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Beyond the CMSSM without an Accelerator: Proton Decay and Direct Dark Matter Detection
We consider two potential non-accelerator signatures of generalizations of the well-studied constrained minimal supersymmetric standard model (CMSSM). In one generalization, the universality constraints on soft supersymmetry-breaking parameters are applied at some input scale $M_{in}$ below the gran...
Autores principales: | , , , , , |
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Lenguaje: | eng |
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2015
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Acceso en línea: | https://dx.doi.org/10.1140/epjc/s10052-015-3842-6 http://cds.cern.ch/record/2055954 |
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author | Ellis, John Evans, Jason L. Luo, Feng Nagata, Natsumi Olive, Keith A. Sandick, Pearl |
author_facet | Ellis, John Evans, Jason L. Luo, Feng Nagata, Natsumi Olive, Keith A. Sandick, Pearl |
author_sort | Ellis, John |
collection | CERN |
description | We consider two potential non-accelerator signatures of generalizations of the well-studied constrained minimal supersymmetric standard model (CMSSM). In one generalization, the universality constraints on soft supersymmetry-breaking parameters are applied at some input scale $M_{in}$ below the grand unification (GUT) scale $M_{GUT}$, a scenario referred to as `sub-GUT'. The other generalization we consider is to retain GUT-scale universality for the squark and slepton masses, but to relax universality for the soft supersymmetry-breaking contributions to the masses of the Higgs doublets. As with other CMSSM-like models, the measured Higgs mass requires supersymmetric particle masses near or beyond the TeV scale. Because of these rather heavy sparticle masses, the embedding of these CMSSM-like models in a minimal SU(5) model of grand unification can yield a proton lifetime consistent with current experimental limits, and may be accessible in existing and future proton decay experiments. Another possible signature of these CMSSM-like models is direct detection of supersymmetric dark matter. The direct dark matter scattering rate is typically below the reach of the LUX-ZEPLIN (LZ) experiment if $M_{in}$ is close to $M_{GUT}$, but may lie within its reach if $M_{in} \lesssim 10^{11}$ GeV. Likewise, generalizing the CMSSM to allow non-universal supersymmetry-breaking contributions to the Higgs offers extensive possibilities for models within reach of the LZ experiment that have long proton lifetimes. |
id | cern-2055954 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2015 |
record_format | invenio |
spelling | cern-20559542023-09-12T03:29:30Zdoi:10.1140/epjc/s10052-015-3842-6http://cds.cern.ch/record/2055954engEllis, JohnEvans, Jason L.Luo, FengNagata, NatsumiOlive, Keith A.Sandick, PearlBeyond the CMSSM without an Accelerator: Proton Decay and Direct Dark Matter DetectionParticle Physics - PhenomenologyWe consider two potential non-accelerator signatures of generalizations of the well-studied constrained minimal supersymmetric standard model (CMSSM). In one generalization, the universality constraints on soft supersymmetry-breaking parameters are applied at some input scale $M_{in}$ below the grand unification (GUT) scale $M_{GUT}$, a scenario referred to as `sub-GUT'. The other generalization we consider is to retain GUT-scale universality for the squark and slepton masses, but to relax universality for the soft supersymmetry-breaking contributions to the masses of the Higgs doublets. As with other CMSSM-like models, the measured Higgs mass requires supersymmetric particle masses near or beyond the TeV scale. Because of these rather heavy sparticle masses, the embedding of these CMSSM-like models in a minimal SU(5) model of grand unification can yield a proton lifetime consistent with current experimental limits, and may be accessible in existing and future proton decay experiments. Another possible signature of these CMSSM-like models is direct detection of supersymmetric dark matter. The direct dark matter scattering rate is typically below the reach of the LUX-ZEPLIN (LZ) experiment if $M_{in}$ is close to $M_{GUT}$, but may lie within its reach if $M_{in} \lesssim 10^{11}$ GeV. Likewise, generalizing the CMSSM to allow non-universal supersymmetry-breaking contributions to the Higgs offers extensive possibilities for models