J/\psi and \psi^{\prime} production in proton(deuteron)-nucleus collisions: lessons from RHIC for the proton-lead LHC run

and production in proton(deuteron)-nucleus collisions: lessons from RHIC for the proton-lead LHC run

E. G. Ferreiro    F. Fleuret    J.P. Lansberg and A. Rakotozafindrabe Departamento de Física de Partículas and IGFAE, Universidad de Santiago de Compostela, 15782 Santiago de Compostela, Spain
 
Laboratoire Leprince Ringuet, École Polytechnique, CNRS/IN2P3, 91128 Palaiseau, France
 
IPNO, Université Paris-Sud, CNRS/IN2P3, F-91406, Orsay, France
 
IRFU/SPhN, CEA Saclay, 91191 Gif-sur-Yvette Cedex, France
elena@fpaxp1.usc.es
Abstract

We study the impact of different cold nuclear matter effects both on and production, among them the modification of the gluon distribution in bound nucleons, commonly known as gluon shadowing, and the survival probability for a bound state to escape the nucleus –the nuclear absorption. Less conventional effects such as saturation and fractional energy loss are also discussed. We pay a particular attention to the recent PHENIX preliminary data on production in Au collisions at GeV, which show a strong suppression for central collisions, 5 times larger than the one obtained for production at the same energy. We conclude that none of the abovementioned mechanisms can explain this experimental result.

1 Introduction

The properties of the production and the absorption of quarkonium in proton(deuteron)-nucleus collisions, such as and suppression in Au collisions at RHIC, offer the opportunity to study Cold Nuclear Matter (CNM) effects in the nuclear medium. This is of particular relevance for the understanding of QCD at high density and temperature in nucleus-nucleus collisions, since it is in fact adventurous to claim that the charmonium family is a quark-gluon plasma (QGP) thermometer [1] without calibrating first the CNM suppression.

We have studied the impact of different cold nuclear matter effects both on and production, namely the survival probability for a bound state to escape the nucleus –the nuclear absorption– and the modification of the gluon distribution in bound nucleons –gluon shadowing. Alternative mechanisms such as saturation and fractional energy loss are also considered.

We have then discussed whether these CNM effects could explain (or not) the data on and within a coherent picture. We have paid a special attention to the recent PHENIX preliminary data [2] on production in Au collisions at GeV, which show a strong suppression for central collisions in the mid-rapidity region.

2 Propagation in the cold nuclear matter: vs

The probability for the heavy-quark pair to be broken up in the propagation through the nuclear medium is commonly known as the nuclear absorption. It is usually parametrised by an effective break-up cross section .

In principle, the larger size of the compared to the tells us that the should suffer more break-up than the . Nevertheless, it is important to remember that the relevant timescale to analyse the pair evolution is its formation time, which, following the uncertainty principle, is related to the time needed – in their rest frame – to distinguish the energy levels of the and states, GeV / 4 GeV fm for the . Moreover, has to be considered in the rest frame of the target nucleus, i.e. the Au beam at RHIC. The boost factor is obtained from the rapidity of the pair corrected by the Au beam rapidity where for RHIC.

The formation time for the different rapidities reached at RHIC are given in Table 1.

-2.0 14.4 5.1 fm 0.0 106 36.7 fm
-1.5 23.7 8.3 fm +1.5 476 166 fm
-1.0 39 14 fm +2.0 786 271 fm
Table 1: Boost and formation-time -dependence in the Au rest frame of the at GeV.

As it is shown there, in the mid and forward rapidity regions at RHIC, is significantly larger than the Au radius. This means that the is nearly always in a pre-resonant state when traversing the nuclear matter. This implies that the break-up probability should be the same for the and , since these states cannot be distinguished at the time they traverse the nucleus.

3 Gluon shadowing and antishadowing

At high energy, the nucleons in a nucleus shadow each other, leading to a modification of the nuclear Parton Distribution Functions (nPDF). This modification, in the form of a shadowing-correction factor, has to be applied to the or yield in Au collisions. This shadowing factor can be expressed in terms of the ratios of the nPDF in a nucleon of a nucleus  to the PDF in the free nucleon.

We shall consider three different shadowing parametrisations: EKS98 [3], EPS08 [4] and nDSg [5] at LO, which have been implemented in our Glauber Monte-Carlo framework JIN [6], already used to describe production at RHIC [7, 8, 9]. Our code accounts for improved kinematics corresponding to a () partonic process for the production as in the Colour-Singlet Model at LO [10] or the Colour-Octet Mechanism at NLO.

In Fig. 1, the effect of the nPDFs on is compared to PHENIX data on and production [2]. We have used the three shadowing parametrisations mentioned above, together with four possibilities for the effective nuclear absortion, namely mb.

Figure 1: Nuclear modification factor in Au collisions, , for and as measured by PHENIX at GeV versus the number of collisions for the mid-rapidity range compared to our computations for four values of the nuclear absorption (from top to bottom: mb) using EKS98 (left), EPS08 (middle) and nDSg (right).

Note that, while the choice of identical break-up cross sections for and is perfectly justified given the argument of large formation times invoked above, the common prejudice that there is a similar shadowing in both cases needs further explanations. It is true that the shadowing corrections, that depends on and , should be very similar for both particle production, due to their similar masses. Nevertheless, the difference between their masses –of the order of GeV– could induce both a shift on the corresponding at a given rapidity and on the corresponding . We have taken the factorisation scale, , equal to the particle mass, 3.7 GeV for the and 3.1 GeV for the . In Fig. 2, our results for the ratio between the shadowing factors for different shadowing parametrisations –EKS98, EPS08, nDSg at LO along with EPS09 at LO and NLO [11] and nDSg at NLO– are shown.

