Strings, Black Holes and the Extreme Energy Cosmic Rays

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dc.creatorDomokos, G.
dc.creatorKovesi-Domokos, S.
dc.date2003-07-07
dc.date2004-07-12
dc.date.accessioned2026-07-07T10:48:48Z
dc.date.available2026-07-07T10:48:48Z
dc.descriptionIn a large class of models the string excitation and black hole pictures invoked as an explanation of trans-GZK cosmic ray events are equivalent. Single particle inclusive distributions are thermal at the Hagedorn temperature. The hadron multiplicities are reminiscent of multiplicities in heavy nucleus initiated interactions.
dc.description10 pages, no figures
dc.identifierhttps://arxiv.org/abs/hep-ph/0307099
dc.identifierhttp://arxiv.org/abs/hep-ph/0307099
dc.identifierAstropart.Phys.27:227-232,2007
dc.identifierdoi:10.1016/j.astropartphys.2006.06.013
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/184007
dc.subjectHigh Energy Physics - Phenomenology
dc.titleStrings, Black Holes and the Extreme Energy Cosmic Rays
dc.typetext

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