New Physics Patterns in ε′/ε\varepsilon^\prime/\varepsilon and εK\varepsilon_K with Implications for Rare Kaon Decays and ΔMKΔM_K

preprint2016arXivOpen access

Abstract

The SM prediction for the ratio ε′/ε\varepsilon^\prime/\varepsilon appears to be significantly below the experimental data. Also εK\varepsilon_K in the SM tends to be below the data. Any NP removing these anomalies will first of all have impact on flavour observables in the KK meson system, in particular on rare KK decays and ΔMKΔM_K. Restricting the operators contributing to ε′/ε\varepsilon^\prime/\varepsilon to the SM ones and to the corresponding primed operators, NP contributions are quite generally dominated either by QCD penguin (QCDP) operators Q6(Q6′)Q_6(Q_6^\prime) or electroweak penguin (EWP) operators Q8(Q8′)Q_8(Q_8^\prime) with rather different implications for other flavour observables. We discuss general models with tree-level ZZ and Z′Z^\prime flavour violating exchanges and few specific models. We find that simultaneous enhancements of ε′/ε\varepsilon^\prime/\varepsilon, εK\varepsilon_K, B(KL→π0ννˉ)\mathcal{B}(K_L\toπ^0ν\barν) and B(K+→π+ννˉ)\mathcal{B}(K^+\toπ^+ν\barν) in ZZ scenarios are only possible in the presence of both LH and RH flavour-violating couplings. In Z′Z^\prime scenarios this is not required but the size of NP effects and the correlation between B(KL→π0ννˉ)\mathcal{B}(K_L\toπ^0ν\barν) and B(K+→π+ννˉ)\mathcal{B}(K^+\toπ^+ν\barν) depends strongly on whether QCDP or EWP dominate NP contributions to ε′/ε\varepsilon^\prime/\varepsilon. In the QCDP case possible enhancements of both branching ratios are much larger than for EWP scenario and take place only on the branch parallel to the Grossman-Nir bound, which is in the case of EWP dominance only possible in the absence of NP in εK\varepsilon_K. QCDP and EWP scenarios of NP in ε′/ε\varepsilon^\prime/\varepsilon can also be uniquely distinguished by the size and the sign of NP contribution to ΔMKΔM_K, elevating the importance of the precise calculation of ΔMKΔM_K in the SM.

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