Figure 2: over nuclear modification factors in the rapidity range (left) and in the mid-rapidity region (right) using EKS98 (black), EPS08 (red), nDSg (green) and EPS09 (blue) at LO (continous line) and NLO (discontinous line). The shaded zone indicates that is there of the order of the Au radius. In this region, the and absorption may be slightly different.

Note that the difference of the shadowing impact is at most 5 %. Even more important, this difference will favour production in the mid-rapidity region, in contradiction to what experimental data show.

4 Other effects: gluon saturation and fractional energy loss

The possibility of a gluon saturation as predicted in the framework of the Color Glass Condensate (CGC) [12, 13] is sometimes invoked to have an impact on quarkonium production. We have already discussed [14] that this impact would be negligible in the case of production at RHIC energies. Let us now discuss if it could affect and production. The relevant scale below which one expects significant non-linear effects in the evolution of the gluon distributions in A is the saturation momentum. It can be evaluated as [15] , with and . Typical values for RHIC kinematics are given in Table. 2 together with the ratio of to the mass.

(GeV) (GeV)
-2.2
-1.2
0 0.3
1.2
2.2
Table 2: Evaluation of the saturation scale in the Au nucleus, , at  GeV in Au collisions as a function of the and rapidities.

Note that in the backward rapidity region is always above –the maximum momentum fraction below which parton saturation can be considered. In the mid and forward rapidity regions, the saturation scale is always below the typical energy scale of the process, namely or . In particular, in the mid-rapidity region the ratio of to the mass is , which makes unlikely the possibility of specific saturation effects. Only in the most forward rapidity region there is a small probability for phenomena beyond collinear factorisation i.e. beyond those encoded in the nPDFs. Moreover, these effects –if they exist– would suppress the slightly more than the , in contradiction to the experimental results.

Recently, the possibility of a medium-induced energy loss that scales with the energy has been pointed out [16]. This fractional energy loss would affect the heavy-quark pair produced in a coloured state provided that it has long enough time to radiate. The fraction of medium-induced radiated energy is given by , where is the broadening of the radiated gluon from the proton and is the transverse mass of the final-state coloured object. If 100% of the ’s were produced in a coloured state at RHIC, . Assuming that the corresponding suppression factor is just the ratio between the PDF of the gluon evaluated at its original , before the loss and the PDF at the resulting : . Taking modern global-fit gluon PDFs, we find that this fractional energy loss could give an extra suppression of the order of 10% in the mid-rapidity region and up to 15% in the forward region. Note that this suppression only applies when the is produced in a coloured state, and that its effect is similar in and production due to their similar masses111In fact, the higher mass of the would lead to a smaller value of , which is compensated by an increase of the mean value of when compared to the case. This makes the quantitative difference between the and the indistinguishable.. Thus, this cannot explain the experimental found either.

In conclusion, we have studied different CNM effects and their impact on and production. We have shown that, at RHIC energies and in the mid-rapidity region, the results from the four CNM effects which we investigated, namely an effective nuclear absorption, the gluon shadowing, the gluon saturation and a fractional energy loss, impact similarly the and the , in contradiction to the recent PHENIX preliminary data on production in Au collisions at 200 GeV. The abovementioned effects should be taken into account in the interpretation of the upcoming LHC data on and production.

Acknowledgments: This work was partially supported by the Ministerio de Ciencia (Spain) & the IN2P3 (France) (AIC-D-2011-0740).

References

  • [1] T. Matsui and H. Satz, Phys. Lett. B 178 (1986) 416.
  • [2] T. Sakaguchi [PHENIX Collaboration], arXiv:1211.0324 [nucl-ex].
  • [3] K. J. Eskola, V. J. Kolhinen, C. A. Salgado, Eur. Phys. J. C 9 (1999) 61.
  • [4] K. J. Eskola, H. Paukkunen, C. A. Salgado, JHEP 0807 (2008) 102.
  • [5] D. de Florian, R. Sassot, Phys. Rev. D 69 (2004) 074028.
  • [6] E. G. Ferreiro, F. Fleuret and A. Rakotozafindrabe, Eur. Phys. J. C 61 (2009) 859.
  • [7] E. G. Ferreiro, F. Fleuret, J. P. Lansberg and A. Rakotozafindrabe, Phys. Lett. B 680, 50 (2009).
  • [8] E. G. Ferreiro, F. Fleuret, J. P. Lansberg and A. Rakotozafindrabe, Phys. Rev. C 81 (2010) 064911.
  • [9] E. G. Ferreiro, F. Fleuret, J. P. Lansberg, N. Matagne and A. Rakotozafindrabe, Few Body Syst. 53 (2012) 27.
  • [10] S. J. Brodsky, J. P. Lansberg, Phys. Rev. D 81 (2010) 051502.
  • [11] K. J. Eskola, H. Paukkunen, C. A. Salgado, JHEP 0904 (2009) 065.
  • [12] E. Iancu, A. Leonidov and L. D. McLerran, Nucl. Phys. A 692 (2001) 583.
  • [13] E. Ferreiro, E. Iancu, A. Leonidov and L. McLerran, Nucl. Phys. A 703 (2002) 489.
  • [14] E. G. Ferreiro, F. Fleuret, J. P. Lansberg, N. Matagne and A. Rakotozafindrabe, arXiv:1110.5047 [hep-ph].
  • [15] J.L. Albacete, N. Armesto, J.G. Milhano, P. Quiroga-Arias and C.A. Salgado, Eur. Phys. J. C 71 (2011) 1705.
  • [16] F. Arleo, S. Peigne and T. Sami, Phys. Rev. D 83 (2011) 114036.
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