Orateur
Dr
Andreas Crivellin
(ITP Bern)
Description
In this talk I review the consequences of radiative flavour violation in the MSSM. Since self-energies can be chirally enhanced and therefore of order one it is possible to generate the light-quark masses and the CKM matrix via loops. In the case of CKM generation in the down-sector constraints from b->s gamma, and in the case of CKM generation in the up-sector from epsilon_K, are observed. In the second case the rare decay K-> pi nu nu receives sizable contributions while in the first case additional contributions to B_s->mu mu via neutral Higgs penguins occur. These Higgs penguins can also contribute to Bs mixing and are capable to explain the observed CP asymmetry. In conclusion I show that for SUSY masses around 1 TeV radiative flavour-violation is an interesting solution to the SUSY flavour and CP problem.
Auteurs principaux
Dr
Andreas Crivellin
(ITP Bern)
Dr
Dominik Scherer
(TTP Karlsruhe)
Dr
Lars Hofer
(Universität Würzburg)
Prof.
Ulrich Nierste
(TTP Karlsruhe)
