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Contributors: G. Isidori and G. D'Ambrosio.
Kaon physics is one of the richest sources of information about the standard model of electroweak interactions (SM). The properties of kaons and their decay patterns provide stringent constraints on any extension of the SM[1] (e.g. , , , etc...).
Discussion centered on decay widths of modes dominated by short distance physics. These observables are of great interest because, even in absence of direct new physics contributions, their measurement would provide valuable information about the flavor structure of the SM. The best examples of such observables are the widths of the neutrino modes and [2]. These occur at second order in electroweak interactions and are virtually free from long-distance contamination. Top-quark loops make the dominant contribution to these decays because of the GIM mechanism and so the decays are sensitive to mixing between the third generation and the light s and d quarks.
The ratio can be calculated to better than 1(a precision currently unobtainable in calculations of B-meson decay modes), with uncertainty in the top mass increasing the uncertainty to 3[3]. Moreover, a combined measurement of and could determine complementarily and comparable to the cleanest CP asymmetry in B decays ( ) [4]. Many new physics models predict different sensitivity to the value of between rare kaon decays and B-meson decays [4,5]. The strong CKM suppression of amplitudes within the SM ( ) implies that even small new physics effects could produce sizable modifications to these decays rates, while not affecting B-meson decay modes. Two popular examples where sizable effects can be found are provided by supersymmetric extensions of the SM [6] and models with a fourth generation of quarks [7], even if the masses of the new particles are .
can be considered a short-distance observable if correlated with two other measurements: the rate of and a precise determination of the low diphoton invariant mass spectrum of [8]. Very interesting from a theoretical point of view but quite challenging is the measurement of the interference term.
The high statistics required to observe , , and decays will provide data in other channels as well. For example,
On the experimental front, an experiment on has been approved at KEK [12] which should reach a sensitivity on the branching ratio of around 10-10. This will be very useful for excluding some new physics scenarios but is not enough to reach the SM value. Two proposals, one at FNAL[13] and one at BNL[14], are slated to reach sensitivities around 10-12. One event has been observed by the Brookhaven experiment E787[15].
Next: Conclusion
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