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Superheavy Supersymmetry

One way to suppress flavor changing neutral currents or CP violating processes in supersymmetry is to make at least some of the first two generations' scalars superheavy (above ~20 TeV). We summarize the motivations and challenges, theoretically and phenomenologically, for superheavy supersymme...

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Detalles Bibliográficos
Autores principales: Ambrosanio, Sandro, Wells, James D.
Lenguaje:eng
Publicado: 1999
Materias:
Acceso en línea:http://cds.cern.ch/record/378506
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author Ambrosanio, Sandro
Wells, James D.
author_facet Ambrosanio, Sandro
Wells, James D.
author_sort Ambrosanio, Sandro
collection CERN
description One way to suppress flavor changing neutral currents or CP violating processes in supersymmetry is to make at least some of the first two generations' scalars superheavy (above ~20 TeV). We summarize the motivations and challenges, theoretically and phenomenologically, for superheavy supersymmetry. We then argue for more viable alternatives on the superheavy theme and are led to models where the heavy spectrum follows a pattern of masses similar to what arises from gauge-mediation or with a "hybrid" spectrum of light and heavy masses based on each particle's transformation under a global SU(5). In the end, despite the differences between the competing ideas, a self-consistent natural theory with superheavy masses seems to prefer low-energy supersymmetry breaking with possible correlations among the light sparticle masses. The resulting light gravitino and its couplings to matter could also impact the discovery capabilities and analyses of these models at colliders. In addition, we comment on how the presence of superheavy states may influence the light spectrum, and how this may help efforts to distinguish between theories post-discovery.
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spelling cern-3785062023-03-14T18:44:18Zhttp://cds.cern.ch/record/378506engAmbrosanio, SandroWells, James D.Superheavy SupersymmetryParticle Physics - PhenomenologyOne way to suppress flavor changing neutral currents or CP violating processes in supersymmetry is to make at least some of the first two generations' scalars superheavy (above ~20 TeV). We summarize the motivations and challenges, theoretically and phenomenologically, for superheavy supersymmetry. We then argue for more viable alternatives on the superheavy theme and are led to models where the heavy spectrum follows a pattern of masses similar to what arises from gauge-mediation or with a "hybrid" spectrum of light and heavy masses based on each particle's transformation under a global SU(5). In the end, despite the differences between the competing ideas, a self-consistent natural theory with superheavy masses seems to prefer low-energy supersymmetry breaking with possible correlations among the light sparticle masses. The resulting light gravitino and its couplings to matter could also impact the discovery capabilities and analyses of these models at colliders. In addition, we comment on how the presence of superheavy states may influence the light spectrum, and how this may help efforts to distinguish between theories post-discovery.One way to suppress flavor changing neutral currents or CP violating processes in supersymmetry is to make at least some of the first two generations' scalars superheavy (above ~20 TeV). We summarize the motivations and challenges, theoretically and phenomenologically, for superheavy supersymmetry. We then argue for more viable alternatives on the superheavy theme and are led to models where the heavy spectrum follows a pattern of masses similar to what arises from gauge-mediation or with a "hybrid" spectrum of light and heavy masses based on each particle's transformation under a global SU(5). In the end, despite the differences between the competing ideas, a self-consistent natural theory with superheavy masses seems to prefer low-energy supersymmetry breaking with possible correlations among the light sparticle masses. The resulting light gravitino and its couplings to matter could also impact the discovery capabilities and analyses of these models at colliders. In addition, we comment on how the presence of superheavy states may influence the light spectrum, and how this may help efforts to distinguish between theories post-discovery.hep-ph/9902242CERN-TH-99-19CERN-TH-99-019oai:cds.cern.ch:3785061999-02-05
spellingShingle Particle Physics - Phenomenology
Ambrosanio, Sandro
Wells, James D.
Superheavy Supersymmetry
title Superheavy Supersymmetry
title_full Superheavy Supersymmetry
title_fullStr Superheavy Supersymmetry
title_full_unstemmed Superheavy Supersymmetry
title_short Superheavy Supersymmetry
title_sort superheavy supersymmetry
topic Particle Physics - Phenomenology
url http://cds.cern.ch/record/378506
work_keys_str_mv AT ambrosaniosandro superheavysupersymmetry
AT wellsjamesd superheavysupersymmetry