English

Open charm and charmonium production at relativistic energies

Nuclear Theory 2009-11-10 v2

Abstract

We calculate open charm and charmonium production in Au+AuAu+Au reactions at s\sqrt{s} = 200 GeV within the hadron-string dynamics (HSD) transport approach employing open charm cross sections from pNpN and πN\pi N reactions that are fitted to results from PYTHIA and scaled in magnitude to the available experimental data. Charmonium dissociation with nucleons and formed mesons to open charm (D+DˉD+\bar{D} pairs) is included dynamically. The 'comover' dissociation cross sections are described by a simple phase-space model including a single free parameter, i.e. an interaction strength M02M_0^2, that is fitted to the J/ΨJ/\Psi suppression data for Pb+PbPb+Pb collisions at SPS energies. As a novel feature we implement the backward channels for charmonium reproduction by DDˉD \bar{D} channels employing detailed balance. From our dynamical calculations we find that the charmonium recreation is comparable to the dissociation by 'comoving' mesons. This leads to the final result that the total J/ΨJ/\Psi suppression at s\sqrt{s} = 200 GeV as a function of centrality is slightly less than the suppression seen at SPS energies by the NA50 Collaboration, where the 'comover' dissociation is substantial and the backward channels play no role. Furthermore, even in case that all directly produced J/ΨJ/\Psi mesons dissociate immediately (or are not formed as a mesonic state), a sizeable amount of charmonia is found asymptotically due to the D+DˉJ/ΨD+\bar{D} \to J/\Psi + meson channels in central collisions of Au+AuAu+Au at s\sqrt{s} = 200 GeV which, however, is lower than the J/ΨJ/\Psi yield expected from binary scaling of pppp collisions.

Keywords

Cite

@article{arxiv.nucl-th/0301083,
  title  = {Open charm and charmonium production at relativistic energies},
  author = {E. L. Bratkovskaya and W. Cassing and H. Stoecker},
  journal= {arXiv preprint arXiv:nucl-th/0301083},
  year   = {2009}
}

Comments

42 pages, including 14 eps figures, discussions extended and references added, to be published in Phys. Rev. C