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Frequentist Analysis of the Parameter Space of Minimal Supergravity

We make a frequentist analysis of the parameter space of minimal supergravity (mSUGRA), in which, as well as the gaugino and scalar soft supersymmetry-breaking parameters being universal, there is a specific relation between the trilinear, bilinear and scalar supersymmetry-breaking parameters, A_0 =...

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Autores principales: Buchmueller, O., Cavanaugh, R., Colling, D., De Roeck, A., Dolan, M.J., Ellis, J.R., Flacher, H., Heinemeyer, S., Olive, K.A., Rogerson, S., Ronga, F.J., Weiglein, G.
Lenguaje:eng
Publicado: 2010
Materias:
Acceso en línea:https://dx.doi.org/10.1140/epjc/s10052-011-1583-8
http://cds.cern.ch/record/1310554
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author Buchmueller, O.
Cavanaugh, R.
Colling, D.
De Roeck, A.
Dolan, M.J.
Ellis, J.R.
Flacher, H.
Heinemeyer, S.
Olive, K.A.
Rogerson, S.
Ronga, F.J.
Weiglein, G.
author_facet Buchmueller, O.
Cavanaugh, R.
Colling, D.
De Roeck, A.
Dolan, M.J.
Ellis, J.R.
Flacher, H.
Heinemeyer, S.
Olive, K.A.
Rogerson, S.
Ronga, F.J.
Weiglein, G.
author_sort Buchmueller, O.
collection CERN
description We make a frequentist analysis of the parameter space of minimal supergravity (mSUGRA), in which, as well as the gaugino and scalar soft supersymmetry-breaking parameters being universal, there is a specific relation between the trilinear, bilinear and scalar supersymmetry-breaking parameters, A_0 = B_0 + m_0, and the gravitino mass is fixed by m_{3/2} = m_0. We also consider a more general model, in which the gravitino mass constraint is relaxed (the VCMSSM). We combine in the global likelihood function the experimental constraints from low-energy electroweak precision data, the anomalous magnetic moment of the muon, the lightest Higgs boson mass M_h, B physics and the astrophysical cold dark matter density, assuming that the lightest supersymmetric particle (LSP) is a neutralino. In the VCMSSM, we find a preference for values of m_{1/2} and m_0 similar to those found previously in frequentist analyses of the constrained MSSM (CMSSM) and a model with common non-universal Higgs masses (NUHM1). On the other hand, in mSUGRA we find two preferred regions: one with larger values of both m_{1/2} and m_0 than in the VCMSSM, and one with large m_0 but small m_{1/2}. We compare the probabilities of the frequentist fits in mSUGRA, the VCMSSM, the CMSSM and the NUHM1: the probability that mSUGRA is consistent with the present data is significantly less than in the other models. We also discuss the mSUGRA and VCMSSM predictions for sparti cle masses and other observables, identifying potential signatures at the LHC and elsewhere.
