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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...

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Detalles Bibliográficos
Autores principales: Carena, Marcela, Garcia, David, Nierste, Ulrich, Wagner, Carlos E.M.
Lenguaje:eng
Publicado: 2000
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.
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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