Short-range repulsion and isospin dependence in the kaon-nucleon
„KN… system
D. Hadjimichef,1J. Haidenbauer,2 and G. Krein31Departamento de Fı´sica, Universidade Federal de Pelotas, 96010-900 Pelotas, RS, Brazil 2Forschungszentrum Ju¨lich, Institut fu¨r Kernphysik, D-52425 Ju¨lich, Germany
3Instituto de Fı´sica Teo´rica, Universidade Estadual Paulista Rua Pamplona, 145-01405-900 Sa˜o Paulo, Sa˜o Paulo, Brazil 共Received 9 September 2002; published 27 November 2002兲
The short-range properties of the kaon-nucleon (KN) interaction are studied within the meson-exchange model of the Ju¨lich group. Specifically, dynamical explanations for the phenomenological short-range repul-sion, required in this model for achieving agreement with the empirical KN data, are explored. Evidence is found that contributions from the exchange of a heavy scalar-isovector meson 关a0(980)兴 as well as from genuine quark-gluon exchange processes are needed. Taking both mechanisms into account, a satisfactory description of the KN phase shifts can be obtained without resorting to phenomenological pieces.
DOI: 10.1103/PhysRevC.66.055214 PACS number共s兲: 13.75.Jz, 12.39.⫺x, 14.20.Jn, 21.30.⫺x
I. INTRODUCTION
The kaon-nucleon (KN) system provides an ideal setting for studying short-distance effects of the hadron-hadron force. This is because pions play a much less important role in the KN system than in the most extensively studied nucleon-nucleon (NN) system. Indeed, the one-pion ex-change is absent in the KN interaction and the contributions from 2 exchange to the interaction seem to be weaker than in the NN system. Under such circumstances one expects that short-distance effects can be most easily isolated from the attractive medium-range background and that possibly effects from explicit quark-gluon degrees of freedom can be identified.
A large body of work accumulated in the last 50 years indicates that meson degrees of freedom are very efficient for describing low-energy hadron-hadron interactions. In par-ticular, for the KN system, a few years ago the Ju¨lich group presented a meson-exchange model for the K⫹N scattering
关1,2兴. Reference 关1兴 considered single boson exchanges 共,,兲, together with contributions from higher-order dia-grams involving N, ⌬, K, and K* intermediate states. It turned out that the S-wave observables of KN experiments could only be described with the model if the value of the
KK coupling constant is increased about 60% above the value that follows from the SU共3兲 共quark flavor兲 symmetry. Specifically, the increased value of the KK coupling con-stant was strictly necessary to obtain the S-wave low-energy parameters and the energy dependence of S-wave phase shifts for both isospin I⫽0 and I⫽1 channels. However, this increased value leads to additional repulsion in the P and higher partial waves which seemed to be not favored by the empirical data, especially in the P03and P13channels.1Thus, it was concluded in Ref.关1兴 that the required additional con-tributions must be much shorter ranged than theexchange. Further evidence for the conjecture that the repulsion needed to describe KN scattering cannot be interpreted
com-pletely in terms of conventional exchange came from sub-sequent investigations of the K¯ N system 关3兴. In a meson-exchange model like the one developed by the Ju¨lich group there is a close connection between the KN and K¯ N interac-tions due to G-parity conservation. Specifically, this means that the repulsive exchange changes sign for K⫺N,
be-cause of the negative G parity of the meson, and becomes attractive. A large contribution from the exchange as fa-vored by the KN S waves turns then into a strongly attractive piece—which is indeed much too strong to fit the K⫺N
data关3兴.
The conclusion from those results was that exchange, as treated in this model, can only be interpreted as an effec-tive contribution that parametrizes besides the ‘‘physical’’ exchange also further shorter-ranged mesonic contributions or genuine quark-gluon effects or both. This was shown by a model analysis where the coupling constants of the meson (gKK, gNN) were kept at their SU共3兲 symmetry values and
an additional phenomenological共extremely short-ranged兲 re-pulsive contribution, a ‘‘re p,’’ with a mass of about 1.2
GeV was added—see Figs. 1共a兲 and 1共b兲.
In Ref. 关2兴 the model was further refined by replacing and exchange by the correlated 2-exchange contribution in the JP⫽0⫹ and JP⫽1⫺ channels, respectively, as illus-trated in Fig. 1共c兲. This was done by starting from a micro-scopic model for the t-channel reaction NN¯→KK¯ with
共and KK¯) intermediate states and using a dispersion relation
over the unitarity cut. Such a realistic model of共effective兲 and exchange was then used to reconstruct an extended meson-exchange model for KN scattering. But again, as in Ref.关1兴, the addition of a phenomenologicalre pwas
essen-tial to describe the data with the SU共3兲 KK coupling con-stant.
One possible interpretation for the need of a very short ranged repulsion, shorter ranged than that provided by exchange, is that quark-gluon effects are playing a role关1兴. The study of the KN interaction in the context of quark mod-els has a long history since the 1980s关4兴. More recently, the subject has gained renewed interest with the works of Barnes and Swanson关5兴 and Silvestre-Brac and collaborators 关6–8兴. The main ingredients in the calculations of both groups are 1The spectroscopic notation used is such that a partial wave with
angular momentum L, total angular momentum J, and isospin I is denoted by LI 2J.
the nonrelativistic quark model and a quark interchange mechanism with one-gluon exchange共OGE兲. One important conclusion of these calculations is that the derived KN inter-action is short ranged and repulsive, and strongly isospin dependent. As we discussed above, although in the Ju¨lich model the overall strength and energy dependence of the S wave phase shift of K⫹N scattering can be obtained by
aug-menting the value of the KK coupling, the P and higher partial waves do not come out right and the introduction of the exchange of a fictitious scalar particle with repulsive character was essential for this matter. In view of this, the substitution of an isospin independent re p by a strongly
isospin-dependent quark-gluon dynamics is not trivial and apparently bound to fail. However, we note that in both Refs.
