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QCD sum rule approach to the new mesons and the gDsJ DK coupling constant

Abstract

We use diquark-antidiquark currents to investigate the masses and partial decay widths of the recently observed mesons D+sJ(2317), D*0(0)(2308) and X(3872), considered as four-quark states, in a QCD sum rule approach. In particular we investigate the coupling constant gDsJ DK. We found that the gDsJ DK obtained in this four-quark scenario is smaller than the coupling constant obtained when D+sJ(2317) is considered as a conventional cs state.

QCD Sum Rule


HEAVY FLAVORS

QCD sum rule approach to the new mesons and the gDsJDK coupling constant

Marina Nielsen

Instituto de Física, Universidade de São Paulo, C.P. 66318, 05315-970 São Paulo-SP, Brazil

ABSTRACT

We use diquark-antidiquark currents to investigate the masses and partial decay widths of the recently observed mesons D+sJ(2317), D*00(2308) and X(3872), considered as four-quark states, in a QCD sum rule approach. In particular we investigate the coupling constant gDsJDK. We found that the gDsJDK obtained in this four-quark scenario is smaller than the coupling constant obtained when D+sJ(2317) is considered as a conventional cs state.

Keywords: QCD Sum Rule

I. INTRODUCTION

The constituent quark model provides a rather successful descrition of the spectrum of the mesons in terms of quark-antiquark bound states, which fit into the suitable multiplets reasonably well. Therefore, it is understandable that the recent observations of the very narrow resonances (2317) by BaBar [1], (2460) by CLEO [2], X(3872) by BELLE [3], and the very broad scalar meson (2308) by BELLE [4], all of them with masses below quark model predictions, have stimulated a renewed interest in the spectroscopy of open charm and charmonium states. The difficulties to identify the mesons (2317) and (2460) as states are rather similar to those appearing in the light scalar mesons below 1 GeV (the isoscalars s (500), f0(980), the isodublet k (800) and the isovector a0(980)), whose masses are also smaller than naive quark model predictions, and that can be interpreted as four-quark states [5, 6]. In the case of X(3872), besides its small mass, the observation, reported by the BELLE collaboration [7], that the X decays to J/ y p +p -p 0, with a strength that is compatible to that of the J/ y p +p - mode:

establishes strong isospin violating effects, which can not be explained if the X(3872) is interpreted as a state.

Due to these facts, these new mesons were considered as good candidates for four-quark states by many authors [8]. In refs. [9, 10] the method of QCD sum rules (QCDSR) [11-13] was used to study the two-point functions for the mesons (2317), (2308)and X(3872) considered as four-quark states in a diquark-antidiquark configuration. The results obtained for their masses are compatible with the experimental values and, therefore, in refs. [9, 10] the authors concluded that it is possible to reproduce the experimental value of the masses using a four-quark representation for these states.

Concerning their decay widths, the study of the three-point functions related to the decay widths (2317) ® p 0, ® D+p - and X(3872) ® J y p +p -, using the diquark-antidiquark configuration for DsJ, and , was done in refs. [14-16]. The results obtained for their partial decay widths are given in Table I, from where we see that the partial decay widths obtained in refs. [14-15], supposing that the mesons (2317) and are four-quark states, are consistent with the experimental upper limit for the total decay width.

However, in the case of the meson X(3872), the partial decay width obtained in ref. [16] is much bigger than the experimental upper limit to the total width.

In ref. [16] it was shown that it is possible to reduce the value of the estimated X(3872) decay width, by imposing that the initial four-quark state has a non-trivial color structure. In this case, some diagrams are eliminated and the partial decay width can be reduced to G (X ® J/ y p +p -)) = (0.7 ± 0.2) MeV. However, that procedure may appear somewhat unjustified and, therefore, more study is needed until one can arrive at a definitive conclusion about the structure of the meson X(3872).

Concerning the meson (2317), although its mass and decay width can be explained in a four-quark scenario, they can also be reproduced in other approaches [8], and it is not yet possible to discriminate between the different structures proposed for this state. Therefore, it is important to find experimental observations that could be used to descriminate between the different quark structure of these mesons. As pointed out in ref. [17], a signal could be obtained by the analysis of certain heavy-ion collision observables. Another possibility is to study the (2317) production in photonucleon reactions. Whith the 12 GeV Upgrade of the CEBAF accelerator at Jefferson Lab., the (2317) can be produced in reactions of the type: gp ® L

0. Therefore, if the coupling constant, , is found to be very different depending on the structure for (2317), then the photo-production of (2317) can be used as a signal to descriminate its structure.

