According to the previous considerations, accurate measurements of the
Dalitz plot for the individual channels would allow a stringent
test of the current theoretical description of the
nonleptonic weak interaction, in particular of the
chiral Lagrangian realization to order
. The determination of isospin
amplitudes requires, in general, the combination of data on both
and
decays. DA
NE is a source of pure kaon beams, free from background
contaminations, which in principle should allow high statistical accuracy
(see Tab. 1), provided that detection efficiencies for decay products are also
high. However, in some cases the present experimental accuracy is mostly
limited by systematic errors that must be decreased accordingly, in order
to take advantage of the quality of kaon beams. Another source of
difficulty, to be taken into account in
analyses, is the
correlations among, e.g., linear and quadratic Dalitz plot slopes, which
relate the accuracies obtainable for these parameters. The case of
is a special one, since the quadratic slope
is not contaminated by the linear amplitude which is zero for this mode
(see Eq. (14)), and electromagnetic corrections are not
required.
The direct observation of many hundreds of decay
events, with practically no background (see Tab. 1), should represent a
significant achievement obtainable at DA
NE and, as pointed out
previously, will allow to carefully test the
component of the
weak Hamiltonian.
Another interesting analysis of is suggested
by the use of DA
NE as an `interferometer', where the time dependence
of
-
interference in vacuum can be accurately studied. Since the
initial
state from
decay is the antisymmetric superposition
where is the direction of the kaons momenta in the c.m.
system, the subsequent
and
decays are correlated, and their
quantum interferences show up in relative time distributions and time
asymmetries, which are of great interest in order to test CP (and CPT)
violation [44]. In addition, as an alternative to the direct
observation, also the CP conserving
amplitude and the final state interaction imaginary parts could be
measured via the time dependent interference of this decay with
[45,12].
Specifically, a convenient observable is represented by
the transition rate for the initial state to decay into the
final states
at time
and
at time
, respectively (in the following,
and
are understood to be the proper times). Defining the
`intensity' of time correlated
events
as:
where and t is the time difference
, making use
of the exponential time-dependence of the mass eigenstates K
and K
,
and integrating over the
phase space, one easily finds,
with the notations
:
and
In Eqs. (40) and (41), ,
, and for the
amplitudes the expansions
(14) or (15) must be introduced.
>From these equations one can notice the possibility to study, in general,
also negative `times', which is peculiar of the
factory
[46].
An important aspect of the interference in (40) and (41) is that, besides the real parts, the (expectedly) small final state interaction imaginary parts appear linearly. Instead, the width depends quadratically on them and thus has less sensitivity to such effects. Accordingly, by a fit to the full t-dependence of the interference, both the real and the imaginary parts could be determined (or at least, for the latter ones, a significant upper bound could be obtained, depending on the available statistics). This would be a desirable achievement, in view of the discussion in Sec. 3.
Using Eq. (14) or (15), the interference terms are
easily seen to drop from the intensities (40) and (41)
integrated over the full Dalitz plot, giving the total
event rates. Considering that in the CP conserving case the Dalitz plot
distributions are even in X for all channels, the interference can be
extracted by integrating the intensities (40) and (41)
over the
phase space with odd-X cuts.
For example, with the phase space element, one can define the
asymmetries
and
Using Eq. (14) to expand
and
up to second order in
the kinematical variables, one finds to a good approximation
where
The amplitude (and
) can be measured from the rates.
Therefore, Eq. (44) shows that the separate determination of the
and
dependences
allows the measurement of the
amplitude
, as well
as of the rescattering relative phase
. In particular,
the leading order
predictions in Eq. (35)
indicate
.
The expression for is directly obtained from (44)
by the changes
,
and
but, as a function of time, the
denominator would quickly become large and suppress the interference.
Analogously, is given by the more complicated expression:
where
and
If separately determined, the coefficients of the
and
terms
could be useful to constrain the value of the quadratic amplitude
and the combination of imaginary parts in (47). In this regard,
we can notice that the expectedly small
has a large coefficient
proportional to
(see Tab. 4). In fact, to leading order in
, the numerator in Eq. (47) must be of order
(the same counting applies to
),
so that for theoretical consistency
, which is of order
, should
not be included. In that case, Eq. (47) simplifies considerably,
and using Eq. (35) we would predict
[12].
In conclusion, studies of the time-dependent interference described above
should provide alternative measurements of the CP conserving
amplitude, and eventually could also give indications on rescattering
phases and test the relevant predictions. A quantitative discussion for
DA
NE, taking into account also the background from the CP even
(
) state due to the radiative decay
, is presented in Ref. [44].