关1,2兴 the a0(980) meson was left out without any apparent reason. This meson, being a scalar isovector, is an important source of isospin dependence and it has a mass not much larger than those of the other mesons considered in the model. Thus, it can, in principle, play an important role in the isospin dependence of the KN interaction.
The main motivation of our paper is to investigate the energy and isospin dependences of the KN interaction in a hybrid model, in which the Ju¨lich model is extended by
add-ing the a0(980) exchange, and where the very short ranged part of the KN interaction is described by quark-gluon ex-change, instead of the phenomenologicalre p. We construct
an effective KN potential from a microscopic nonrelativistic quark model from the interquark exchange mechanism and use all components of the OGE interaction. These include the Coulomb, spin-independent contact, and spin-orbit interac-tions. In addition, we use a linearly rising potential to repre-sent quark confinement.
The paper is organized as follows. In the following sec-tion we describe the KN meson-exchange model of the Ju¨-lich group. In Sec. III we provide an overview of studies on the KN system that were carried out in the framework of the quark model. In Sec. IV we present and discuss our results. Specifically, we investigate the consequences of replacing the phenomenological re p of the Ju¨lich model by
quark-gluon exchange. Our conclusions and perspectives are pre-sented in Sec. V. The Appendix presents the expressions for the effective KN potentials in the quark model.
II. THE JU¨ LICH KN MODEL
The Ju¨lich meson-exchange model of the KN interaction has been widely described in the literature关1,2,9,10兴 and we refer the reader to those works for details. Here we will only summarize the features that are relevant to the present study. The Ju¨lich meson-exchange model of the KN interaction was constructed along the lines of the共full兲 Bonn NN model
关11兴 and its extension to the hyperon-nucleon (YN) system 关12兴. Specifically, this means that one has used the same
scheme共time-ordered perturbation theory兲, the same type of processes, and vertex parameters共coupling constants, cutoff masses of the vertex form factors兲 fixed already by the study of these other reactions.
The diagrams considered for the KN interaction are shown in Fig. 1. Based on these diagrams a KN potential V is derived, and the corresponding reaction amplitude T is then obtained by solving a Lippmann-Schwinger type equation defined by the time-ordered perturbation theory,
T⫽V⫹VG0T. 共1兲
From this amplitude, phase shifts and observables共cross sec-tions, polarizations兲 can be obtained in the usual way.
As seen in Fig. 1, obviously the Ju¨lich model contains not only single-meson共and baryon兲 exchanges, but also higher-order box diagrams involving NK*, ⌬K, and ⌬K* interme-diate states. Most vertex parameters involving the nucleon and the ⌬共1232兲 isobar can be taken over from the 共full兲 Bonn NN potential. The coupling constants at vertices in-volving strange baryons are fixed from the Y N model共model B of Ref. 关12兴兲. Those quantities (gN⌳K, gN⌺K, gNY*K)
have been related to the empirical NN coupling by the assumption of SU共6兲 symmetry, cf. Refs. 关1,2兴.
For the vertices involving mesons only, most coupling constants have been fixed by SU共3兲 relating them to the em-pirical →2 decay. Exceptions are the coupling constants
gKK and gKK, which have been adjusted to the KN data
for the following reason: Themeson共with a mass of about
FIG. 1. Meson-exchange contributions to KN scattering in the Ju¨lich model关1,2兴. Diagrams 共a兲 and 共b兲 define the model of Ref.
关1兴 and diagram 共c兲 is the correlated 2 exchange calculated in Ref. 关2兴, which was parametrized by diagram 共a兲 in Ref. 关1兴.
600 MeV兲 is not considered as a genuine particle but as a simple parametrization of correlated 2-exchange processes in the scalar-isoscalar channel. Therefore, its coupling strength cannot be taken from symmetry relations. Concern-ing the exchange it was found that a much larger strength than obtained from SU共3兲 was required in order to obtain sufficient short-range repulsion for a reasonable description of the S-wave KN phase shifts关1兴. The coupling gKKhad
to be increased by about 60% over the symmetry value— quite analogous to the situation in the NN system关11兴. How-ever, such an increased exchange turned out to be in con-tradiction with the empirical data on P- and higher partial waves. Specifically, P03 and P13do not really demand addi-tional repulsive contributions. Thus, it was concluded that the additional repulsion should be of rather short-ranged na-ture. Such a contribution would still allow to obtain a rea-sonable description of the S waves, but would leave P and higher partial waves basically unchanged.
As a consequence, the Ju¨lich group presented a model where the coupling strengths for both gNN and gKK were
kept at their SU共6兲 values. At the same time, a phenomeno-logical, very short ranged contribution was added. This phe-nomenological piece has the same analytical form as ex-change, but an exchange mass of 1200 MeV and, most importantly, an opposite sign. Accordingly, it was denoted re p.