II. THE COUPLING CONSTANT

The coupling, , defined through the effective lagrangian

was evaluated in ref. [18], supposing that the meson (2317) is a conventional state. They got:

Here, we extend the calculation done in refs. [14, 15] to study the hadronic vertex DsJ DK. The QCDSR calculation for the vertex, DsJDK, centers around the three-point function given by

where is the interpolating field for the scalar DsJ meson [9]:

where a, b, c, ... are colour indices and C is the charge conjugation matrix. In Eq. (4), p = p' +q and the interpolating fields for the kaon and for the D mesons are given by:

where q stands for the light quark u or d.

The calculation of the phenomenological side proceeds by inserting intermediate states for D, K and DsJ, and by using the definitions: á 0 | | K(q) ñ = iq µ FK, á 0 | jD | D(p') ñ = , á 0 | (p) ñ = l . We obtain the following relation:

where the coupling constant, , is defined by the on-mass-shell matrix element: á DK | DsJ ñ = . The continuum contribution in Eq.(7) contains the contributions of all possible excited states.

In the case of the light scalar mesons, considered as diquark-antidiquark states, the study of their vertex functions using the QCD sum rule approach at the pion pole [12, 13, 19], was done in ref.[20]. It was shown that the decay widths determined from the QCD sum rule calculation are consistent with existing experimental data. Here, we follow ref. [21] and work at the kaon pole. The main reason for working at the kaon pole is that one does not have to deal with the complications associated with the extrapolation of the form factor [22]. The kaon pole method consists in neglecting the kaon mass in the denominator of Eq. (7) and working at q2 = 0. In the OPE side one singles out the leading terms in the operator product expansion of Eq.(4) that match the 1/q2 term. Since we are working at q2 = 0, we take the limit p2 = p'2 and we apply a single Borel transformation to p2,p'2® M2. On the phenomenological side, in the structure q µ we get:

where A and r cc(u) stands for the pole-continuum transitions and pure continuum contributions, with s0 and u0 being the continuum thresholds for DsJ and D respectively [14, 15]. For simplicity, one assumes that the pure continuum contribution to the spectral density, r cc(u), is given by the result obtained in the OPE side. Therefore, one uses the ansatz: r cc(u) = r OPE(u). In Eq.(8), A is a parameter which, together with , has to be determined by the sum rule.

On the OPE side we single out the leading terms proportional to q µ /q2. Transferring the pure continuum contribution to the OPE side, the sum rule for the coupling constant, up to dimension 7, is given by:

with

III. RESULTS AND CONCLUSIONS

In the numerical analysis of the sum rules, the values used for the meson masses, quark masses and condensates are: = 2.317 GeV, mD = 1.87 GeV, mc = 1.2 GeV, ms = .13 GeV á ñ = -(0.23)3 GeV3, á ñ = 0.8 á ñ . For the meson decay constants we use FK = 160 MeV and fD = 0.22 GeV [23]. We use u0 = 6 GeV2 and for the current meson coupling, l , we are going to use the result obtained from the two-point function in ref. [9]. Considering 2.6 < < 2.8 GeV we get l = (2.9 ± 0.3)×10-3 GeV5.

In Fig. 1 we show, through the dots, the right-hand side (RHS) of Eq.(9) as a function of the Borel mass. To determine we fit the QCDSR results with the analytical expression in the left-hand side (LHS) of Eq.(9):

Using = 2.7 GeV we get: C = 4.53×10-4 GeV7 and A = -4.68×10-4 GeV7. Using the definition of C in Eq.(10) and l = 2.9×10-3 GeV5 (the value obtained for = 2.7 GeV) we get = 2.8 GeV. Allowing s0 to vary in the interval 2.6 < < 2.8 GeV, the corresponding variation obtained for the coupling constant is

Fixing = 2.7 GeV and varying the quark condensate, the charm quark and the strange quark masses in the intervals: -(0.24)3< á ñ < -(0.22)3 GeV3, 1.1 < mc < 1.3 GeV and 0.11 < ms < 0.15 GeV, we get results for the coupling constant still between the lower and upper limits given above. it is important to mention that the agreement between the RHS and LHS of the sum rule in Fig.1 is not so good, in this case, as it was in the case of the couplings and evaluated in refs. [14, 15]. One possible reason for that is the fact that the kaon mass is much bigger than the pion mass. Therefore, neglecting the kaon mass in Eq. (7) is not an approximation as good as it is in the case of the sum rule in the pion pole.


