Cargando…

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...

Descripción completa

Detalles Bibliográficos
Autores principales: Ellis, John, Evans, Jason L., Luo, Feng, Nagata, Natsumi, Olive, Keith A., Sandick, Pearl
Lenguaje:eng
Publicado: 2015
Materias:
Acceso en línea:https://dx.doi.org/10.1140/epjc/s10052-015-3842-6
http://cds.cern.ch/record/2055954
_version_ 1780948320020070400
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
work_keys_str_mv AT ellisjohn beyondthecmssmwithoutanacceleratorprotondecayanddirectdarkmatterdetection
AT evansjasonl beyondthecmssmwithoutanacceleratorprotondecayanddirectdarkmatterdetection
AT luofeng beyondthecmssmwithoutanacceleratorprotondecayanddirectdarkmatterdetection
AT nagatanatsumi beyondthecmssmwithoutanacceleratorprotondecayanddirectdarkmatterdetection
AT olivekeitha beyondthecmssmwithoutanacceleratorprotondecayanddirectdarkmatterdetection
AT sandickpearl beyondthecmssmwithoutanacceleratorprotondecayanddirectdarkmatterdetection