Light stops and fine-tuning in MSSM
Abstract We discuss the fine-tuning issue within the MSSM framework. Following the idea that the fine-tuning can measure effects of some missing mechanism, we impose non-universal gaugino masses at the GUT scale, and explore the low scale implications. We realize that the fine-tuning parametrized wi...
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doaj-e12e4b446034445b9099f4346e26182f2020-11-24T21:18:58ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522018-01-0178111410.1140/epjc/s10052-018-5549-yLight stops and fine-tuning in MSSMAli Çiçi0Zerrin Kırca1Cem Salih Ün2Department of Physics, Uludag̃ UniversityDepartment of Physics, Uludag̃ UniversityDepartment of Physics, Uludag̃ UniversityAbstract We discuss the fine-tuning issue within the MSSM framework. Following the idea that the fine-tuning can measure effects of some missing mechanism, we impose non-universal gaugino masses at the GUT scale, and explore the low scale implications. We realize that the fine-tuning parametrized with $$\Delta _{EW}$$ ΔEW can be as low as zero. We consider the stop mass with a special importance and focus on the mass scales as $$m_{\tilde{t}} \le 700$$ mt~≤700 GeV, which are excluded by the current experiments when the stop decays into a neutralino along with a top quark or a chargino along with a bottom quark. We find that the stop mass can be as low as about 250 GeV with $$\Delta _{EW} \sim 50$$ ΔEW∼50 . We find that the solutions in this region can be exluded only up to $$60\%$$ 60% when stop decays into a neutralino-top quark, and $$50\%$$ 50% when it decays into a chargino-b quark. Setting $$65\%$$ 65% CL to be potential exclusion and $$95\%$$ 95% to be pure exclusion limit such solutions will be tested in near future experiments, which are conducted with higher luminosity. In addition to stop, the region with low fine-tuning and light stops predicts masses for the other supersymmetric particles such as $$m_{\tilde{b}} \gtrsim 700$$ mb~≳700 GeV, $$m_{\tilde{\tau }} \gtrsim 1$$ mτ~≳1 TeV, $$m_{\tilde{\chi }_{1}^{\pm }} \gtrsim 120$$ mχ~1±≳120 GeV. The details for the mass scales and decay rates are also provided by tables of benchmark points.http://link.springer.com/article/10.1140/epjc/s10052-018-5549-y |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Ali Çiçi Zerrin Kırca Cem Salih Ün |
spellingShingle |
Ali Çiçi Zerrin Kırca Cem Salih Ün Light stops and fine-tuning in MSSM European Physical Journal C: Particles and Fields |
author_facet |
Ali Çiçi Zerrin Kırca Cem Salih Ün |
author_sort |
Ali Çiçi |
title |
Light stops and fine-tuning in MSSM |
title_short |
Light stops and fine-tuning in MSSM |
title_full |
Light stops and fine-tuning in MSSM |
title_fullStr |
Light stops and fine-tuning in MSSM |
title_full_unstemmed |
Light stops and fine-tuning in MSSM |
title_sort |
light stops and fine-tuning in mssm |
publisher |
SpringerOpen |
series |
European Physical Journal C: Particles and Fields |
issn |
1434-6044 1434-6052 |
publishDate |
2018-01-01 |
description |
Abstract We discuss the fine-tuning issue within the MSSM framework. Following the idea that the fine-tuning can measure effects of some missing mechanism, we impose non-universal gaugino masses at the GUT scale, and explore the low scale implications. We realize that the fine-tuning parametrized with $$\Delta _{EW}$$ ΔEW can be as low as zero. We consider the stop mass with a special importance and focus on the mass scales as $$m_{\tilde{t}} \le 700$$ mt~≤700 GeV, which are excluded by the current experiments when the stop decays into a neutralino along with a top quark or a chargino along with a bottom quark. We find that the stop mass can be as low as about 250 GeV with $$\Delta _{EW} \sim 50$$ ΔEW∼50 . We find that the solutions in this region can be exluded only up to $$60\%$$ 60% when stop decays into a neutralino-top quark, and $$50\%$$ 50% when it decays into a chargino-b quark. Setting $$65\%$$ 65% CL to be potential exclusion and $$95\%$$ 95% to be pure exclusion limit such solutions will be tested in near future experiments, which are conducted with higher luminosity. In addition to stop, the region with low fine-tuning and light stops predicts masses for the other supersymmetric particles such as $$m_{\tilde{b}} \gtrsim 700$$ mb~≳700 GeV, $$m_{\tilde{\tau }} \gtrsim 1$$ mτ~≳1 TeV, $$m_{\tilde{\chi }_{1}^{\pm }} \gtrsim 120$$ mχ~1±≳120 GeV. The details for the mass scales and decay rates are also provided by tables of benchmark points. |
url |
http://link.springer.com/article/10.1140/epjc/s10052-018-5549-y |
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AT alicici lightstopsandfinetuninginmssm AT zerrinkırca lightstopsandfinetuninginmssm AT cemsalihun lightstopsandfinetuninginmssm |
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