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1 Introduction - Caltech High Energy Physics - California Institute of ...

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408 New <strong>Physics</strong><br />

CP violation from µ and At phases<br />

Let us first discuss minimal flavor violation models with effective SUSY spectra. In this model, flavor<br />

violation comes through the CKM matrix, whereas CP violation originates from the µ and At phases, as<br />

well as the CKM phase. The one loop electric dipole moment (EDM) constraint is evaded in the effective<br />

SUSY model due to the decoupling <strong>of</strong> the first/second generation sfermions, but there are potentially large<br />

two loop contribution to electron/neutron EDM’s through Barr-Zee type diagrams in the large tan β region<br />

[208]. Imposing this two-loop EDM constraint and direct search limits on Higgs and SUSY particles, we find<br />

that [209, 210]<br />

• There are no new phase shifts in B 0 B 0 and B 0 sB 0<br />

s mixing: Time-dependent CP asymmetries in Bd →<br />

J/ψ K 0 S still measure the CKM angle β = φ1 [Fig. 5-36 (a)]<br />

• ∆MBd can be enhanced up to ∼ 80% compared to the Standard Model prediction [Fig. 5-36 (b)]<br />

• Direct CP asymmetry in B → Xsγ (A b→sγ<br />

CP ) can be as large as ±15% [see Fig. 5-37]<br />

• Rµµ can be as large as 1.8<br />

• ɛK can differ from the Standard Model value by ∼ 40%<br />

One can therefore anticipate substantial deviations in certain observables in the B system in SUSY models<br />

with minimal flavor violation and complex µ and At parameters. This class <strong>of</strong> models include electroweak<br />

baryogenesis (EWBGEN) within the MSSM and some <strong>of</strong> its extensions (such as NMSSM), where the chargino<br />

and stop sectors are the same as in the MSSM. In the EWBGEN scenario within the MSSM, the current<br />

lower limit on the Higgs mass requires a large radiative correction from the stop loop. Since ˜tR has to be<br />

light to have a sufficiently strong 1st order electroweak phase transition, one has to have heavy ˜tL to induce<br />

a large ∆m2 h . After considering B → Xsγ, one expects a very small deviations in A b→sγ<br />

CP and ∆MBd [211].<br />

However, in some extensions <strong>of</strong> the MSSM, the tension between mh and m˜tL becomes significantly diluted<br />

in EWBGEN scenarios, because there could be tree level contributions to m2 h . Therefore, the predictions<br />

made in Refs. [209, 210] will be still valid in EWBGEN scenarios beyond the MSSM.<br />

Super B Factoriesshould be able to measure A b→sγ<br />

CP to higher accuracy, and will impose a strong constraint<br />

on a new CP -violating phase that could appear in B → Xsγ. Also the forward-backward asymmetries in<br />

B → Xsℓ + ℓ− with ℓ = e or µ are equally important probes <strong>of</strong> new CP -violating phases, and important<br />

observables to be measured at Super B Factories, for which LHCb or BTeV cannot compete.<br />

CP violation from gluino-squark loops<br />

In effective SUSY scenarios, it is possible that the gluino-mediated b → s transition is dominant over other<br />

SUSY contributions. Cohen et al. have described qualitative features <strong>of</strong> such scenarios in B physics [212]; a<br />

more quantitative analysis was presented by other groups. In Ref. [213], effects <strong>of</strong> possible new CP -violating<br />

phases on B → Xsγ and B → Xsℓ + ℓ− were considered both in a model-independent manner, and in gluino<br />

mediation dominance scenario. In effective SUSY models, A b→sγ<br />

CP<br />

can be as large as ±10%, if the third<br />

generation squarks are light enough m˜ b � (100 − 200) GeV (see Fig. 5-38), whereas B → Xsℓ + ℓ − is almost<br />

the same as the Standard Model prediction [213].<br />

How to distinguish the µ or At phase from the δ d 23 phase<br />

Should we find deviations in sin 2βφK0 or Ab→sγ<br />

S CP , it will be very important to figure out the origin <strong>of</strong> new CP -<br />

violating phases. In an effective SUSY context, one has complex At, µ or (δd AB )23 (with A, B = L, R). The<br />

effects <strong>of</strong> these new complex parameters on some oservables in the B system are shown in Table 5-16. The<br />

only process which is not directly affected by gluino-mediated FCNC is B → Xsνν. All the other observables<br />

The Discovery Potential <strong>of</strong> a Super B Factory

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