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The fine-tuning price of LEP

We quantify the amount of fine tuning of input parameters of the Minimal Supersymmetric Extension of the Standard Model (MSSM) that is needed to respect the lower limits on sparticle and Higgs masses imposed by precision electroweak measurements at LEP, measurements of $b\to X_s\gamma$, and searches...

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Detalles Bibliográficos
Autores principales: Chankowski, Piotr H., Ellis, John R., Pokorski, Stefan
Lenguaje:eng
Publicado: 1997
Materias:
Acceso en línea:https://dx.doi.org/10.1016/S0370-2693(98)00060-4
http://cds.cern.ch/record/339939
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author Chankowski, Piotr H.
Ellis, John R.
Pokorski, Stefan
author_facet Chankowski, Piotr H.
Ellis, John R.
Pokorski, Stefan
author_sort Chankowski, Piotr H.
collection CERN
description We quantify the amount of fine tuning of input parameters of the Minimal Supersymmetric Extension of the Standard Model (MSSM) that is needed to respect the lower limits on sparticle and Higgs masses imposed by precision electroweak measurements at LEP, measurements of $b\to X_s\gamma$, and searches at LEP 2. If universal input scalar masses are assumed in a gravity-mediated scenario, a factor of $\gappeq180$ is required at $\tan\beta\sim1.65$, decreasing to if non-universal input scalar Higgs masses are allowed, but may be significantly reduced if some theoretical relations between MSSM parameters are assumed.
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spelling cern-3399392023-03-14T18:55:01Zdoi:10.1016/S0370-2693(98)00060-4http://cds.cern.ch/record/339939engChankowski, Piotr H.Ellis, John R.Pokorski, StefanThe fine-tuning price of LEPParticle Physics - PhenomenologyWe quantify the amount of fine tuning of input parameters of the Minimal Supersymmetric Extension of the Standard Model (MSSM) that is needed to respect the lower limits on sparticle and Higgs masses imposed by precision electroweak measurements at LEP, measurements of $b\to X_s\gamma$, and searches at LEP 2. If universal input scalar masses are assumed in a gravity-mediated scenario, a factor of $\gappeq180$ is required at $\tan\beta\sim1.65$, decreasing to if non-universal input scalar Higgs masses are allowed, but may be significantly reduced if some theoretical relations between MSSM parameters are assumed.We quantify the amount of fine tuning of input parameters of the Minimal Supersymmetric Extension of the Standard Model (MSSM) that is needed to respect the lower limits on sparticle and Higgs masses imposed by precision electroweak measurements at LEP, measurements of $b\to X_s\gamma$, and searches at LEP 2. If universal input scalar masses are assumed in a gravity-mediated scenario, a factor of $\gappeq180$ is required at $\tan\beta\sim1.65$, decreasing to $\sim20$ at $\tan\beta\sim10$. The amount of fine tuning is not greatly reduced if non-universal input scalar Higgs masses are allowed, but may be significantly reduced if some theoretical relations between MSSM parameters are assumed.We quantify the amount of fine tuning of input parameters of the Minimal Supersymmetric Extension of the Standard Model (MSSM) that is needed to respect the lower limits on sparticle and Higgs masses imposed by precision electroweak measurements at LEP, measurements of b → X s γ , and searches at LEP 2. If universal input scalar masses are assumed in a gravity-mediated scenario, a factor of ≳180 is required at tan β ∼1.65, decreasing to ∼20 at tan β ∼10. The amount of fine tuning is not greatly reduced if non-universal input scalar Higgs masses are allowed, but may be significantly reduced if some theoretical relations between MSSM parameters are assumed.hep-ph/9712234CERN-TH-97-343IFT-97-19CERN-TH-97-343IFT-97-19oai:cds.cern.ch:3399391997-12-03
spellingShingle Particle Physics - Phenomenology
Chankowski, Piotr H.
Ellis, John R.
Pokorski, Stefan
The fine-tuning price of LEP
title The fine-tuning price of LEP
title_full The fine-tuning price of LEP
title_fullStr The fine-tuning price of LEP
title_full_unstemmed The fine-tuning price of LEP
title_short The fine-tuning price of LEP
title_sort fine-tuning price of lep
topic Particle Physics - Phenomenology
url https://dx.doi.org/10.1016/S0370-2693(98)00060-4
http://cds.cern.ch/record/339939
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