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$b \to s \gamma$ and supersymmetry with large $\beta$
We discuss the constraints on the supersymmetric parameter space from the decay mode b -> s \gamma for large values of tan\beta. We improve the theoretical prediction for the decay rate by summing very large radiative corrections to all orders in perturbation theory. This extends the validity of...
Autores principales: | , , , |
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Lenguaje: | eng |
Publicado: |
2000
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1016/S0370-2693(01)00009-0 http://cds.cern.ch/record/467082 |
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author | Carena, Marcela Garcia, David Nierste, Ulrich Wagner, Carlos E.M. |
author_facet | Carena, Marcela Garcia, David Nierste, Ulrich Wagner, Carlos E.M. |
author_sort | Carena, Marcela |
collection | CERN |
description | We discuss the constraints on the supersymmetric parameter space from the decay mode b -> s \gamma for large values of tan\beta. We improve the theoretical prediction for the decay rate by summing very large radiative corrections to all orders in perturbation theory. This extends the validity of the perturbative calculation to the large tan\beta regime. This resummation of terms of order alpha_s^n tan^{n+1}\beta uses a recently proposed effective lagrangian for the Yukawa interaction of bottom quarks. Moreover, we identify an additional source of tan\beta-enhanced terms, which are of order alpha_s tan\beta and involve the charged Higgs boson, and analyze their behaviour in higher orders of perturbation theory. After correcting the current expressions for this rare decay branching ratio at next-to-leading order, we obtain that, contrary to recent claims, the presently measured branching ratio of b -> s \gamma constrains the supersymmetric parameter space in a relevant way, even if tan\beta is large. |
id | cern-467082 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2000 |
record_format | invenio |
spelling | cern-4670822023-01-31T08:15:13Zdoi:10.1016/S0370-2693(01)00009-0http://cds.cern.ch/record/467082engCarena, MarcelaGarcia, DavidNierste, UlrichWagner, Carlos E.M.$b \to s \gamma$ and supersymmetry with large $\beta$Particle Physics - PhenomenologyWe discuss the constraints on the supersymmetric parameter space from the decay mode b -> s \gamma for large values of tan\beta. We improve the theoretical prediction for the decay rate by summing very large radiative corrections to all orders in perturbation theory. This extends the validity of the perturbative calculation to the large tan\beta regime. This resummation of terms of order alpha_s^n tan^{n+1}\beta uses a recently proposed effective lagrangian for the Yukawa interaction of bottom quarks. Moreover, we identify an additional source of tan\beta-enhanced terms, which are of order alpha_s tan\beta and involve the charged Higgs boson, and analyze their behaviour in higher orders of perturbation theory. After correcting the current expressions for this rare decay branching ratio at next-to-leading order, we obtain that, contrary to recent claims, the presently measured branching ratio of b -> s \gamma constrains the supersymmetric parameter space in a relevant way, even if tan\beta is large.We discuss the constraints on the supersymmetric parameter space from the decay mode b -> s \gamma for large values of tan\beta. We improve the theoretical prediction for the decay rate by summing very large radiative corrections to all orders in perturbation theory. This extends the validity of the perturbative calculation to the large tan\beta regime. This resummation of terms of order alpha_s^n tan^{n+1}\beta uses a recently proposed effective lagrangian for the Yukawa interaction of bottom quarks. Moreover, we identify an additional source of tan\beta-enhanced terms, which are of order alpha_s tan\beta and involve the charged Higgs boson, and analyze their behaviour in higher orders of perturbation theory. After correcting the current expressions for this rare decay branching ratio at next-to-leading order, we obtain that, contrary to recent claims, the presently measured branching ratio of b -> s \gamma constrains the supersymmetric parameter space in a relevant way, even if tan\beta is large.We discuss the constraints on the supersymmetric parameter space from the decay mode b -> s \gamma for large values of tan\beta. We improve the theoretical prediction for the decay rate by summing very large radiative corrections to all orders in perturbation theory. This extends the validity of the perturbative calculation to the large tan\beta regime. This resummation of terms of order alpha_s^n tan^{n+1}\beta uses a recently proposed effective lagrangian for the Yukawa interaction of bottom quarks. Moreover, we identify an additional source of tan\beta-enhanced terms, which are of order alpha_s tan\beta and involve the charged Higgs boson, and analyze their behaviour in higher orders of perturbation theory. After correcting the current expressions for this rare decay branching ratio at next-to-leading order, we obtain that, contrary to recent claims, the presently measured branching ratio of b -> s \gamma constrains the supersymmetric parameter space in a relevant way, even if tan\beta is large.We discuss the constraints on the supersymmetric parameter space from the decay mode b → sγ for large values of tan β . We improve the theoretical prediction for the decay rate by summing very large radiative corrections to all orders in perturbation theory. This extends the validity of the perturbative calculation to the large tan β regime. This resummation of terms of order α s n tan n +1 β is based on a recently proposed effective Lagrangian for the Yukawa interaction of bottom quarks. Moreover, we identify an additional source of tan β -enhanced terms, which are of order α s tan β and involve the charged Higgs boson, and analyse their behaviour in higher orders of perturbation theory. After correcting the current expressions for this rare decay branching ratio at next-to-leading order, we obtain that, contrary to recent claims, the measured branching ratio of b → sγ constrains the supersymmetric parameter space in a relevant way, even if tan β is large.hep-ph/0010003FERMILAB-PUB-00-242-TCERN-TH-2000-295SCIPP-00-34ANL-HEP-PR-00-104EFI-2000-35CERN-TH-2000-295EFI-2000-35-[CHICAGO]FERMILAB-PUB-2000-242-TSCIPP-2000-43oai:cds.cern.ch:4670822000-10-02 |
spellingShingle | Particle Physics - Phenomenology Carena, Marcela Garcia, David Nierste, Ulrich Wagner, Carlos E.M. $b \to s \gamma$ and supersymmetry with large $\beta$ |
title | $b \to s \gamma$ and supersymmetry with large $\beta$ |
title_full | $b \to s \gamma$ and supersymmetry with large $\beta$ |
title_fullStr | $b \to s \gamma$ and supersymmetry with large $\beta$ |
title_full_unstemmed | $b \to s \gamma$ and supersymmetry with large $\beta$ |
title_short | $b \to s \gamma$ and supersymmetry with large $\beta$ |
title_sort | $b \to s \gamma$ and supersymmetry with large $\beta$ |
topic | Particle Physics - Phenomenology |
url | https://dx.doi.org/10.1016/S0370-2693(01)00009-0 http://cds.cern.ch/record/467082 |
work_keys_str_mv | AT carenamarcela btosgammaandsupersymmetrywithlargebeta AT garciadavid btosgammaandsupersymmetrywithlargebeta AT niersteulrich btosgammaandsupersymmetrywithlargebeta AT wagnercarlosem btosgammaandsupersymmetrywithlargebeta |