In a subsequent investigation the(600) and also the el-ementary were replaced by a microscopic model for cor-related 2 共and KK¯) exchange between a kaon and a nucleon, in the corresponding scalar-isoscalar and vector-isovector channels 关2兴. The starting point for this was a model for the reaction NN¯→KK¯ with intermediate 2 and
KK¯ states, based on a transition in terms of baryon (N,⌬,⌳,⌺) exchange and a realistic coupled channel
→, →KK¯, and KK¯→KK¯ amplitude. The contribu-tion in the s channel is then obtained by performing a dis-persion relation over the unitarity cut. But also in this model the phenomenological short-rangedre pwas needed in order
to achieve agreement with the empirical phase shifts. Since the results of Ref.关2兴 indicate that the contributions of the correlated 2exchange in the scalar-isoscalar channel are in rough agreement with the effective description by -exchange used in Ref.关1兴, we will employ the latter in the present investigation for simplicity reasons. Specifically, we will use the KN model I presented in Ref. 关2兴. The param-eters of this model are summarized in Table I. Resulting phase shifts for the Ju¨lich model I 关2兴 will be shown and compared with empirical data in Sec. IV. Further results, including scattering observables, can be found in Ref.关2兴.
III. THE KN INTERACTION IN THE QUARK MODEL In this section we briefly review the salient features of model calculations of the KN interaction that are based on quark-gluon exchange and derived within the nonrelativistic quark model. Specifically, we will focus on the more recent calculations of Barnes and Swanson 关5兴 and Silvestre-Brac and collaborators关6–8兴.
Barnes and Swanson use the quark-Born-diagram共QBD兲 method关13兴. In this method, the KN scattering amplitude is assumed to be the coherent sum of all OGE interactions fol-lowed by all alfol-lowed quark line exchanges. The input to this method is the microscopic quark-quark interaction and kaon and nucleon wave functions. Barnes and Swanson 关5兴 used the contact spin-spin ‘‘color-hyperfine’’ component of the OGE and used Gaussian wave functions for the interacting hadrons, which allowed them to evaluate the KN scattering amplitude analytically. They calculated isospin I⫽0 and I
⫽1 scattering observables such as S-wave phase shifts and
scattering lengths. The model has only two parameters, the ratio of the u,d to s quark masses,⫽mq/ms, and ␣s/mq
2 , where ␣s is the quark-gluon coupling constant. By using
typical quark-model parameters and using the Born approxi-mation, Barnes and Swanson obtained very reasonable re-sults for the S-wave phase shifts关5兴.
The studies of Silvestre-Brack and collaborators 关6–8兴 complement the work of Barnes and Swanson in several as-pects. First of all, Refs.关6–8兴 employ the resonating group method 共RGM兲 instead of the QBD method. The main dif-ference between the two methods refers to the way orthogo-nality effects in the relative KN wave functions are treated. These are effects due to the Pauli principle for quarks in different clusters. It can be shown 关14兴 that the differences between effective hadron-hadron interactions calculated with both methods are usually small, although not entirely negli-gible. In Ref. 关6兴 the authors calculate S-wave scattering phase shifts using the Coulomb, spin-spin, and constant con-tact pieces of the OGE quark-quark interaction. In addition, they include the exchange of and mesons—considered TABLE I. Vertex parameters used in the Ju¨lich KN model I关2兴. Numbers in parentheses denote corresponding values of the model discussed in the present paper, when different.
Process Exchanged particle Mror mra 共MeV兲 g1g2/4b 关 f1/g1兴 ⌳1c 共GeV兲 ⌳2 c 共GeV兲 KN→KN 600 1.300 1.7 1.5 共1.000兲 共1.2兲 re p 1200 – 40 1.5 1.5 (•) (•) (•) a0 980 - - -共2.600兲 共1.5兲 共1.5兲 782.6 2.318关0 1.5 1.5 769 0.773关6.1兴 1.4 1.6 ⌳ 1116 0.905 4.1 4.1 ⌺ 1193 0.031 4.1 4.1 Y* 1385 0.037 1.8 1.8 KN→K*N 138.03 3.197 1.3 0.8 769 0.773关6.1兴 1.4 1.0 KN→K*⌬ 138.03 0.506 1.2 0.8 769 4.839 1.3 1.0 KN→K⌬ 769 4.839 1.3 1.6
aMass of exchanged particle.
bProduct of coupling constants共ratio of tensor to vector coupling兲. cCutoff mass.
as elementary particles—between quarks, and a linearly ris-ing confinris-ing potential. The same quark-quark interaction is used to build the K and N wave functions and to generate the
KN interaction. The parameters are constrained to reproduce
the low-lying meson and baryon spectrum. The main conclu-sion of this study was that it is impossible to describe both
I⫽0 and I⫽1 isospin channels simultaneously within the
model. Relativistic kinetic energy effects were investigated in Ref. 关7兴. The results obtained for the S waves, for which one expects such effects to be more important, were not much different from the corresponding nonrelativistic ones. In Ref. 关8兴, scattering phase shifts from S up to G waves were calculated. The difference from Ref.关6兴 is that a spin-orbit interaction was added to the OGE and confining pieces used there. No meson exchanges between quarks were con-sidered. The parameters were again fixed by requiring a good description of the low-lying meson and baryon spectrum. The results obtained are such that the I⫽0 S-wave phase shift is reasonably well described, while the corresponding
I⫽1 is too repulsive. The P and higher partial-wave phase
shifts are poorly described, with the exception of the P11,
D13, D15, and G19 phases. The P01 phase, for example, is predicted to be almost zero, while the corresponding experi-mental phase grows from zero up to 60° at plab⫽1 GeV.
