Phenomenology of multi-W processes in cosmic rays

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 proces...

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Detalles Bibliográficos
Autores principales: Morris, D.A., Ringwald, A.
Lenguaje:eng
Publicado: 1993
Materias:
Particle Physics - Phenomenology
Acceso en línea:http://cds.cern.ch/record/253395
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author Morris, D.A.
Ringwald, A.
author_facet Morris, D.A.
Ringwald, A.
author_sort Morris, D.A.
collection CERN
description 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.
id cern-253395
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 1993
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spelling cern-2533952020-07-23T02:48:19Zhttp://cds.cern.ch/record/253395engMorris, D.A.Ringwald, A.Phenomenology of multi-W processes in cosmic raysParticle Physics - PhenomenologyWe 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.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.hep-ph/9309259CERN-TH-7005-93UCLA-93-TEP-32CERN-TH-7005-93UCLA-93-TEP-32oai:cds.cern.ch:2533951993
spellingShingle Particle Physics - Phenomenology
Morris, D.A.
Ringwald, A.
Phenomenology of multi-W processes in cosmic rays
title Phenomenology of multi-W processes in cosmic rays
title_full Phenomenology of multi-W processes in cosmic rays
title_fullStr Phenomenology of multi-W processes in cosmic rays
title_full_unstemmed Phenomenology of multi-W processes in cosmic rays
title_short Phenomenology of multi-W processes in cosmic rays
title_sort phenomenology of multi-w processes in cosmic rays
topic Particle Physics - Phenomenology
url http://cds.cern.ch/record/253395
work_keys_str_mv AT morrisda phenomenologyofmultiwprocessesincosmicrays
AT ringwalda phenomenologyofmultiwprocessesincosmicrays

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