Open charm production in relativistic nucleus–nucleus collisions
✍ Scribed by W. Cassing; E.L. Bratkovskaya; A. Sibirtsev
- Publisher
- Elsevier Science
- Year
- 2001
- Tongue
- English
- Weight
- 534 KB
- Volume
- 691
- Category
- Article
- ISSN
- 0375-9474
No coin nor oath required. For personal study only.
✦ Synopsis
We calculate excitation functions for open charm mesons in Au + Au reactions from AGS to RHIC energies within the HSD transport approach which is based on string, quark, diquark (q, q, qq, q q) and hadronic degrees of freedom. The open charm cross sections from pN and πN reactions are fitted to results from PYTHIA and scaled in magnitude to the available experimental data. From our dynamical calculations we find an approximate m T -scaling for pions, kaons, D mesons and J/Ψ -when discarding final-state elastic scattering of kaons and φ mesons with pions -in central collisions of Au + Au at 160 A GeV (with an apparent slope of 176 MeV) without employing the assumption of a Quark-Gluon Plasma (QGP). We demonstrate that this result is essentially due to a relative m T -scaling in pp collisions at √ s ≈ 17.3 GeV. At lower bombarding energies of 25 A GeV a suppression of D mesons by a factor of ∼ 10 relative to a global m T -scaling with slope 143 MeV is expected. However, when incorporating attractive D-meson self-energies as suggested by QCD sum rules, an approximate m T -scaling is regained even at 25 A GeV. The effects of D-meson rescattering and charmonium absorption are discussed, furthermore, with respect to rapidity and transverse mass distributions in central collisions of Au + Au at 25, 160 A GeV and 21.3 A TeV.
📜 SIMILAR VOLUMES
For relativistic beam nuclei up to 4He and medium heavy target nuclei, absorption cross sections and partial production cross sections are computed. Eclipse corrections are found to be essential. For C, N, and 0 beam nuclei, Coulomb dissociation is computed.