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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...
Autores principales: | , , , |
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Lenguaje: | eng |
Publicado: |
2014
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1007/JHEP06(2014)153 http://cds.cern.ch/record/1642049 |
_version_ | 1780934909026631680 |
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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 |
record_format | invenio |
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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