The results of Silvestre-Brac and collaborators 关6–8兴 clearly indicate that the quark-interchange mechanism with OGE alone is not sufficient to describe the K⫹N data.
How-ever, it seems to provide at least enough strength for S waves. In view of the discussion above on the Ju¨lich model, we investigate here the substitution ofre pin that model by
the quark-interchange mechanism with OGE. Recently, one of us 关15兴 has derived the contribution of the spin-spin part of the OGE to the central part of the KN interaction using the mapping formalism developed in Ref. 关14兴. The different contributions to the K⫹N effective potential from the
quark-interchange mechanism are illustrated in Fig. 2. The on-shell
KN amplitude is identical to the one derived by Barnes and
Swanson关5兴. In order to iterate the potential in a Lippmann-Schwinger equation one needs the off-shell amplitude. For this purpose, we have calculated the contributions of all re-maining components of the OGE to the K⫹N effective
po-tential within the framework of Ref.关14兴. We found that the spin-spin component of the OGE gives by far the most im-portant contribution to the K⫹N effective potential.
For illustrative purposes we present, in this section, the phases calculated in Born approximation—in the following section the OGE KN potential is iterated in the Lippmann-Schwinger type of equation, Eq.共1兲. In Fig. 3 we present the
S- and P-wave phase shifts resulting from the OGE and the
confining interaction. The higher partial waves are very small and are not shown. The experimental data points in this figure are taken from Refs.关16–18兴. The analytical expres-sions for the KN potential are given in the Appendix. The parameters of the potential are the masses of the constituent quarks, mq(⫽mu⫽md) and ms, the quark-gluon hyperfine
coupling ␣s, and the size parameters of the nucleon and
kaon wave functions, ␣ and. We use the ‘‘reference pa-rameter set’’ of Barnes and Swanson关5兴, which contains con-ventional quark model parameters. These are
⫽mq/ms⫽0.33 GeV/0.55 GeV⫽0.6,
␣s/mq
2
⫽0.6/共0.33兲2 GeV2,
␣⫽0.4 GeV, ⫽0.35 GeV. 共2兲
The string tension of the confining potential is taken to be ⫽0.18 GeV2 关19兴. In addition, when calculating the phase shifts we use the physical masses of the nucleon and the kaon, MN⫽0.940 GeV and MK⫽0.495 GeV. Figure 3
shows that S waves are reasonably well described by the model, although the I⫽0 phase agrees less well with the data at higher energies. The fit can be improved slightly by choos-ing another set of parameters, as done by Barnes and
Swan-FIG. 2. The four quark-interchange kaon-nucleon scattering dia-grams.
FIG. 3. KN phase shifts. The solid lines are the result from the full quark-model calcuation described in the text. Experimental phase shifts are taken from Refs. 关16兴 共open circles兲, 关17兴 共open squares兲, and 关18兴 共filled circles and pluses兲.
son in their study of the S-wave phase shifts关5兴. In this paper we maintain the reference set, since the general trend of the higher partial waves will not be modified by a change of the quark model parameters.
In Fig. 4 we show the separate contributions of the OGE and confining interaction to S and P phases. The dominance of the spin-spin component of OGE is clearly seen. The con-fining interaction gives a very small contribution to all waves, and the only noticeable effect from the other compo-nents of the OGE is the one from the Coulomb part in the S11 wave.
IV. RESULTS AND DISCUSSION
As discussed in the last two sections, the KN interaction in the low-energy region ( plab⭐1 GeV/c) can be well
un-derstood within the meson-exchange picture. However, a good quantitative overall description of the data can only be achieved by adding a phenomenological contribution that is extremely short ranged and repulsive—and therefore affects essentially the S waves only. At the same time, interaction models based on quark-gluon degrees of freedom yield only a mediocre overall reproduction of the KN phase shifts. However, the predicted S waves are in fairly good agreement with empirical results, suggesting that at least the short-ranged part of the KN interaction is well accounted for by the one-gluon-exchange mechanism that is the dominant in-gredient in those quark models. It is, therefore, tempting to combine the contributions of those two complementary ap-proaches to the KN force. Indeed, such a procedure is in the spirit of the original KN model of the Ju¨lich group where it was suggested that the short-ranged phenomenological piece added in this model might be an effective parametrization of either further short-ranged mesonic contributions or of genu-ine quark-gluon effects or both关1,20兴.
Results for the KN phase shifts of the original Ju¨lich model共note that we use here model I of Ref. 关2兴兲 are shown
by the dash-dotted lines in Fig. 5. If we switch off the con-tribution from the phenomenological re p and add the
con-tribution from one-gluon exchange instead we obtain the short-dashed lines. The parameters of the quark model are the same as in the preceding section. We see that the OGE is indeed capable of producing repulsive contributions which are of a comparable order of magnitude as the one of the phenomenologicalre p. Indeed, after the discussion in Sec. III this could have been expected. However, it is definitely surprising that for the S11partial wave the results with OGE
共and without re p) are almost identical to the ones of the
original Ju¨lich model. In case of the S01, the situation is somewhat less satisfying. Here the repulsion provided by the OGE is significantly smaller than the one parametrized by there p. This is simply a consequence of the isospin
depen-dence inherent in the OGE—the phenomenological re p is,
of course, per construction an isoscalar. The higher partial waves 共in the I⫽0 as well as the I⫽1) are again only mar-ginally changed as compared to the original results— testifying that also the OGE is of rather short range.
