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MSSM radiative contributions to the WW$\gamma$ and WWZ form factors

We evaluate one-loop contributions to the C and P conserving WW\gamma, WWZ form factors in the Minimal Supersymmetric Standard Model (MSSM), and in a more constrained Supergravity Grand Unified Theory (SUGRA-GUT). A systematic search of maximal effects in the available parameter space, shows that at...

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Detalles Bibliográficos
Autores principales: Arhrib, A, Kneur, J L, Moultaka, G
Lenguaje:eng
Publicado: 1995
Materias:
Acceso en línea:https://dx.doi.org/10.1016/0370-2693(96)00191-8
http://cds.cern.ch/record/293770
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author Arhrib, A
Kneur, J L
Moultaka, G
author_facet Arhrib, A
Kneur, J L
Moultaka, G
author_sort Arhrib, A
collection CERN
description We evaluate one-loop contributions to the C and P conserving WW\gamma, WWZ form factors in the Minimal Supersymmetric Standard Model (MSSM), and in a more constrained Supergravity Grand Unified Theory (SUGRA-GUT). A systematic search of maximal effects in the available parameter space, shows that at LEP2 energy MSSM contributions can hardly reach the border of the most optimistic accuracy expected on those couplings, even for particles close to their production thresholds. At NLC energies, the effects are more comfortably of the order of the expected sensitivity, and may therefore provide useful information on MSSM parameter values which will not be available from direct particle production. We also discuss briefly some variance with other studies.
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institution Organización Europea para la Investigación Nuclear
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publishDate 1995
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spelling cern-2937702019-09-30T06:29:59Zdoi:10.1016/0370-2693(96)00191-8http://cds.cern.ch/record/293770engArhrib, AKneur, J LMoultaka, GMSSM radiative contributions to the WW$\gamma$ and WWZ form factorsParticle Physics - PhenomenologyWe evaluate one-loop contributions to the C and P conserving WW\gamma, WWZ form factors in the Minimal Supersymmetric Standard Model (MSSM), and in a more constrained Supergravity Grand Unified Theory (SUGRA-GUT). A systematic search of maximal effects in the available parameter space, shows that at LEP2 energy MSSM contributions can hardly reach the border of the most optimistic accuracy expected on those couplings, even for particles close to their production thresholds. At NLC energies, the effects are more comfortably of the order of the expected sensitivity, and may therefore provide useful information on MSSM parameter values which will not be available from direct particle production. We also discuss briefly some variance with other studies.hep-ph/9512437CERN-TH-95-344PM-95-25oai:cds.cern.ch:2937701995-12-28
spellingShingle Particle Physics - Phenomenology
Arhrib, A
Kneur, J L
Moultaka, G
MSSM radiative contributions to the WW$\gamma$ and WWZ form factors
title MSSM radiative contributions to the WW$\gamma$ and WWZ form factors
title_full MSSM radiative contributions to the WW$\gamma$ and WWZ form factors
title_fullStr MSSM radiative contributions to the WW$\gamma$ and WWZ form factors
title_full_unstemmed MSSM radiative contributions to the WW$\gamma$ and WWZ form factors
title_short MSSM radiative contributions to the WW$\gamma$ and WWZ form factors
title_sort mssm radiative contributions to the ww$\gamma$ and wwz form factors
topic Particle Physics - Phenomenology
url https://dx.doi.org/10.1016/0370-2693(96)00191-8
http://cds.cern.ch/record/293770
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