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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
Up: Kaon
Physics Previous: Speakers
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