Phenomenology of Multi-W Processes in Cosmic Rays

dc.creatorMorris, D. A.
dc.creatorRingwald, A.
dc.date1993-09-14
dc.date.accessioned2026-07-25T19:19:49Z
dc.descriptionWe report on a study of the potential of various cosmic ray physics experiments to search for Standard Model processes involving the nonperturbative production of O(30) weak gauge bosons. Whereas present and near-future experiments are insensitive to proton-induced processes, neutrino-induced processes give rise to promising signatures and rates in AMANDA, DUMAND, MACRO and NESTOR provided that a cosmic neutrino flux exists at levels suggested by recent models of active galactic nuclei. The Fly's Eye currently constrains the largest region of parameter space characterizing multi-W phenomena.
dc.description(Invited talk presented by A. Ringwald at 17th Johns Hopkins Workshop on Current Problems in Particle Theory, Particles and the Universe, July 30-August 1, 1993, Budapest, Hungary), 16 pages (LaTeX) + 10 uuencoded PostScript figures, CERN-TH.7005/93, UCLA/93/TEP/32
dc.identifierhttps://arxiv.org/abs/hep-ph/9309259
dc.identifierhttp://arxiv.org/abs/hep-ph/9309259
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/63710
dc.subjectHigh Energy Physics - Phenomenology
dc.titlePhenomenology of Multi-W Processes in Cosmic Rays
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