The above results can be seen as an indication that the OGE is not the only short-range physics that is parametrized by the re p of the Ju¨lich KN model. 共Indeed, one might
argue that this could have been already guessed from the difference in the isospin structure.兲 Besides possible higher-order contributions resulting from quark-gluon dynamics, one should not forget to take into consideration further shorter-ranged mesonic contributions. Indeed, the exchange of the a0(980) meson, which is a scalar-isovector particle, is a natural candidate for this. With its mass of about 1 GeV its contributions are definitely of short-ranged nature as re-quired. Furthermore, its isospin structure leads to attractive contributions in the I⫽1 channel but to repulsive contribu-tions in the I⫽0 channel. Thus, it complements the isospin dependence of the OGE in an almost ideal way and in con-junction with the latter would lead to contributions that are almost isospin independent—as those of the phenomenologi-cal re p. The a0(980) meson is taken into account in the Bonn NN model关11兴 共it is denoted as␦ meson there兲. How-ever, for unexplained reasons, it was not included in the original Ju¨lich KN model. Subsequent investigations of the Ju¨lich group on the structure of the a0(980) meson sug-gested that this resonance can be understood in terms of strong correlations in the -KK¯ channel 关21兴. Thus, the situation is similar to the strong -KK¯ correlations in the scalar-isoscalar channel that are usually effectively param-etrized by the meson. Accordingly, it is in the spirit of the Bonn/Ju¨lich models of hadronic reactions to consider the contributions of the a0(980) meson, and indeed it is included in the more recently developed models of the N 关22,23兴
and Y N 关24兴 interactions. Following the arguments in Refs.
关21,22兴 we do not view the a0 exchange as a genuine meson exchange but rather as a parametrization of correlations in the mesonic systems in the scalar-isovector channel. There-fore we consider the a0 coupling constants as free param-eters. In principle, gKK¯ a0 could be determined from the a0 decay width into the KK¯ system. However, the experimental information on this quantity is still very poor, cf. Ref. 关25兴,
FIG. 4. KN phase shifts resulting from various contributions of
the quark model, cf. Appendix: Coulomb 共dash-dotted line兲; spin
orbit 共pluses兲; confinement 共short-dashed line兲; contact spin-spin
and thus cannot provide more than a guideline. Note that in the a0 exchange the product of the NNa0 and KK¯ a0 cou-pling constants appears, and therefore we list only this prod-uct in Table I.
Results including now a0 meson exchange as well as the OGE contributions are shown by the long-dashed lines in Fig. 5. The coupling strength of the a0 exchange has been chosen in such a way that the model prediction for the S01 partial wave agrees roughly with the result of the original Ju¨lich KN model. As can be seen in Fig. 5, the inclusion of the a0 exchange influences also the KN P waves in the I
⫽0 channel, i.e., the P01 and P03, whereas all other higher partial waves remain basically unchanged. As a matter of fact, the present model based on a0 meson exchange and OGE contributions yields pretty much the same results as the original Ju¨lich model utilizing the phenomenological re p.
Minor differences occur only in the S11partial wave, which turns out to be now somewhat too less repulsive in compari-son to the data. Thus, as a last step, we have slightly read-justed the parameters of the meson, cf. Table I, which then leads to the final results shown by the solid lines in Fig. 5. Those results provide clear evidence that a comparable
quan-titative description of the KN interaction can be achieved with a model that avoids phenomenological contributions like there pof the original Ju¨lich model.
Finally, we want to address the question whether a de-scription of the KN interaction is possible within the Ju¨lich model without introducing explicit contributions from the OGE. Treating the coupling constants of the and a0 me-sons as completely free parameters we were indeed able to obtain a reasonable reproduction of the S01 and S11 partial waves. However, it could only be achieved by assuming that the-exchange contribution is basically zero. Of course, this is completely unrealistic in view of the results obtained for the strength of the correlated two-pion exchange in the channel in Ref. 关2兴. Moreover, the description of the higher partial waves deteriorates significantly if the -exchange contribution is so strongly reduced.
V. CONCLUSIONS AND PERSPECTIVES
In this paper we have studied the short-range properties of the KN interaction. In particular, we have taken the KN meson-exchange model of the Ju¨lich group and we explored
FIG. 5. KN phase shifts. The dash-dotted lines are the phase shifts of the original Ju¨lich model I from Ref.关2兴. The short-dashed line shows results where the phenomenologicalre pin the Ju¨lich model is replaced by the quark-model contribution. Adding the a0-exchange
contribution yields the long-dashed line. The solid line is obtained after refitting the parameters of the. Same description of experimental phase shifts as in Fig. 3.
possible dynamical explanations for a phenomenological
共extremely short-ranged兲 repulsive contribution, a ‘‘re p’’
with a mass of about 1.2 GeV, that is present in the Ju¨lich model. Such a phenomenological, repulsive, and rather short-ranged piece had to be introduced in that model for achieving agreement with the empirical KN data.
The very short-ranged nature of this repulsion could be a sign that quark-gluon dynamics is playing a role. Therefore, we have calculated corresponding contributions to the KN interaction based on the nonrelativistic quark model and a quark interchange mechanism with one-gluon exchange. It turned out that those processes are indeed short ranged and repulsive. However, unlike the phenomenological ‘‘re p’’ in
the Ju¨lich model, they are also strongly isospin dependent. Thus, one-gluon exchange alone can certainly not explain the required short-range physics. Consequently, we examined additional short-range physics that arises in the mesonic sec-tor, and specifically the exchange of the 共scalar-isovector兲
a0(980) meson. Its contribution was not included in the original Ju¨lich KN model.
