INFN - Laboratori Nazionali di Frascati, May 1995

From: The Second DAFNE Physics Handbook

Chapter 5: The $pipi$ Interaction

Eds. L. Maiani, G. Pancheri, N. Paver

Supported by the INFN, by the EC under the HCM contract number CHRX-CT920026 and by the authors home institutions.



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The Amplitude in


Generalized Chiral Perturbation Theory

M. Knecht B. Moussallam and J. Stern

Division de Physique Théorique gif, Institut de Physique Nucléaire
F-91406 Orsay Cedex, France

Abstract:

The interaction is studied at order one loop in the framework of Generalized Chiral Perturbation Theory.

The general requirements of analyticity, unitarity and crossing symmetry, together with the Goldstone nature of the pion and isospin invariance, determine a low energy representation of the scattering amplitude up to corrections of order [1], where denotes the scale at which particles other than pions can appear as intermediate states. This general representation depends on six independent low energy subtraction constants, which can be determined from experiment, given sufficiently precise data. Furthermore, only four of these constants (denoted as , , and in the sequel) appear if two loop contributions are neglected [1]:

 

with

 

and where stands for the usual loop function,

The corresponding scattering lengths and slope parameters are given as follows:

 

and

 

The above parametrization of the low energy behaviour of the amplitude and of the threshold parameters holds independently of more detailed considerations like, for instance, the value of the quark-antiquark condensate in the chiral limit. On the other hand, the expansions of , , , in powers of quark masses up to a given order will differ according to whether one assumes 1 GeV, or 100 MeV. In the sequel, we shall consider the amplitude up to and including order contributions only, within the framework of SU(3)SU(3) Generalized Chiral Perturbation Theory (GPT) [1,2]. This means that both in Eq. (1) for the scattering amplitude and in the expressions (4) and (5) for the threshold parameters, only the leading order expressions are to be retained for the parts that are quadratic in and . In particular, of Eq. (1) should be replaced by at that order, since the difference only affects contributions at orders and . The leading order expressions and and the higher order corrections are obtained from the effective lagrangian given in [2]. Expanding the contributions from and intermediate states in powers of , () and retaining only the dominant terms at order , one obtains the following result for and for ( is an arbitrary subtraction scale):

 

In these expressions, one recognizes the contributions coming from the tree diagrams, given in terms of the low energy constants , and , and the chiral logarithms coming from the loops. While these different contributions separately depend on the subtraction scale , and are -independent. The same holds for and , for which one obtains a similar decomposition:

The tree level contributions read:

 

with

whereas

 

Notice that varies from 1 (the standard case) up to = 4 for r = , . In the above expressions, and represent contributions from , and . Their scale dependences are compensated by the -dependences of the loop contributions, which read:

 

and

 

with denoting the combination

of pseudoscalar masses, and , . In the standard case, and are relegated to higher orders, while the quark mass ratio takes the value , with [3]

To the order we consider here, the standard expressions for and are

while the splitting of the decay constants is expressed as [3]

with

(, and are -independent). The expressions (6) for and for remain unchanged, while one finds that and become

  

These formulae could also be obtained directly from the standard expansion of the SU(3)SU(3) effective lagrangian. The above exercise is a rather non trivial illustration of how the standard case arises as a special case of the generalized PT. Notice also that restricting further the formulae (6), (19) and (20) to the SU(2)SU(2) chiral limit reproduces the scattering amplitude of Ref. [3].

Let us now come back to the expressions of Eqs. (8) and (11) for and Eqs. (10), (12) for . Apart from the observable pseudoscalar masses and decay constants, they involve various other quantities which we discuss in turn:

i) As already mentioned earlier, and collect tree level contributions from , and . The various low energy constants involved in these pieces of the effective lagrangian, and which would appear only starting from order in the standard case, are not under quantitative control at present. As an estimate of the uncertainties in and in coming from our lack of knowledge of and of , we shall take the changes in and in as the subtraction scale is varied between = 547.5 MeV and = 770 MeV.

ii) The two parameters () and are also not known. Their values are expected to remain small as compared to unity, due to the Zweig rule. At leading order, the same vacuum stability argument that requires demands that remains bounded as varies between and ,

In what follows, we shall assume that these bounds still provide, at order , a good estimate of the uncertainty on , which we further restrict not to become larger than 0.5, i.e.,

 

As for the remaining Zweig rule violating quantity , we allow it to vary between --0.2 and +0.2,

 

Notice that appears in the expression for the cross section already at order one loop in GPT [4], and also contributes to the form factors, especially to F. Its value may in principle be obtained from very accurate data, together with , and . Before discussing the values of these latter low energy constants, let us consider the ranges of values accessible to and according to the preceeding discussiongif . We show on Fig. 1 the bands of allowed values as functions of the quark mass ratio r. The bands delimited by the dotted curves correspond to the variations of and of in the ranges (22) and (23), respectively, and to the estimates, via the -dependences of and of , of the values and of the uncertainties associated to and to , respectively. The solid curves show the range of variation of and of when only these last uncertainties are taken into account, with and both taken to vanish. In the standard case, with the values of , , and as given in Ref. [3], we obtain, from Eqs. (19) and (20)

in agreement with the values read from Fig. 1 for 25.

