Cargando…
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...
Autores principales: | , , , , , , , , , , , , , , , , |
---|---|
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 |
_version_ | 1780925382538559488 |
---|---|
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%. |
id | cern-1471098 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2012 |
record_format | invenio |
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 |
work_keys_str_mv | AT buchmuellero thecmssmandnuhm1inlightof7tevlhcbstomumuandxenon100data AT cavanaughr thecmssmandnuhm1inlightof7tevlhcbstomumuandxenon100data AT citronm thecmssmandnuhm1inlightof7tevlhcbstomumuandxenon100data AT deroecka thecmssmandnuhm1inlightof7tevlhcbstomumuandxenon100data AT dolanmj thecmssmandnuhm1inlightof7tevlhcbstomumuandxenon100data AT ellisjr thecmssmandnuhm1inlightof7tevlhcbstomumuandxenon100data AT flacherh thecmssmandnuhm1inlightof7tevlhcbstomumuandxenon100data AT heinemeyers thecmssmandnuhm1inlightof7tevlhcbstomumuandxenon100data AT isidorig thecmssmandnuhm1inlightof7tevlhcbstomumuandxenon100data AT marrouchej thecmssmandnuhm1inlightof7tevlhcbstomumuandxenon100data AT martinezsantosd thecmssmandnuhm1inlightof7tevlhcbstomumuandxenon100data AT nakachs thecmssmandnuhm1inlightof7tevlhcbstomumuandxenon100data AT oliveka thecmssmandnuhm1inlightof7tevlhcbstomumuandxenon100data AT rogersons thecmssmandnuhm1inlightof7tevlhcbstomumuandxenon100data AT rongafj thecmssmandnuhm1inlightof7tevlhcbstomumuandxenon100data AT devrieskj thecmssmandnuhm1inlightof7tevlhcbstomumuandxenon100data AT weigleing thecmssmandnuhm1inlightof7tevlhcbstomumuandxenon100data AT buchmuellero cmssmandnuhm1inlightof7tevlhcbstomumuandxenon100data AT cavanaughr cmssmandnuhm1inlightof7tevlhcbstomumuandxenon100data AT citronm cmssmandnuhm1inlightof7tevlhcbstomumuandxenon100data AT deroecka cmssmandnuhm1inlightof7tevlhcbstomumuandxenon100data AT dolanmj cmssmandnuhm1inlightof7tevlhcbstomumuandxenon100data AT ellisjr cmssmandnuhm1inlightof7tevlhcbstomumuandxenon100data AT flacherh cmssmandnuhm1inlightof7tevlhcbstomumuandxenon100data AT heinemeyers cmssmandnuhm1inlightof7tevlhcbstomumuandxenon100data AT isidorig cmssmandnuhm1inlightof7tevlhcbstomumuandxenon100data AT marrouchej cmssmandnuhm1inlightof7tevlhcbstomumuandxenon100data AT martinezsantosd cmssmandnuhm1inlightof7tevlhcbstomumuandxenon100data AT nakachs cmssmandnuhm1inlightof7tevlhcbstomumuandxenon100data AT oliveka cmssmandnuhm1inlightof7tevlhcbstomumuandxenon100data AT rogersons cmssmandnuhm1inlightof7tevlhcbstomumuandxenon100data AT rongafj cmssmandnuhm1inlightof7tevlhcbstomumuandxenon100data AT devrieskj cmssmandnuhm1inlightof7tevlhcbstomumuandxenon100data AT weigleing cmssmandnuhm1inlightof7tevlhcbstomumuandxenon100data |