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Global fits of GUT-scale SUSY models with GAMBIT
We present the most comprehensive global fits to date of three supersymmetric models motivated by grand unification: the constrained minimal supersymmetric standard model (CMSSM), and its Non-Universal Higgs Mass generalisations NUHM1 and NUHM2. We include likelihoods from a number of direct and ind...
Autores principales: | , , , , , , , , , , , , , , , , , , , , , , , , |
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Lenguaje: | eng |
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2017
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1140/epjc/s10052-017-5167-0 http://cds.cern.ch/record/2266045 |
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author | Athron, Peter Balázs, Csaba Bringmann, Torsten Buckley, Andy Chrząszcz, Marcin Conrad, Jan Cornell, Jonathan M. Dal, Lars A. Edsjö, Joakim Farmer, Ben Jackson, Paul Krislock, Abram Kvellestad, Anders Mahmoudi, Farvah Martinez, Gregory D. Putze, Antje Raklev, Are Rogan, Christopher Ruiz de Austri, Roberto Saavedra, Aldo Savage, Christopher Scott, Pat Serra, Nicola Weniger, Christoph White, Martin |
author_facet | Athron, Peter Balázs, Csaba Bringmann, Torsten Buckley, Andy Chrząszcz, Marcin Conrad, Jan Cornell, Jonathan M. Dal, Lars A. Edsjö, Joakim Farmer, Ben Jackson, Paul Krislock, Abram Kvellestad, Anders Mahmoudi, Farvah Martinez, Gregory D. Putze, Antje Raklev, Are Rogan, Christopher Ruiz de Austri, Roberto Saavedra, Aldo Savage, Christopher Scott, Pat Serra, Nicola Weniger, Christoph White, Martin |
author_sort | Athron, Peter |
collection | CERN |
description | We present the most comprehensive global fits to date of three supersymmetric models motivated by grand unification: the constrained minimal supersymmetric standard model (CMSSM), and its Non-Universal Higgs Mass generalisations NUHM1 and NUHM2. We include likelihoods from a number of direct and indirect dark matter searches, a large collection of electroweak precision and flavour observables, direct searches for supersymmetry at LEP and Runs I and II of the LHC, and constraints from Higgs observables. Our analysis improves on existing results not only in terms of the number of included observables, but also in the level of detail with which we treat them, our sampling techniques for scanning the parameter space, and our treatment of nuisance parameters. We show that stau co-annihilation is now ruled out in the CMSSM at more than 95% confidence. Stop co-annihilation turns out to be one of the most promising mechanisms for achieving an appropriate relic density of dark matter in all three models, whilst avoiding all other constraints. We find high-likelihood regions of parameter space featuring light stops and charginos, making them potentially detectable in the near future at the LHC. We also show that tonne-scale direct detection will play a largely complementary role, probing large parts of the remaining viable parameter space, including essentially all models with multi-TeV neutralinos. |
id | cern-2266045 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2017 |
record_format | invenio |
spelling | cern-22660452022-04-19T06:06:46Zdoi:10.1140/epjc/s10052-017-5167-0http://cds.cern.ch/record/2266045engAthron, PeterBalázs, CsabaBringmann, TorstenBuckley, AndyChrząszcz, MarcinConrad, JanCornell, Jonathan M.Dal, Lars A.Edsjö, JoakimFarmer, BenJackson, PaulKrislock, AbramKvellestad, AndersMahmoudi, FarvahMartinez, Gregory D.Putze, AntjeRaklev, AreRogan, ChristopherRuiz de Austri, RobertoSaavedra, AldoSavage, ChristopherScott, PatSerra, NicolaWeniger, ChristophWhite, MartinGlobal fits of GUT-scale SUSY models with GAMBITastro-ph.COAstrophysics and Astronomyhep-phParticle Physics - PhenomenologyWe present the most comprehensive global fits to date of three supersymmetric models motivated by grand unification: the constrained minimal supersymmetric standard model (CMSSM), and its Non-Universal Higgs Mass generalisations NUHM1 and NUHM2. We include likelihoods from a number of direct and indirect dark matter searches, a large collection of electroweak precision and flavour observables, direct searches for supersymmetry at LEP and Runs I and II of the LHC, and constraints from Higgs observables. Our analysis improves on existing results not only in terms of the number of included observables, but also in the level of detail with which we treat them, our sampling techniques for scanning the parameter space, and our treatment of nuisance parameters. We show that stau co-annihilation is now ruled out in the CMSSM at more than 95% confidence. Stop co-annihilation turns out to be one of the most promising mechanisms for achieving an appropriate relic density of dark matter in all three models, whilst avoiding all other constraints. We find high-likelihood regions of parameter space featuring light stops and charginos, making them potentially detectable in the near future at the LHC. We also show that tonne-scale direct detection will play a largely complementary role, probing large parts of the remaining viable parameter space, including essentially all models with multi-TeV neutralinos.We present the most comprehensive global fits to date of three supersymmetric models motivated by grand unification: the Constrained Minimal Supersymmetric Standard Model (CMSSM), and its Non-Universal Higgs Mass generalisations NUHM1 and NUHM2. We include likelihoods from a number of direct and indirect dark matter searches, a large collection of electroweak precision and flavour observables, direct searches for supersymmetry at LEP and Runs I and II of the LHC, and constraints from Higgs observables. Our analysis improves on existing results not only in terms of the number of included observables, but also in the level of detail with which we treat them, our sampling techniques for scanning the parameter space, and our treatment of nuisance parameters. We show that stau co-annihilation is now ruled out in the CMSSM at more than 95\% confidence. Stop co-annihilation turns out to be one of the most promising mechanisms for achieving an appropriate relic density of dark matter in all three models, whilst avoiding all other constraints. We find high-likelihood regions of parameter space featuring light stops and charginos, making them potentially detectable in the near future at the LHC. We also show that tonne-scale direct detection will play a largely complementary role, probing large parts of the remaining viable parameter space, including essentially all models with multi-TeV neutralinos.arXiv:1705.07935COEPP-MN-17-9CERN-TH-2017-168NORDITA 2017-080CoEPP-MN-17-9gambit-physicsgambit-physics-2017oai:cds.cern.ch:22660452017-05-22 |
spellingShingle | astro-ph.CO Astrophysics and Astronomy hep-ph Particle Physics - Phenomenology Athron, Peter Balázs, Csaba Bringmann, Torsten Buckley, Andy Chrząszcz, Marcin Conrad, Jan Cornell, Jonathan M. Dal, Lars A. Edsjö, Joakim Farmer, Ben Jackson, Paul Krislock, Abram Kvellestad, Anders Mahmoudi, Farvah Martinez, Gregory D. Putze, Antje Raklev, Are Rogan, Christopher Ruiz de Austri, Roberto Saavedra, Aldo Savage, Christopher Scott, Pat Serra, Nicola Weniger, Christoph White, Martin Global fits of GUT-scale SUSY models with GAMBIT |
title | Global fits of GUT-scale SUSY models with GAMBIT |
title_full | Global fits of GUT-scale SUSY models with GAMBIT |
title_fullStr | Global fits of GUT-scale SUSY models with GAMBIT |
title_full_unstemmed | Global fits of GUT-scale SUSY models with GAMBIT |
title_short | Global fits of GUT-scale SUSY models with GAMBIT |
title_sort | global fits of gut-scale susy models with gambit |
topic | astro-ph.CO Astrophysics and Astronomy hep-ph Particle Physics - Phenomenology |
url | https://dx.doi.org/10.1140/epjc/s10052-017-5167-0 http://cds.cern.ch/record/2266045 |
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