within reach of the LZ experiment that have long proton lifetimes.We consider two potential non-accelerator signatures of generalizations of the well-studied constrained minimal supersymmetric standard model (CMSSM). In one generalization, the universality constraints on soft supersymmetry-breaking parameters are applied at some input scale $M_{\mathrm{in}}$ below the grand unification (GUT) scale $M_{\mathrm{GUT}}$ , a scenario referred to as ‘sub-GUT’. The other generalization we consider is to retain GUT-scale universality for the squark and slepton masses, but to relax universality for the soft supersymmetry-breaking contributions to the masses of the Higgs doublets. As with other CMSSM-like models, the measured Higgs mass requires supersymmetric particle masses near or beyond the TeV scale. Because of these rather heavy sparticle masses, the embedding of these CMSSM-like models in a minimal SU(5) model of grand unification can yield a proton lifetime consistent with current experimental limits, and may be accessible in existing and future proton decay experiments. Another possible signature of these CMSSM-like models is direct detection of supersymmetric dark matter. The direct dark matter scattering rate is typically below the reach of the LUX-ZEPLIN (LZ) experiment if $M_{\mathrm{in}}$ is close to $M_{\mathrm{GUT}}$ , but it may lie within its reach if $M_{\mathrm{in}} \lesssim 10^{11}$ GeV. Likewise, generalizing the CMSSM to allow non-universal supersymmetry-breaking contributions to the Higgs offers extensive possibilities for models within reach of the LZ experiment that have long proton lifetimes.We consider two potential non-accelerator signatures of generalizations of the well-studied constrained minimal supersymmetric standard model (CMSSM). In one generalization, the universality constraints on soft supersymmetry-breaking parameters are applied at some input scale $M_{in}$ below the grand unification (GUT) scale $M_{GUT}$, a scenario referred to as `sub-GUT'. The other generalization we consider is to retain GUT-scale universality for the squark and slepton masses, but to relax universality for the soft supersymmetry-breaking contributions to the masses of the Higgs doublets. As with other CMSSM-like models, the measured Higgs mass requires supersymmetric particle masses near or beyond the TeV scale. Because of these rather heavy sparticle masses, the embedding of these CMSSM-like models in a minimal SU(5) model of grand unification can yield a proton lifetime consistent with current experimental limits, and may be accessible in existing and future proton decay experiments. Another possible signature of these CMSSM-like models is direct detection of supersymmetric dark matter. The direct dark matter scattering rate is typically below the reach of the LUX-ZEPLIN (LZ) experiment if $M_{in}$ is close to $M_{GUT}$, but may lie within its reach if $M_{in} \lesssim 10^{11}$ GeV. Likewise, generalizing the CMSSM to allow non-universal supersymmetry-breaking contributions to the Higgs offers extensive possibilities for models within reach of the LZ experiment that have long proton lifetimes.arXiv:1509.08838KCL-PH-TH-2015-42LCTS-2015-29CERN-PH-TH-2015-229UMN-TH-3502-15FTPI--MINN--15-41IPMU15--0174CETUP2015-021UMN--TH--3502-15KCL-PH-TH-2015-42LCTS-2015-29CERN-PH-TH-2015-229UMN-TH-3502-15FTPI-MINN-15-41IPMU15-0174CETUP-2015-021oai:cds.cern.ch:20559542015-09-29 |
spellingShingle | Particle Physics - Phenomenology Ellis, John Evans, Jason L. Luo, Feng Nagata, Natsumi Olive, Keith A. Sandick, Pearl Beyond the CMSSM without an Accelerator: Proton Decay and Direct Dark Matter Detection |
title | Beyond the CMSSM without an Accelerator: Proton Decay and Direct Dark Matter Detection |
title_full | Beyond the CMSSM without an Accelerator: Proton Decay and Direct Dark Matter Detection |
title_fullStr | Beyond the CMSSM without an Accelerator: Proton Decay and Direct Dark Matter Detection |
title_full_unstemmed | Beyond the CMSSM without an Accelerator: Proton Decay and Direct Dark Matter Detection |
title_short | Beyond the CMSSM without an Accelerator: Proton Decay and Direct Dark Matter Detection |
title_sort | beyond the cmssm without an accelerator: proton decay and direct dark matter detection |
topic | Particle Physics - Phenomenology |
url | https://dx.doi.org/10.1140/epjc/s10052-015-3842-6 http://cds.cern.ch/record/2055954 |
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