Detecting Neutrinos from AGNs and Topological Defects with Neutrino Telescopes

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dc.creatorGandhi, Raj
dc.creatorQuigg, Chris
dc.creatorReno, M. H.
dc.creatorSarcevic, Ina
dc.date1996-09-29
dc.date.accessioned2026-07-07T04:00:16Z
dc.date.available2026-07-07T04:00:16Z
dc.descriptionWe evaluate neutrino-nucleon cross section for energies up to $10^{21} eV$ in light of new information on the small-$x$ behavior of parton distributions. We give predictions for large underground neutrino telescope event rates for ultrahigh-energy neutrinos from Active Galactic Nuclei and from the decay of topological defects formed in the early Universe.
dc.descriptionTalk presented by I. Sarcevic at Annual Meeting of Division of Particles and Fields of the APS (DPF'96), Minneapolis, MN, August 10-15, 1996, 3 pp
dc.identifierhttps://arxiv.org/abs/hep-ph/9609516
dc.identifierhttp://arxiv.org/abs/hep-ph/9609516
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/46517
dc.subjectHigh Energy Physics - Phenomenology
dc.titleDetecting Neutrinos from AGNs and Topological Defects with Neutrino Telescopes
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