Supersymmetry breaking and the supersymmetric flavor problem: An analysis of decoupling the first two generation scalars

The supersymmetric contributions to the flavor changing neutral current processes may be suppressed by decoupling the scalers of the first and second generations. It is known, however, that the heavy scalars drive the top squark mass squareds negative through the two-loop renormalization group evolution. This tension is studied in detail. Two new items are included in this analysis: the effect of the top quark Yukawa coupling and the QCD corrections to the supersymmetric contributions to Delta m(K). Even with Cabibbo-like degeneracy between the squarks of the first two generations, these squarks must be heavier than similar to 40 TeV to suppress Delta m(K). This implies, in the case of a high scale of supersymmetry breaking, that the boundary value of the top squark mass has to be greater than similar to 7 TeV to keep the top squark mass squared positive at the weak scale. Low-energy supersymmetry breaking at a scale that is of the same order as the mass of the heavy scalars is also considered. In this case the finite parts of the two-loop diagrams are computed to estimate the contribution of the heavy scaler masses to the top squark mass squared. It is found that for Cabibbo-like mixing between the squarks, the top squark mass at the boundary needs to be larger than similar to 2 TeV. Thus, for both cases, the large boundary value of the top squark masses leads to an unnatural amount of fine tuning to obtain the comet Z mass. [S0556-2821(98)04023-5].