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Black holes from high-energy beam--beam collisions

Using a recent technique, proposed by Eardley and Giddings, we extend their results to the high-energy collision of two beams of massless particles, i.e. of two finite-front shock waves. Closed (marginally) trapped surfaces can be determined analytically in several cases even for collisions at non-v...

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Detalles Bibliográficos
Autores principales: Kohlprath, Emmanuel, Veneziano, Gabriele
Lenguaje:eng
Publicado: 2002
Materias:
Acceso en línea:https://dx.doi.org/10.1088/1126-6708/2002/06/057
http://cds.cern.ch/record/544954
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author Kohlprath, Emmanuel
Veneziano, Gabriele
author_facet Kohlprath, Emmanuel
Veneziano, Gabriele
author_sort Kohlprath, Emmanuel
collection CERN
description Using a recent technique, proposed by Eardley and Giddings, we extend their results to the high-energy collision of two beams of massless particles, i.e. of two finite-front shock waves. Closed (marginally) trapped surfaces can be determined analytically in several cases even for collisions at non-vanishing impact parameter in D\ge 4 space-time dimensions. We are able to confirm and extend earlier conjectures by Yurtsever, and to deal with arbitrary axisymmetric profiles, including an amusing case of ``fractal'' beams. We finally discuss some implications of our results in high-energy experiments and in cosmology.
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institution Organización Europea para la Investigación Nuclear
language eng
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spelling cern-5449542021-09-17T03:01:02Zdoi:10.1088/1126-6708/2002/06/057http://cds.cern.ch/record/544954engKohlprath, EmmanuelVeneziano, GabrieleBlack holes from high-energy beam--beam collisionsGeneral Relativity and CosmologyUsing a recent technique, proposed by Eardley and Giddings, we extend their results to the high-energy collision of two beams of massless particles, i.e. of two finite-front shock waves. Closed (marginally) trapped surfaces can be determined analytically in several cases even for collisions at non-vanishing impact parameter in D\ge 4 space-time dimensions. We are able to confirm and extend earlier conjectures by Yurtsever, and to deal with arbitrary axisymmetric profiles, including an amusing case of ``fractal'' beams. We finally discuss some implications of our results in high-energy experiments and in cosmology.Using a recent technique, proposed by Eardley and Giddings, we extend their results to the high-energy collision of two beams of massless particles, i.e. of two finite-front shock waves. Closed (marginally) trapped surfaces can be determined analytically in several cases even for collisions at non-vanishing impact parameter in D\ge 4 space-time dimensions. We are able to confirm and extend earlier conjectures by Yurtsever, and to deal with arbitrary axisymmetric profiles, including an amusing case of ``fractal'' beams. We finally discuss some implications of our results in high-energy experiments and in cosmology.gr-qc/0203093CERN-TH-2002-064CERN-TH-2002-064oai:cds.cern.ch:5449542002-03-26
spellingShingle General Relativity and Cosmology
Kohlprath, Emmanuel
Veneziano, Gabriele
Black holes from high-energy beam--beam collisions
title Black holes from high-energy beam--beam collisions
title_full Black holes from high-energy beam--beam collisions
title_fullStr Black holes from high-energy beam--beam collisions
title_full_unstemmed Black holes from high-energy beam--beam collisions
title_short Black holes from high-energy beam--beam collisions
title_sort black holes from high-energy beam--beam collisions
topic General Relativity and Cosmology
url https://dx.doi.org/10.1088/1126-6708/2002/06/057
http://cds.cern.ch/record/544954
work_keys_str_mv AT kohlprathemmanuel blackholesfromhighenergybeambeamcollisions
AT venezianogabriele blackholesfromhighenergybeambeamcollisions