hadronc contributions to rare B-decays; rare B-decays; QCD corrections to electroweak processes; effective field theory; renormalization group improvements; SUSY contributions to rare decays; Determination of CKM matrix elements; new physics contributions to flavour observables
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This project on flavour physics embraces a major direction ofresearch that will be under investigation at the Institute of TheoreticalPhysics at the University of Bern. The main focus of this proposal is on multi-loop calculation forflavour observables in the quark sector and the charged lepton sector of the Standard Model(SM), the SM supplemented by gauge invariant dimension 6 operators, theTwo-Higgs-Doublet model (THDM), models with leptoquarks and the Minimal Supersymmetric Standard Model(MSSM). The proposal is divided into several subprojects:1.) Precision calculations in the standard modelA) Hadronic effects in $b\to s$ exclusive transitions at next-to-leading order}B) Contributions of the current-current operators to B -> X_s gamma gamma and implementation of the photon/hadron separation2.) Precision calculations in extensions of the SMC) B-physics phenomenology from the SM Effective Field TheoryD) Two-loop Renormalization Group Evolution of Dipole Operators in the gauge-invariant Effective Field TheoryE) Enhanced electroweak corrections to B -> X_s gamma in two-higgs-doublet modelsF) QCD corrections to the leptoquark induced l_i -> l_f gamma transitionsG) Two-loop electroweak contributions to quark-quark-Higgs couplings in the MSSMThe goal of the first part is the precise calculation of the SMcontributions to these flavour-changing neutral current (FCNC)processes. This is important in order to identify and quantify possible newphysics contributions and/or to obtain more stringent bounds on theflavour parameters.The second part aims at a better understanding of theflavour-structure in various extensions of the SM. On the one hand, this limits the allowed parameter-space ofthese models which gives important constraints for model building. On theother hand one can correlate the predictions for rare decays in these models andjudge whether (some of) these models could explain possible deviations from the SMpredictions.