iii) The low energy constants , i=1, 2, 3, can be extracted from the data on decays [5,6]. The expressions of the corresponding axial and vector current matrix elements are known at the one loop level both in the standard case [5,7] and in generalized PT [8]. In the latter case, the form factors depend on r in addition. This dependence on the quark mass ratio may affect the values of the 's one extracts from the data. In the standard case, the most recent analysis [7] of the data of Rosselet et al. [9] leads to the following values,

 

which give

 

A preliminary study of the generalized case shows that these values of , and tend to decrease in absolute value with r [8]. The constant is the most sensitive to variations in the quark mass ratio r and its central value becomes , for , with an uncertainty comparable to the one shown in Eq. (25). The variations in the values of and of , however, are smaller and affected by larger error bars. Within these, they remain compatible with the standard values (25). For and for , as before, remains unchanged, but decreases (in absolute value) by 30% and its central value becomes .

In Figs. 2 to 4 we have plotted the behaviours of the scattering lengths and , and of the slope parameter (all in units of ) as the quark mass ratio varies between 8 and 30. The two error bands (solid lines and dotted lines) come from the corresponding errors on and on shown in Fig. 1. The plots correspond to the central values of the 's, i=1,2,3, as given by Eq. (25) above. In Fig. 5 we show the difference , which can be obtained directly from the lifetime measurement of atoms, an experiment planed at CERN [10].

The phase shift combination can be extracted down to very small energies by analyzing decay data. In order to calculate the phase shifts, one first constructs the amplitude for a given partial wave l and isospin I from (see e.g. the appendix of Ref [1]). At order the phase shifts are given as usual by

 

This expression for should only be used close to the threshold, since the perturbative amplitude violates unitarity for energies above 430-440 MeV. The predictions of the GPT for is shown in Fig. 6, for r=10, and compared to the data of Rosselet et al. [9]. The predictions of the standard PT are also plotted. In the latter case, we use the values (25) of the low energy constants , and take for and the central values in Eq. (24), whereas the leading order values of and are both equal to 1. At present, both results are compatible with the data, but it is clear that a reduction of the experimental error bars by a factor of two could be enough to make the distinction between the alternatives and . Notice also that the uncertainties materialized by the dotted lines in Fig. 6 include the variations of the values of between and . The solid lines, which represent the variations induced by changing the subtraction scale in and in between and , correspond to . For , the solid lines would lie at the center of the dotted band.

Finally, we have gathered, in Table 1, the central values of the threshold parameters of Eqs. (4) and (5), for r=10. The value r=10 taken in the table below and in Fig. 6 showing the phase shifts, is suggested both by the analysis of the deviation from the Goldberger-Treiman relation [11], and by a recent analysis of the process in GPT [4]. The main differences between the standard predictions and the generalized case for r=10 arise in (30%), in (50%) and in (for the lowest value of ).

In all the figures presented here, the error bands delimited by the dotted lines are in principle reducible, if our knowledge of the two Zweig rule violating parameters and were to improve. A simultaneous determination of r and of is in principle possible from very accurate data on both and scattering. As for the value of , it might be obtained from more precise data on decays and on . The smaller error bands, delimited by the solid curves, reflect our lack of information concerning the low energy constants of , and , and a significant improvement seems unlikely so far. Living with only these last uncertainties still offers a good possibility to desentangle the low and large alternatives, provided the experimental data become accurate enough. On the theoretical side, it is in principle possible to study the effect of higher orders on the values of the parameters , and , i=1, 2, by comparing a fit to the data obtained from the parametrization of the amplitude given in Eq. [1], with a similar fit done by using the general parametrization of up to and including the order two loop given in Ref. [1].

true cm Table 1: Results for the threshold parameters for r=10 and for two values of , as compared to the standard predictions. The values shown correspond to the central values , , (for ) or (for ), and .

 
Figure 1: The bands of allowed values of (a) and of (b) as functions of the quark mass ratio . The dotted curves correspond to variations of and of in the ranges set by Eqs. (22) and (23), respectively, and with and estimated by the respective variations of and of for between 547.5 MeV and 770 MeV. The solid curves show the allowed values of and of when only the latter uncertainties are taken into account, having put and to zero.

 
Figure 2: The I=0 S-wave scattering lenth as varies between 8 and 30. The band delimited by the solid lines and the band delimited by the dotted lines arise from the corresponding uncertainties in and in shown in Fig. 1.

 
Figure 3: The I=0 S-wave slope parameter as varies between 8 and 30. The band delimited by the solid lines and the band delimited by the dotted lines arise from the corresponding uncertainties in and in shown in Fig. 1.

 
Figure 4: The I=1 P-wave scattering lenth 10 as varies between 8 and 30. The band delimited by the solid lines and the band delimited by the dotted lines arise from the corresponding uncertainties in and in shown in Fig. 1.

 
Figure 5: The difference of S-wave scattering lengths as a function of .

 
Figure 6: Plot of the phase shifts as a function of energy. The dashed line corresponds to the predictions of the standard case. The solid and dotted lines give the allowed values for r=10 in the generalized case (see text). The data points are from Rosselet et al. [8].





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Carlos E.Piedrafita