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The CMSSM and NUHM1 in Light of 7 TeV LHC, $B_s \to \mu^+\mu^-$ and XENON100 Data

We make a frequentist analysis of the parameter space of the CMSSM and NUHM1, using a Markov Chain Monte Carlo (MCMC) with 95 (221) million points to sample the CMSSM (NUHM1) parameter spaces. Our analysis includes the ATLAS search for supersymmetric jets + MET signals using ~ 5/fb of LHC data at 7...

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Detalles Bibliográficos
Autores principales: Buchmueller, O., Cavanaugh, R., Citron, M., De Roeck, A., Dolan, M.J., Ellis, J.R., Flacher, H., Heinemeyer, S., Isidori, G., Marrouche, J., Martinez Santos, D., Nakach, S., Olive, K.A., Rogerson, S., Ronga, F.J., de Vries, K.J., Weiglein, G.
Lenguaje:eng
Publicado: 2012
Materias:
Acceso en línea:https://dx.doi.org/10.1140/epjc/s10052-012-2243-3
http://cds.cern.ch/record/1471098
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author Buchmueller, O.
Cavanaugh, R.
Citron, M.
De Roeck, A.
Dolan, M.J.
Ellis, J.R.
Flacher, H.
Heinemeyer, S.
Isidori, G.
Marrouche, J.
Martinez Santos, D.
Nakach, S.
Olive, K.A.
Rogerson, S.
Ronga, F.J.
de Vries, K.J.
Weiglein, G.
author_facet Buchmueller, O.
Cavanaugh, R.
Citron, M.
De Roeck, A.
Dolan, M.J.
Ellis, J.R.
Flacher, H.
Heinemeyer, S.
Isidori, G.
Marrouche, J.
Martinez Santos, D.
Nakach, S.
Olive, K.A.
Rogerson, S.
Ronga, F.J.
de Vries, K.J.
Weiglein, G.
author_sort Buchmueller, O.
collection CERN
description We make a frequentist analysis of the parameter space of the CMSSM and NUHM1, using a Markov Chain Monte Carlo (MCMC) with 95 (221) million points to sample the CMSSM (NUHM1) parameter spaces. Our analysis includes the ATLAS search for supersymmetric jets + MET signals using ~ 5/fb of LHC data at 7 TeV, which we apply using PYTHIA and a Delphes implementation that we validate in the relevant parameter regions of the CMSSM and NUHM1. Our analysis also includes the constraint imposed by searches for B_s to mu+mu- by LHCb, CMS, ATLAS and CDF, and the limit on spin-independent dark matter scattering from 225 live days of XENON100 data. We assume M_h ~ 125 GeV, and use a full set of electroweak precision and other flavour-physics observables, as well as the cold dark matter density constraint. The ATLAS 5/fb constraint has relatively limited effects on the 68 and 95% CL regions in the (m_0, m_1/2) planes of the CMSSM and NUHM1. The new B_s to mu+mu- constraint has greater impacts on these CL regions, and also impacts significantly the 68 and 95% CL regions in the (M_A, tan beta) planes of both models, reducing the best-fit values of tan beta. The recent XENON100 data eliminate the focus-point region in the CMSSM and affect the 68 and 95% CL regions in the NUHM1. In combination, these new constraints reduce the best-fit values of m_0, m_1/2 in the CMSSM, and increase the global chi^2 from 31.0 to 32.8, reducing the p-value from 12% to 8.5%. In the case of the NUHM1, they have little effect on the best-fit values of m_0, m_1/2, but increase the global chi^2 from 28.9 to 31.3, thereby reducing the p-value from 15% to 9.1%.
