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Radiative corrections to the decay H --> hh in the minimal supersymmetric Standard Model
We set up a suitable renormalization programme for the one-loop computation of the decay rate Gamma(H==>hh) in the Minimal Supersymmetric extension of the Standard Model. We then perform an explicit diagrammatic calculation, including the full contributions from top, bottom, stop and sbottom loop...
Autores principales: | , |
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Lenguaje: | eng |
Publicado: |
1993
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1016/0370-2693(93)90885-L http://cds.cern.ch/record/242653 |
_version_ | 1780885063441842176 |
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author | Brignole, A. Zwirner, F. |
author_facet | Brignole, A. Zwirner, F. |
author_sort | Brignole, A. |
collection | CERN |
description | We set up a suitable renormalization programme for the one-loop computation of the decay rate Gamma(H==>hh) in the Minimal Supersymmetric extension of the Standard Model. We then perform an explicit diagrammatic calculation, including the full contributions from top, bottom, stop and sbottom loops. We find that, for tan(beta) close to 1, and m_H greater than or approximately equal to 2 m_t, the results can significantly differ from those previously obtained in the effective potential approach. However, the latter method remains a good approximation in the region of parameter space which is most relevant for H searches at large hadron colliders. |
id | cern-242653 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 1993 |
record_format | invenio |
spelling | cern-2426532023-03-14T19:28:31Zdoi:10.1016/0370-2693(93)90885-Lhttp://cds.cern.ch/record/242653engBrignole, A.Zwirner, F.Radiative corrections to the decay H --> hh in the minimal supersymmetric Standard ModelParticle Physics - TheoryParticle Physics - PhenomenologyWe set up a suitable renormalization programme for the one-loop computation of the decay rate Gamma(H==>hh) in the Minimal Supersymmetric extension of the Standard Model. We then perform an explicit diagrammatic calculation, including the full contributions from top, bottom, stop and sbottom loops. We find that, for tan(beta) close to 1, and m_H greater than or approximately equal to 2 m_t, the results can significantly differ from those previously obtained in the effective potential approach. However, the latter method remains a good approximation in the region of parameter space which is most relevant for H searches at large hadron colliders.We set up a suitable renormalization programme for the one-loop computation of the decay rate Gamma(H==>hh) in the Minimal Supersymmetric extension of the Standard Model. We then perform an explicit diagrammatic calculation, including the full contributions from top, bottom, stop and sbottom loops. We find that, for tan(beta) close to 1, and m_H greater than or approximately equal to 2 m_t, the results can significantly differ from those previously obtained in the effective potential approach. However, the latter method remains a good approximation in the region of parameter space which is most relevant for H searches at large hadron colliders.We set up a suitable renormalization programme for the one-loop computation of the decay rate Gamma(H==>hh) in the Minimal Supersymmetric extension of the Standard Model. We then perform an explicit diagrammatic calculation, including the full contributions from top, bottom, stop and sbottom loops. We find that, for tan(beta) close to 1, and m_H greater than or approximately equal to 2 m_t, the results can significantly differ from those previously obtained in the effective potential approach. However, the latter method remains a good approximation in the region of parameter space which is most relevant for H searches at large hadron colliders.We set up a suitable renormalization programme for the one-loop computation of the decay rate Γ ( H → hh ) in the minimal supersymmetric extension of the standard model. We then perform an explicit diagrammatic calculation, including the full contributions from top, bottom, stop and sbottom loops. We find that, for tan β close to 1 and m H ⪆ 2m t , the results can significantly differ from those previously obtained in the effective potential approach. However, the latter method remains a good approximation in the region of parameter space which is most relevant for H searches at large hadron colliders.hep-ph/9210266CERN-TH-6603-92CERN-TH-6603-92oai:cds.cern.ch:2426531993 |
spellingShingle | Particle Physics - Theory Particle Physics - Phenomenology Brignole, A. Zwirner, F. Radiative corrections to the decay H --> hh in the minimal supersymmetric Standard Model |
title | Radiative corrections to the decay H --> hh in the minimal supersymmetric Standard Model |
title_full | Radiative corrections to the decay H --> hh in the minimal supersymmetric Standard Model |
title_fullStr | Radiative corrections to the decay H --> hh in the minimal supersymmetric Standard Model |
title_full_unstemmed | Radiative corrections to the decay H --> hh in the minimal supersymmetric Standard Model |
title_short | Radiative corrections to the decay H --> hh in the minimal supersymmetric Standard Model |
title_sort | radiative corrections to the decay h --> hh in the minimal supersymmetric standard model |
topic | Particle Physics - Theory Particle Physics - Phenomenology |
url | https://dx.doi.org/10.1016/0370-2693(93)90885-L http://cds.cern.ch/record/242653 |
work_keys_str_mv | AT brignolea radiativecorrectionstothedecayhhhintheminimalsupersymmetricstandardmodel AT zwirnerf radiativecorrectionstothedecayhhhintheminimalsupersymmetricstandardmodel |