Phenomenology of Multi-W Processes in Cosmic Rays

Details Phenomenology of Multi-W Processes in Cosmic Rays Phenomenology of Multi-W Processes in Cosmic Rays

1993-09-14

arxiv.org/abs/hep-ph/9309259v1

Physics

High Energy Physics

High Energy Physics - Phenomenology

(Invited talk presented by A. Ringwald at 17th Johns Hopkins Workshop on Current Problems in Particle Theory, Particles and th

Scientific paper

We 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.

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