We have presented a QCD sum rule study of the vertex function associated with the hadronic vertex DsJDK, where the DsJ(2317) meson was considered as diquark-antidiquark state. Comparing the results in Eqs. (12) and (3) we see that when the meson DsJ(2317) is considered as a conventional state one gets a coupling constant much bigger than when DsJ(2317) is considered a four-quark state. This result can be usefull to experimentally investigate the quark structure of the meson DsJ(2317) through, for example, its photo-production on nucleon targets.

Acknowledgements

This work has been supported by CNPq and FAPESP.

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[8] for a review see E. S. Swanson, Phys. Rept. 429, 243 (2006).

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[10] R. Matheus, S. Narison, M. Nielsen, and J.-M. Richard, hep-ph/0608297.

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[12] L. J. Reinders, H. Rubinstein, and S. Yazaky, Phys. Rep. 127, 1 (1985).

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[14] M. Nielsen, Phys. Lett. B 634, 35 (2006).

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[16] F. S. Navarra and M. Nielsen, Phys. Lett. B 639, 272 (2006).

[17] A. D. Polosa, hep-ph/0609137.

[18] Z. G. Wang, S.L. Wan, Phys. Rev. D 73, 094020 (2006).

[19] S. Narison, Phys. Lett. B 175, 88 (1986); S. Narison and R. Tarrach, Phys. Lett. B 125, 217 (1983).

[20] T. V. Brito et al., Phys. Lett. B 608, 69 (2005).

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[22] R. S. Marques de Carvalho et al., Phys. Rev. D 60, 034009 (1999).

[23] CLEO Coll., M. Artuso et al., Phys. Rev. Lett. 95, 251801 (2005).

Received on 24 October, 2006; revised version received on 18 January, 2007

  • [1] BABAR Coll., B. Auber et al., Phys. Rev. Lett. 90, 242001 (2003);
  • Phys. Rev. D 69, 031101 (2004).
  • [2] CLEO Coll., D. Besson et al., Phys. Rev. D 68, 032002 (2003).
  • [3] BELLE Coll., S.-L. Choi et al., Phys. Rev. Lett. 91, 262001 (2003).
  • [4] BELLE Coll., K. Abe et al., Phys. Rev. D 69, 112002 (2004).
  • [5] R. L. Jaffe, Phys. Rev. D 15, 267, 281 (1977); D 17, 1444 (1978).
  • [6] for a review see F. E. Close, and N. A. Törnqvist, J. Phys. G 28, R249 (2002).
  • [7] K. Abe et al. [Belle Collaboration], hep-ex/0505037, hep-ex/0505038.
  • [8] for a review see E. S. Swanson, Phys. Rept. 429, 243 (2006).
  • [9] M.E. Bracco et al., Phys. Lett. B 624, 217 (2005).
  • [10] R. Matheus, S. Narison, M. Nielsen, and J.-M. Richard, hep-ph/0608297.
  • [11] M. A. Shifman, A. I. and Vainshtein, and V.I. Zakharov, Nucl. Phys., B 147, 385 (1979).
  • [12] L. J. Reinders, H. Rubinstein, and S. Yazaky, Phys. Rep. 127, 1 (1985).
  • [13] S. Narison, QCD spectral sum rules , World Sci. Lect. Notes Phys. 26, 1;
  • QCD as a theory of hadrons, Cambridge Monogr. Part. Phys. Nucl. Phys. Cosmol.17, 1 (2002) [hep-h/0205006]
  • [14] M. Nielsen, Phys. Lett. B 634, 35 (2006).
  • [15] M. Nielsen, F. S. Navarra, and M. E. Bracco hep-ph/0609184.
  • [16] F. S. Navarra and M. Nielsen, Phys. Lett. B 639, 272 (2006).
  • [17] A. D. Polosa, hep-ph/0609137.
  • [18] Z. G. Wang, S.L. Wan, Phys. Rev. D 73, 094020 (2006).
  • [19] S. Narison, Phys. Lett. B 175, 88 (1986);
  • S. Narison and R. Tarrach, Phys. Lett. B 125, 217 (1983).
  • [20] T. V. Brito et al., Phys. Lett. B 608, 69 (2005).
  • [21] M. E. Bracco, F. S. Navarra, and M. Nielsen, Phys. Lett. B 454, 346 (1999).
  • [22] R. S. Marques de Carvalho et al., Phys. Rev. D 60, 034009 (1999).
  • [23] CLEO Coll., M. Artuso et al., Phys. Rev. Lett. 95, 251801 (2005).

Publication Dates

  • Publication in this collection
    10 Aug 2007
  • Date of issue
    June 2007

History

  • Reviewed
    18 Jan 2007
  • Received
    24 Oct 2006
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