TeV Strings and Ultrahigh-Energy Cosmic Rays

dc.creatorIllana, Jose I.
dc.date2001-10-05
dc.date2001-10-09
dc.date.accessioned2026-07-07T03:45:29Z
dc.date.available2026-07-07T03:45:29Z
dc.descriptionThe origin and nature of ultrahigh-energy cosmic ray events, above the Greisen-Zatsepin-Kuzmin (GZK) cutoff energy, constitute a long-standing, unsolved mistery. Neutrinos are proposed candidates but their standard interactions with matter are too weak. In the context of a TeV-scale string theory, motivated by possible extra space dimensions, the neutrino-nucleon scattering is examined. Resonant string contributions increase substantially the standard model neutrino-nucleon cross section. Although they seem insufficient to explain the trans-GZK cosmic ray events, their effects might be detected in next experiments.
dc.description12 pages, LaTeX, 2 figures; talk presented at the XXV International School of Theoretical Physics, Ustron, Poland, September 10-16, 2001. Discussion on gravity versus gauge effects improved
dc.identifierhttps://arxiv.org/abs/hep-ph/0110092
dc.identifierhttp://arxiv.org/abs/hep-ph/0110092
dc.identifierActa Phys.Polon. B32 (2001) 3695-3706
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/40941
dc.subjectHigh Energy Physics - Phenomenology
dc.titleTeV Strings and Ultrahigh-Energy Cosmic Rays
dc.typetext

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