Black hole formation in the grazing collision of high-energy particles

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dc.creatorYoshino, Hirotaka
dc.creatorNambu, Yasusada
dc.date2002-09-02
dc.date.accessioned2026-07-07T10:48:11Z
dc.date.available2026-07-07T10:48:11Z
dc.descriptionWe numerically investigate the formation of D-dimensional black holes in high-energy particle collision with the impact parameter and evaluate the total cross section of the black hole production. We find that the formation of an apparent horizon occurs when the distance between the colliding particles is less than 1.5 times the effective gravitational radius of each particles. Our numerical result indicates that although both the one-dimensional hoop and the (D-3)-dimensional volume corresponding to the typical scale of the system give a fairly good condition for the horizon formation in the higher-dimensional gravity, the (D-3)-dimensional volume provide a better condition to judge the existence of the horizon.
dc.description13 pages, 6 figures
dc.identifierhttps://arxiv.org/abs/gr-qc/0209003
dc.identifierhttp://arxiv.org/abs/gr-qc/0209003
dc.identifierPhys.Rev.D67:024009,2003
dc.identifierdoi:10.1103/PhysRevD.67.024009
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/183789
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectHigh Energy Physics - Theory
dc.titleBlack hole formation in the grazing collision of high-energy particles
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