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The MSSM with large tan(beta) and heavy squarks is a theoretically wellmotivated and phenomenologically interesting extension of the SM. This scenarionaturally accommodates the (g-2)_\mu anomaly and the upper bound on the Higgsboson mass. In a wide region of the parameter space, visible non-standardeffects are expected in a few low-energy observables, such as BR(B->tau nu),BR(B->l+ l-), BR(B->Xs gamma), and BR(mu->e gamma). We analyse the correlationsof these non-standard effects under the additional assumption that the relicdensity of a Bino-like LSP accommodates the observed dark matter distribution.Comment: 19 pages, 7 figures; v2: published version (minor modifications

physical review. d. particles, fields, gravitation, and cosmology/physical review. d, particles, fields, gravitation, and cosmology

Flavor physics at large tan<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>β</mml:mi></mml:math>with a binolike lightest supersymmetric particle

Flavor physics at large tanβwith a binolike lightest supersymmetric particle