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A precision study of the fine tuning in the DiracNMSSM

Recently the DiracNMSSM has been proposed as a possible solution to reduce the fine tuning in supersymmetry. We determine the degree of fine tuning needed in the DiracNMSSM with and without non-universal gaugino masses and compare it with the fine tuning in the GNMSSM. To apply reasonable cuts on th...

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Detalles Bibliográficos
Autores principales: Kaminska, Anna, Ross, Graham G., Schmidt-Hoberg, Kai, Staub, Florian
Lenguaje:eng
Publicado: 2014
Materias:
Acceso en línea:https://dx.doi.org/10.1007/JHEP06(2014)153
http://cds.cern.ch/record/1642049
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author Kaminska, Anna
Ross, Graham G.
Schmidt-Hoberg, Kai
Staub, Florian
author_facet Kaminska, Anna
Ross, Graham G.
Schmidt-Hoberg, Kai
Staub, Florian
author_sort Kaminska, Anna
collection CERN
description Recently the DiracNMSSM has been proposed as a possible solution to reduce the fine tuning in supersymmetry. We determine the degree of fine tuning needed in the DiracNMSSM with and without non-universal gaugino masses and compare it with the fine tuning in the GNMSSM. To apply reasonable cuts on the allowed parameter regions we perform a precise calculation of the Higgs mass. In addition, we include the limits from direct SUSY searches and dark matter abundance. We find that both models are comparable in terms of fine tuning, with the minimal fine tuning in the GNMSSM slightly smaller.
id cern-1642049
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2014
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spelling cern-16420492022-08-10T20:09:46Zdoi:10.1007/JHEP06(2014)153http://cds.cern.ch/record/1642049engKaminska, AnnaRoss, Graham G.Schmidt-Hoberg, KaiStaub, FlorianA precision study of the fine tuning in the DiracNMSSMParticle Physics - PhenomenologyRecently the DiracNMSSM has been proposed as a possible solution to reduce the fine tuning in supersymmetry. We determine the degree of fine tuning needed in the DiracNMSSM with and without non-universal gaugino masses and compare it with the fine tuning in the GNMSSM. To apply reasonable cuts on the allowed parameter regions we perform a precise calculation of the Higgs mass. In addition, we include the limits from direct SUSY searches and dark matter abundance. We find that both models are comparable in terms of fine tuning, with the minimal fine tuning in the GNMSSM slightly smaller.Recently the DiracNMSSM has been proposed as a possible solution to reduce the fine tuning in supersymmetry. We determine the degree of fine tuning needed in the DiracNMSSM with and without non-universal gaugino masses and compare it with the fine tuning in the GNMSSM. To apply reasonable cuts on the allowed parameter regions we perform a precise calculation of the Higgs mass. In addition, we include the limits from direct SUSY searches and dark matter abundance. We find that both models are comparable in terms of fine tuning, with the minimal fine tuning in the GNMSSM slightly smaller.arXiv:1401.1816DESY-13-256OUTP-13-25PCERN-PH-TH-2014-002BONN-TH-2014-01DESY-13-256OUTP-13-25PCERN-PH-TH-2014-002BONN-TH-2014-01oai:cds.cern.ch:16420492014-01-08
spellingShingle Particle Physics - Phenomenology
Kaminska, Anna
Ross, Graham G.
Schmidt-Hoberg, Kai
Staub, Florian
A precision study of the fine tuning in the DiracNMSSM
title A precision study of the fine tuning in the DiracNMSSM
title_full A precision study of the fine tuning in the DiracNMSSM
title_fullStr A precision study of the fine tuning in the DiracNMSSM
title_full_unstemmed A precision study of the fine tuning in the DiracNMSSM
title_short A precision study of the fine tuning in the DiracNMSSM
title_sort precision study of the fine tuning in the diracnmssm
topic Particle Physics - Phenomenology
url https://dx.doi.org/10.1007/JHEP06(2014)153
http://cds.cern.ch/record/1642049
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