b -> s γand supersymmetry with large tanβ

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dc.creatorCarena, M.
dc.creatorGarcia, D.
dc.creatorNierste, U.
dc.creatorWagner, C. E. M.
dc.date2000-10-02
dc.date2000-10-11
dc.date.accessioned2026-07-07T10:52:09Z
dc.date.available2026-07-07T10:52:09Z
dc.descriptionWe discuss the constraints on the supersymmetric parameter space from the decay mode b -> s γfor large values of tanβ. 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 tanβregime. This resummation of terms of order alpha_s^n tan^{n+1}βuses a recently proposed effective lagrangian for the Yukawa interaction of bottom quarks. Moreover, we identify an additional source of tanβ-enhanced terms, which are of order alpha_s tanβand 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 γconstrains the supersymmetric parameter space in a relevant way, even if tanβis large.
dc.description"Note added" changed, 2 references and 2 footnotes added
dc.identifierhttps://arxiv.org/abs/hep-ph/0010003
dc.identifierhttp://arxiv.org/abs/hep-ph/0010003
dc.identifierPhys.Lett.B499:141-146,2001
dc.identifierdoi:10.1016/S0370-2693(01)00009-0
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/185065
dc.subjectHigh Energy Physics - Phenomenology
dc.titleb -> s γand supersymmetry with large tanβ
dc.typetext

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