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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...

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Detalles Bibliográficos
Autores principales: 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
Lenguaje:eng
Publicado: 2017
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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