Phenomenology of Multi-W Processes in Cosmic Rays
Abstract
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.
Keywords
Cite
@article{arxiv.hep-ph/9309259,
title = {Phenomenology of Multi-W Processes in Cosmic Rays},
author = {D. A. Morris and A. Ringwald},
journal= {arXiv preprint arXiv:hep-ph/9309259},
year = {2007}
}
Comments
(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