Many models have been suggested to describe inelastic charmonium production in the framework of perturbative QCD, such as the color-singlet model (CSM) [167,169,168,170], the color-evaporation model [171,172] and soft color interactions [173]. Most recently the ansatz of non-relativistic quantum chromodynamics (NRQCD) factorization was introduced in which colour octet states contribute to the charmonium production cross section.
Theoretical calculations based on the NRQCD factorization approach [174,175,176] are available in leading order [177,178,179,180,181,182]. In the NRQCD factorization approach the size of the color octet contributions, which are described by long distance matrix elements (LDME), are additional free parameters and have been determined in fits to the Tevatron data [183]. The NRQCD factorization approach contains the color singlet model which is recovered in the limit in which the long distance matrix elements tend to zero.
For and photoproduction, the CSM calculations are available including next-to-leading order contributions [184,185]. Alternatively, using the CSM, inelastic production can be modeled in the factorization approach (see section 2.5) using an unintegrated ( dependent) gluon density in the proton [187,186,190].
Figure 41 shows data from CDF [191,192] together with CSM calculations to leading order and fitted color octet contributions. It can be seen that the color octet contributions are large, leading to a good description of the data. Unfortunately those long distance matrix elements which are most important in and photoproduction at HERA, are not well constrained by the Tevatron data and thus contain large uncertainties [165]. The new charmonium results from the Tevatron Run-II (see e.g.fig.7) which provide much more statistics and extend to lower values of could help to reduce the uncertainties of the LDME significantly.
It should be noted that next-to-leading-order corrections might change the size of the color octet contributions substantially. Although the NLO terms have not been calculated in the NRQCD approach, effects that are similar to those in the CSM may be expected, in which the NLO terms lead to an increase in the cross section of typically a factor two, with a strong dependence.
Figure 42 shows the measurements of the cross section by the H1 collaboration [29] and the ZEUS collaboration [32], compared with the theoretical predictions given in Ref. [165]. The variable denotes the fraction of the photon energy in the proton rest frame that is transferred to the and is defined as
The data are not corrected for feeddown processes from diffractive and inelastic production of mesons ( ), the production of hadrons with subsequent decays to mesons, or feeddown from the production of states. The latter two contributions are estimated to contribute between 5% at medium and 30% at the lowest values of .
The open band in fig.42 represents the sum of the color-singlet and color-octet contributions, calculated in leading order NRQCD. The uncertainty is due to the uncertainty in the color-octet NRQCD matrix elements. The shaded band shows the calculation of the color-singlet contribution to next-to-leading order in [184,185] which describes the data quite well without the inclusion of a color-octet contribution. The next-to-leading-order QCD corrections are crucial in describing the shape of the transverse-momentum distribution of the .
The factorization approach [187,188,189,190] has been applied for production [186]. Figure 43 shows a comparison of the data with the predictions from the factorization approach as implemented in the Monte Carlo generator CASCADE. Good agreement is observed between data and predictions for . At high values, the CASCADE calculation underestimates the cross section. The CASCADE predictions for the the dependence of the cross section (fig.43c) fit the data considerably better than the collinear LO calculations (dotted curve in fig.42b). This improved fit is attributed to the transverse momentum of the gluons from the proton, which contribute to the transverse momentum of the meson.
The polarization of the meson is expected to differ in the various theoretical approaches discussed here and could in principle be used to distinguish between them, independently of normalization uncertainties. The general decay angular distribution can be parameterized as
(11) |
In fig.44, the data are shown, together with the results from two LO calculations: the NRQCD prediction, including color-octet and color-singlet contributions [178], and the color-singlet contribution alone. In contrast to the predictions shown in fig.44, in which is zero or positive, the prediction of the factorization approach is that should become increasingly negative toward larger values of , reaching at GeV. However, at present, the errors in the data preclude any firm conclusions. In order to distinguish between full NRQCD and the color-singlet contribution alone, measurements at larger are required. The measured values of , for which no prediction is available from the factorization approach, slightly favor the full NRQCD prediction.
In conclusion, it should be noted that calculations to next-to-leading order, which are not yet available in the framework of NRQCD factorization, could be an essential ingredient in a full quantitative understanding of charmonium production at HERA, and also at other experiments, such as those at the Tevatron.