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language eng
publishDate 2010
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spelling cern-13105542020-08-28T12:57:58Zdoi:10.1140/epjc/s10052-011-1583-8http://cds.cern.ch/record/1310554engBuchmueller, O.Cavanaugh, R.Colling, D.De Roeck, A.Dolan, M.J.Ellis, J.R.Flacher, H.Heinemeyer, S.Olive, K.A.Rogerson, S.Ronga, F.J.Weiglein, G.Frequentist Analysis of the Parameter Space of Minimal SupergravityParticle Physics - PhenomenologyWe make a frequentist analysis of the parameter space of minimal supergravity (mSUGRA), in which, as well as the gaugino and scalar soft supersymmetry-breaking parameters being universal, there is a specific relation between the trilinear, bilinear and scalar supersymmetry-breaking parameters, A_0 = B_0 + m_0, and the gravitino mass is fixed by m_{3/2} = m_0. We also consider a more general model, in which the gravitino mass constraint is relaxed (the VCMSSM). We combine in the global likelihood function the experimental constraints from low-energy electroweak precision data, the anomalous magnetic moment of the muon, the lightest Higgs boson mass M_h, B physics and the astrophysical cold dark matter density, assuming that the lightest supersymmetric particle (LSP) is a neutralino. In the VCMSSM, we find a preference for values of m_{1/2} and m_0 similar to those found previously in frequentist analyses of the constrained MSSM (CMSSM) and a model with common non-universal Higgs masses (NUHM1). On the other hand, in mSUGRA we find two preferred regions: one with larger values of both m_{1/2} and m_0 than in the VCMSSM, and one with large m_0 but small m_{1/2}. We compare the probabilities of the frequentist fits in mSUGRA, the VCMSSM, the CMSSM and the NUHM1: the probability that mSUGRA is consistent with the present data is significantly less than in the other models. We also discuss the mSUGRA and VCMSSM predictions for sparti cle masses and other observables, identifying potential signatures at the LHC and elsewhere.We make a frequentist analysis of the parameter space of minimal supergravity (mSUGRA), in which, as well as the gaugino and scalar soft supersymmetry-breaking parameters being universal, there is a specific relation between the trilinear, bilinear and scalar supersymmetry-breaking parameters, A_0 = B_0 + m_0, and the gravitino mass is fixed by m_{3/2} = m_0. We also consider a more general model, in which the gravitino mass constraint is relaxed (the VCMSSM). We combine in the global likelihood function the experimental constraints from low-energy electroweak precision data, the anomalous magnetic moment of the muon, the lightest Higgs boson mass M_h, B physics and the astrophysical cold dark matter density, assuming that the lightest supersymmetric particle (LSP) is a neutralino. In the VCMSSM, we find a preference for values of m_{1/2} and m_0 similar to those found previously in frequentist analyses of the constrained MSSM (CMSSM) and a model with common non-universal Higgs masses (NUHM1). On the other hand, in mSUGRA we find two preferred regions: one with larger values of both m_{1/2} and m_0 than in the VCMSSM, and one with large m_0 but small m_{1/2}. We compare the probabilities of the frequentist fits in mSUGRA, the VCMSSM, the CMSSM and the NUHM1: the probability that mSUGRA is consistent with the present data is significantly less than in the other models. We also discuss the mSUGRA and VCMSSM predictions for sparticle masses and other observables, identifying potential signatures at the LHC and elsewhere.arXiv:1011.6118CERN-PH-TH-2010-169DCPT-10-196DESY-10-211IPPP-10-98FTPI-MINN-10-34KCL-PH-TH-2010-34UMN-TH-2928-10FERMILAB-PUB-10-734-CMSCERN-PH-TH-2010-169DCPT-10-196DESY 10-211IPPP-10-98FTPI-MINN-10-34KCL-PH-TH-2010-34UMN-TH-2928-10oai:cds.cern.ch:13105542010-11-30
spellingShingle Particle Physics - Phenomenology
Buchmueller, O.
Cavanaugh, R.
Colling, D.
De Roeck, A.
Dolan, M.J.
Ellis, J.R.
Flacher, H.
Heinemeyer, S.
Olive, K.A.
Rogerson, S.
Ronga, F.J.
Weiglein, G.
Frequentist Analysis of the Parameter Space of Minimal Supergravity
title Frequentist Analysis of the Parameter Space of Minimal Supergravity
title_full Frequentist Analysis of the Parameter Space of Minimal Supergravity
title_fullStr Frequentist Analysis of the Parameter Space of Minimal Supergravity
title_full_unstemmed Frequentist Analysis of the Parameter Space of Minimal Supergravity
title_short Frequentist Analysis of the Parameter Space of Minimal Supergravity
title_sort frequentist analysis of the parameter space of minimal supergravity
topic Particle Physics - Phenomenology
url https://dx.doi.org/10.1140/epjc/s10052-011-1583-8
http://cds.cern.ch/record/1310554
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