Cosmic Ray Signatures of Multi-W Processes

Details Cosmic Ray Signatures of Multi-W Processes Cosmic Ray Signatures of Multi-W Processes

1993-08-13

arxiv.org/abs/hep-ph/9308269v1

Astropart.Phys.2:43-66,1994

Physics

High Energy Physics

High Energy Physics - Phenomenology

44 pages (LaTeX) + 19 PostScript figures in accompanying file (uuencoded), CERN-TH.6822/93,UCLA 93/TEP/24

Scientific paper

10.1016/0927-6505(94)90017-5

We explore the discovery potential of cosmic ray physics experiments for Standard Model processes involving the nonperturbative production of O(30) weak gauge bosons. We demonstrate an experimental insensitivity to proton-induced processes and emphasize the importance of neutrino-induced processes. The Fly's Eye currently constrains the largest region of parameter space characterizing multi-W phenomena if a cosmic neutrino flux exists at levels suggested by recent models of active galactic nuclei. MACRO (DUMAND) can constrain or observe additional regions by searching for 1-100 (1-10) characteristic near-vertical (near-horizontal) spatially compact energetic muon bundles per year.

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