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spelling cern-14710982020-08-28T12:54:46Zdoi:10.1140/epjc/s10052-012-2243-3http://cds.cern.ch/record/1471098engBuchmueller, O.Cavanaugh, R.Citron, M.De Roeck, A.Dolan, M.J.Ellis, J.R.Flacher, H.Heinemeyer, S.Isidori, G.Marrouche, J.Martinez Santos, D.Nakach, S.Olive, K.A.Rogerson, S.Ronga, F.J.de Vries, K.J.Weiglein, G.The CMSSM and NUHM1 in Light of 7 TeV LHC, $B_s \to \mu^+\mu^-$ and XENON100 DataParticle Physics - PhenomenologyWe make a frequentist analysis of the parameter space of the CMSSM and NUHM1, using a Markov Chain Monte Carlo (MCMC) with 95 (221) million points to sample the CMSSM (NUHM1) parameter spaces. Our analysis includes the ATLAS search for supersymmetric jets + MET signals using ~ 5/fb of LHC data at 7 TeV, which we apply using PYTHIA and a Delphes implementation that we validate in the relevant parameter regions of the CMSSM and NUHM1. Our analysis also includes the constraint imposed by searches for B_s to mu+mu- by LHCb, CMS, ATLAS and CDF, and the limit on spin-independent dark matter scattering from 225 live days of XENON100 data. We assume M_h ~ 125 GeV, and use a full set of electroweak precision and other flavour-physics observables, as well as the cold dark matter density constraint. The ATLAS 5/fb constraint has relatively limited effects on the 68 and 95% CL regions in the (m_0, m_1/2) planes of the CMSSM and NUHM1. The new B_s to mu+mu- constraint has greater impacts on these CL regions, and also impacts significantly the 68 and 95% CL regions in the (M_A, tan beta) planes of both models, reducing the best-fit values of tan beta. The recent XENON100 data eliminate the focus-point region in the CMSSM and affect the 68 and 95% CL regions in the NUHM1. In combination, these new constraints reduce the best-fit values of m_0, m_1/2 in the CMSSM, and increase the global chi^2 from 31.0 to 32.8, reducing the p-value from 12% to 8.5%. In the case of the NUHM1, they have little effect on the best-fit values of m_0, m_1/2, but increase the global chi^2 from 28.9 to 31.3, thereby reducing the p-value from 15% to 9.1%.We make a frequentist analysis of the parameter space of the CMSSM and NUHM1, using a Markov Chain Monte Carlo (MCMC) with 95 (221) million points to sample the CMSSM (NUHM1) parameter spaces. Our analysis includes the ATLAS search for supersymmetric jets + MET signals using ~ 5/fb of LHC data at 7 TeV, which we apply using PYTHIA and a Delphes implementation that we validate in the relevant parameter regions of the CMSSM and NUHM1. Our analysis also includes the constraint imposed by searches for B_s to mu+mu- by LHCb, CMS, ATLAS and CDF, and the limit on spin-independent dark matter scattering from 225 live days of XENON100 data. We assume M_h ~ 125 GeV, and use a full set of electroweak precision and other flavour-physics observables, as well as the cold dark matter density constraint. The ATLAS 5/fb constraint has relatively limited effects on the 68 and 95% CL regions in the (m_0, m_1/2) planes of the CMSSM and NUHM1. The new B_s to mu+mu- constraint has greater impacts on these CL regions, and also impacts significantly the 68 and 95% CL regions in the (M_A, tan beta) planes of both models, reducing the best-fit values of tan beta. The recent XENON100 data eliminate the focus-point region in the CMSSM and affect the 68 and 95% CL regions in the NUHM1. In combination, these new constraints reduce the best-fit values of m_0, m_1/2 in the CMSSM, and increase the global chi^2 from 31.0 to 32.8, reducing the p-value from 12% to 8.5%. In the case of the NUHM1, they have little effect on the best-fit values of m_0, m_1/2, but increase the global chi^2 from 28.9 to 31.3, thereby reducing the p-value from 15% to 9.1%.KCL-PH-TH-2012-26LCTS-2012-13CERN-PH-TH-2012-164DCPT-12-82DESY-12-115IPPP-12-41FTPI-MINN-12-20UMN-TH-3106-12FERMILAB-PUB-12-868-TarXiv:1207.7315KCL-PH-TH-2012-26LCTS-2012-13CERN-PH-TH-2012-164DCPT-12-82DESY 12-115IPPP-12-41FTPI-MINN-12-20UMN-TH-3106-12oai:cds.cern.ch:14710982012-08-01
spellingShingle Particle Physics - Phenomenology
Buchmueller, O.
Cavanaugh, R.
Citron, M.
De Roeck, A.
Dolan, M.J.
Ellis, J.R.
Flacher, H.
Heinemeyer, S.
Isidori, G.
Marrouche, J.
Martinez Santos, D.
Nakach, S.
Olive, K.A.
Rogerson, S.
Ronga, F.J.
de Vries, K.J.
Weiglein, G.
The CMSSM and NUHM1 in Light of 7 TeV LHC, $B_s \to \mu^+\mu^-$ and XENON100 Data
title The CMSSM and NUHM1 in Light of 7 TeV LHC, $B_s \to \mu^+\mu^-$ and XENON100 Data
title_full The CMSSM and NUHM1 in Light of 7 TeV LHC, $B_s \to \mu^+\mu^-$ and XENON100 Data
title_fullStr The CMSSM and NUHM1 in Light of 7 TeV LHC, $B_s \to \mu^+\mu^-$ and XENON100 Data
title_full_unstemmed The CMSSM and NUHM1 in Light of 7 TeV LHC, $B_s \to \mu^+\mu^-$ and XENON100 Data
title_short The CMSSM and NUHM1 in Light of 7 TeV LHC, $B_s \to \mu^+\mu^-$ and XENON100 Data
title_sort cmssm and nuhm1 in light of 7 tev lhc, $b_s \to \mu^+\mu^-$ and xenon100 data
topic Particle Physics - Phenomenology
url https://dx.doi.org/10.1140/epjc/s10052-012-2243-3
http://cds.cern.ch/record/1471098
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