
dc.identifierhttps://arxiv.org/abs/0707.0274
dc.identifierhttp://arxiv.org/abs/0707.0274
dc.identifierPhys.Rev.D76:044005,2007
dc.identifierdoi:10.1103/PhysRevD.76.044005
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/193002
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleQCD and spin effects in black hole airshowers
dc.typetext

Files

Collections

arXiv