Due to its isospin structure the a0(980) exchange pro-vides attraction in the I⫽1 channel and repulsion in the I
⫽0 channel, and therefore counterbalances the isospin
de-pendence of the one-gluon exchange. Taking both mecha-nisms (a0as well as one-gluon exchange兲 into account yields a short ranged and repulsive but basically isospin-independent interaction—similar to the one parametrized by there p—and, consequently, a satisfactory description of the KN phase shifts can be obtained without resorting to
phe-nomenological pieces, as demonstrated in the present paper. The authors of the original Ju¨lich KN model conjectured that the introduced phenomenological re p might be an
ef-fective parametrization of either further short-ranged me-sonic contributions or genuine quark-gluon effects or both
关1兴. Our investigation provides strong evidence that the third
alternative is realized. Specifically, it lends support to the supposition that effects from quark-gluon degrees of freedom can be explicitly seen in the KN system. Still one can raise the question whether contributions from genuine quark-gluon dynamics are really needed. For example, could their role be taken over by the exchange of heavier vector mesons, say? To answer this question it will be very instructive to study the K¯ N system again, using the present model. For example, the investigations in Ref. 关3兴 have shown that the
K¯ N data require only a strongly reduced short-ranged
repul-sive piece, i.e., only about 20% of the phenomenological re p used in the KN system. It will be interesting to see
whether the present scenario of combined a0(980) exchange and quark-gluon dynamics is able to generate these proper-ties when going over to the K¯ N system. One should note, however, that the treatment of the K¯ N channel in the nonrel-ativistic quark model is more complicated than the KN sys-tem since it involves s-channel gluon exchange. Special care must be taken with such processes because it is not clear that the use of perturbative massless gluons makes physical sense in this model. Contributions of intermediate hybrid qq¯ g states to the process must certainly be considered. Still the extension of the quark interchange model to incorporate
gluon annihilation in the K¯ N system would be a very inter-esting new development. Investigations along this line are planned for the future.
ACKNOWLEDGMENTS
The authors are thankful to Ted Barnes for illuminating discussions. Financial support for this work was provided in part by the international exchange program DLR共Germany, Grant No. BRA W0B 2F兲 and CNPq 共Brazil, Grant No. 910133/94-8兲.
APPENDIX: CONTRIBUTIONS TO THE KN INTERACTION FROM OGE AND CONFINEMENT In this appendix we present the different contributions the OGE and from the confining potential to the KN potential used in the present paper. Let us denote the initial and final three momenta of the interacting quarks by kជ1, kជ2, kជ1
⬘
, andkជ2
⬘
共prime means final state兲. It is convenient to define thefollowing combinations of momenta: qជ⫽kជ1
⬘
⫺kជ1⫽kជ2⫺kជ2⬘
,p1⫽(kជ1⫹kជ1
⬘
)/2 and p2⫽(kជ2⫹kជ2⬘
)/2. In terms of these, the interquark interaction can be written asHOGE⫽
兺
i j冋
兺
a Fa共i兲Fa共 j兲
册
Vi j共qជ, pជi, pជj兲, 共A1兲
where i, j identify the quarks 共or antiquarks兲 1,2 and
Vi j(qជ, pជi, pជj) depends on spin variables and the indicated
momenta. The color SU共3兲 matrices Fa(i), a⫽1, . . . ,8, are given in terms of the Gell-Mann matrices a as Fa(i)
⫽a/2 when i is a quark andFa(i)⫽⫺aT/2 when i is an
antiquark (T means transpose兲. We refer the reader to the literature for the explicit expression of Vi j(qជ, pជi, pជj)—see,
for example, Eq. 共3兲 of Ref. 关19兴.
Next, we present the individual contributions in
Vi j(qជ, pជi, pជj) to the KN potential. We represent each contri-bution to the KN potential as
V共pជ, pជ
⬘
兲⫽1 2 D兺
⫽ad
关VD共pជ, pជ
⬘
兲⫹VD共pជ⬘
, pជ兲兴, 共A2兲where pជ and pជ
⬘
are the initial and final center of mass mo-menta of the the KN system, and the index D identifies the diagrams a, . . . ,d of Fig. 2. The explicit evaluation of these diagrams requires also the specification of the nucleon and kaon wave functions,⌿Nand⌿K. These are taken to be inmomentum space of the form
⌿N共pជ兲⫽␦共pជ⫺kជ1⫺kជ2⫺kជ3兲 N共pជ兲共kជ1兲共kជ2兲共kជ3兲, 共A3兲 where 共kជ兲⫽
冉
1 ␣2冊
3/4 exp共⫺kជ2/2␣2兲,N共pជ兲⫽共3␣2兲3/4exp t共pជ2/6␣2兲, 共A4兲 and ⌿K共pជ兲⫽␦共pជ⫺kជq⫺kជq¯兲
冉
1 2冊
3/4 exp冋
⫺共m1kជq⫺m2kជ¯q兲 2 82册
, 共A5兲 with m1⫽ 2m¯q mq⫹mq¯ , m2⫽ 2mq mq⫹m¯q . 共A6兲For convenience, we also introduce the quantities
⫽mq/ms, g2⫽␣/, b⫽1/␣. 共A7兲
The explicit contributions of the different pieces of the OGE and of the confining potential to the effective KN interaction are given by the following expressions.
