“…In contrast, in SUSY scenarios the scalar and pseudo-scalar operators, O S,P , can be very important, particularly at large tan β > ∼ 30 where the contributions to C S and C P from neutral Higgs penguin diagrams can become large and dominate the branching ratio, because in this case the branching ratio grows with tan β as tan 6 β. The studies in the literature of these MSSM Higgs-penguin contributions to BR(B s → µ + µ − ) have focused on both MFV [54,66,67] and NMFV scenarios [33,56,61,64]. In both cases the rates for BR(B s → µ + µ − ) at large tan β can be enhanced by a few orders of magnitude compared with the prediction in the SM, therefore providing an optimal window for SUSY signals.…”