1. Coulomb VDCoul共pជ, pជ
⬘
兲⫽4␣sD共I兲冕
0 ⬁ dsD共s兲 ⫻exp关⫺AD共s兲 p2⫺BD共s兲,p⬘
2 ⫹CD共s兲pជ•pជ⬘
兴, 共A8兲where the variable s comes in because we have chosen to perform a Laplace transform of the Coulomb potential 1/q2 in order to integrate over the variable q, and the coefficients D(I) (I identifies isospin I⫽1 or I⫽0) come from
sum-ming over color-spin flavor of quarks. The functions
AD,BD,CD, and D for each diagram can be written as a
ratio AD⫽n(AD)/d(AD), . . . , D⫽n(D)/d(D). Diagram (a). n共Aa兲⫽24b42⫹9b2m12⫹共80b22⫹24b44 ⫺48b22m 1⫹6m1 2⫹18b22m 1 2兲s, n共Ba兲⫽n共Aa兲, n共Ca兲⫽8b42⫹3b2m1 2⫹共⫺16b22⫹8b44 ⫹16b22m 1⫹2m1 2兲s, n共a兲⫽3
冑
3b3/83, d共Aa兲⫽d共Ba兲⫽6d共Ca兲⫽482关3b2⫹共2⫹3b22兲s兴, d共a兲⫽关3b2⫹共2⫹3b22兲s兴3/2, a共1兲⫽⫺4/9, a共0兲⫽0. 共A9兲 Diagram (b). n共Ab兲⫽⫺24⫺80b22⫹24b44⫹12m1⫹60b22m1 ⫺9b22m 1 2 ⫺共962⫹176b24⫺48b46 ⫺482m 1⫺62m1 2⫹120b24m 1⫺18b24m1 2兲s, n共Bb兲⫽12⫹20b22⫺24b44⫺6 m1⫺18b22m1 ⫹共482⫹8b24⫺48b46⫺242m 1 ⫺12b24m 1⫺32m1 2⫺9b24m 1 2兲s, n共Cb兲⫽2b42⫹2b2共m1⫺1兲 ⫹共4b44⫺8b22⫹8b22m 1⫹m1 2兲s, d共Ab兲⫽2d共Bb兲⫽122d共Cb兲 ⫽242关1⫹3 b22⫹共42⫹6b24兲s兴, b共1兲⫽4/9, b共0兲⫽0. 共A10兲 Diagram (c). Ac共s兲⫽64b42⫹12b64⫺60b42m1⫹21b2m1 2 ⫹36b42m 1 2 ⫹共320b22⫹96b44 ⫺192b22m 1⫹24m1 2⫹72b22m 1 2兲s, Bc共s兲⫽256b42⫹12b64⫺132b42m1 ⫹21b2m 1 2⫹36b42m 1 2⫹共320b22⫹96b44 ⫺192b22m 1⫹24m1 2⫹72b22m 1 2兲s, Cc共s兲⫽⫺32b42⫹4b64⫹32b42m1⫹7b2m1 2 ⫹关32b44⫹64b22共m 1⫺1兲⫹8m1 2兴s, c共s兲⫽24冑
3b3/3, d共Ac兲⫽d共Ab兲⫽6d共Ac兲⫽482关7b2⫹6b42⫹共8⫹12b22兲s兴, d共c兲⫽关7b2⫹6b42⫹共8⫹12b22兲s兴3/2, c共1兲⫽4/9, c共0兲⫽0. 共A11兲 Diagram (d). n共Ad兲⫽80b2⫹160b42⫹12b64⫺72b2m1⫺132b42m1 ⫹21b2m 1 2⫹36b42m 1 2 ⫹共320b22⫹96b44 ⫺192b22m 1⫹24m1 2⫹72b22m 1 2兲s, n共Bd兲⫽n共Ad兲,
n共Cd兲⫽⫺16b2⫺32b42⫹4b64⫹8b2m1 ⫹20b42m 1⫹b2m1 2 ⫹共⫺64b22⫹32b44⫹64b22m 1⫹8m1 2兲s, n共d兲⫽⫺24
冑
3b33/3, d共Ad兲⫽d共Bd兲⫽6d共Cd兲 ⫽48共2⫹3b22兲共1⫹2b22⫹42s兲, d共d兲⫽关共2⫹3b22兲共1⫹2b22⫹42s兲兴3/2, d共1兲⫽⫺4/9, d共0兲⫽0. 共A12兲 2. Spin orbit VDSO共pជ, pជ⬘
兲⫽i共pជ⫻pជ⬘
兲•SជNwDSO共pជ, pជ⬘
兲, 共A13兲 with SNthe spin operator of the nucleon andwDSO共pជ, pជ
⬘
兲⫽4␣sD共I兲冕
0 ⬁ dsD共s兲 ⫻exp关⫺AD共s兲p2⫺BD共s兲p⬘
2⫹CD共s兲pជ•pជ⬘
兴, 共A14兲where the functions A,B,C are the same as in the Coulomb potential, and theD’s are given by
a共s兲⫽ 3
冑
3b5共8⫺3m1兲 323关3b2⫹共2⫹3b22兲s兴5/2, b共s兲⫽⫺ 3 83冑
3 2 b33共m1⫺2兲共4b22⫹m1兲 关1⫹3b22⫹共42⫹6b24兲s兴5/2, c共s兲⫽⫺ 3冑
3b5共m1⫺4⫺2b22兲 3关7b2⫹6b42⫹共8⫹12b22兲s兴5/2, d (1) 共s兲⫽⫺ 3冑
3b 44共1⫹2b22兲共2b22⫹m 1兲共28b44⫹m1 2⫹8b22⫹8b22m 1兲 23共2⫹3b22兲共1⫹4b22⫹3b44兲3/2共4⫹2b22⫺m1兲关1⫹22共b2⫹2s兲兴5/2 , d (2)共s兲⫽3冑
3 23 b33共2b22⫹m1兲共28b44⫹m1 2⫹8b22⫹8b22m 1兲 共2⫹3b22兲5/2共4b22⫹m 1兲关1⫹22共b2⫹2s兲兴5/2 , a共0兲⫽⫺ 4 3 1 m2, a共1兲⫽⫹ 8 9 1 m2, b共0兲⫽⫹ 2 9冉
1 ms 2⫺ 1 m2冊
, b共1兲⫽⫺ 4 27冉
1 ms 2⫺ 1 m2冊
, c共0兲⫽⫹ 1 3 1 m2, c共1兲⫽⫺ 1 9 1 m2, d (1)共0兲⫽⫺1 9冉
1 m2⫹ 4 mms冊
, d (1)共1兲⫽⫺ 1 27冉
1 m2⫹ 8 mms冊
, 共A15兲 d (2)共0兲⫽⫹2 9冉
1 ms2⫹ 1 mms冊
, d (2)共1兲⫽⫺ 2 27冉
2 ms2⫺ 1 mms冊
. 共A16兲 3. Contact spin-spinVDSS共pជ, pជ
⬘
兲⫽ssD共I兲Dexp关⫺ADp2⫺BDp⬘
2⫹CDpជ•pជ⬘
兴.共A17兲 Diagram (a). Aa⫽2共1⫹兲 2⫹3g 12␣2共1⫹兲2 , Ba⫽Aa, Ca⫽ 2共1⫹兲2⫹3g 6␣2共1⫹兲2 , a⫽1, a共1兲⫽1/3, a共0兲⫽0, a共1兲⫽1/3, a共0兲⫽0. Diagram (b). Ab⫽ 共5g⫹3兲2⫹共⫺2g⫹6兲⫹共2g⫹3兲 6␣2共g⫹3兲共1⫹兲2 , Bb⫽ 共5g⫹3兲2⫹共10g⫹6兲⫹共5g⫹3兲 6␣2共g⫹3兲共1⫹兲2 , Cb⫽ 共1⫺g兲2⫹2⫹共g⫹1兲 ␣2共g⫹3兲共1⫹兲2 , b⫽
冉
6 g⫹3冊
3/2 , b共1兲⫽1/3, b共0兲⫽0.Diagram (c). Ac⫽ 共16g⫹3兲2⫹共2g⫹6兲⫹共21g2⫹22g⫹3兲 12␣2共7g⫹6兲共1⫹兲2 , Bc⫽ 共64g⫹3兲2⫹共62g⫹6兲⫹共21g2⫹34g⫹3兲 12␣2共7g⫹6兲共1⫹兲2 , Cc⫽ 共1⫺8g兲2⫹2⫹共7g2⫹8g⫹1兲 2␣2共7g⫹6兲共1⫹兲2 , c⫽
冉
12g 7g⫹6冊
3/2 , c共1兲⫽1/18, c共0兲⫽1/6. Diagram (d). Ad⫽ 共20g2⫹40g⫹3兲2⫹共4g2⫹14g⫹6兲⫹共5g2⫹10g⫹3兲 12␣2共2g⫹3兲共g⫹2兲共1⫹兲2 , Bd⫽Ad, Cd⫽ 共1⫺4g2⫺8g兲2⫹共2⫺4g2⫺6g兲⫹共g2⫹2g⫹1兲 2␣2共2g⫹3兲共g⫹2兲共1⫹兲2 , d⫽冋
12g 共2g⫹3兲共g⫹2兲册
3/2 , d共1兲⫽1/18, d共0兲⫽1/6. 4. Contact spin-independent VDCon-SI共pជ, pជ⬘
兲⫽4␣sD共I兲exp关⫺ADp2⫺BDp⬘
2 ⫹CDpជ•pជ⬘
兴, 共A18兲where the functions AD, . . . are the same as for the
spin-spin interaction and
a共1兲⫽⫹ 1 9 1 m2, a共0兲⫽0, b共1兲⫽⫺ 1 18 1 m2共1⫹ 2兲, a共0兲⫽0, c共1兲⫽⫺ 1 9 1 m2, a共0兲⫽0, c共1兲⫽⫺ 1 18 1 m2共1⫹ 2兲, a共0兲⫽0. 共A19兲 5. Confinement
The confining interaction is taken to be a linearly rising potential, which in momentum space is given as
Vcon f⫽
6
q4 , 共A20兲
where is the string tension. Equation 共A20兲 includes a color factor of 3/4. The effective KN interaction is given by
VDConf共pជ, pជ
⬘
兲⫽6D共I兲冕
0 ⬁ du冕
u ⬁ dsD共s兲 ⫻exp关⫺AD共s兲p2⫺BD共s兲p⬘
2⫹CD共s兲pជ•pជ⬘
兴, 共A21兲where the functions AD(s),BD(s),CD(s), and D are the
same as for the Coulomb term, and theD(I)’s are given by
a共1兲⫽⫹4/9, a共0兲⫽0,
b共1兲⫽⫺4/9, b共0兲⫽0,
c共1兲⫽⫺4/9, a共0兲⫽0,
d共1兲⫽⫹4/9, d共0兲⫽0. 共A22兲
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