A Hydrodynamic Description of Heavy Ion Collisions at the SPS and RHIC
D. Teaney, J. Lauret, E. V. Shuryak
TL;DR
This work develops a hydro+cascade framework to describe relativistic heavy-ion collisions across SPS to RHIC energies, using an EOS with tunable latent heat to capture both the soft and hard features of the QCD phase transition. By coupling 2D relativistic hydrodynamics to a hadronic cascade via Cooper-Frye emission, and by varying the latent-heat parameter LH, the authors reproduce radial and elliptic flow observables for multiple particle species, centralities, and energies, with LH8 providing the best global agreement. The study shows that strong early QGP pressure, followed by differential hadronic freezeout, naturally explains the RHIC-era data, including the elevated ⟨M_T⟩, the p_T-dependent elliptic flow, and the anomalous ⟨p̄⟩/π− ratios, while highlighting the importance of hadronic rescattering for final-state spectra. The results underscore the sensitivity of collective flow to the EOS and freezeout dynamics, offering a quantitative link between macroscopic fluid behavior and microscopic hadronic interactions, and point to ongoing challenges such as HBT radii to be resolved in future work.
Abstract
A hydrodynamic + cascade model of relativistic heavy ion collisions is presented and compared to available hadronic data from the SPS to RHIC. The model consistently reproduces the radial and elliptic flow data for different particles, collision energies, and impact parameters. Three ingredients are essential to the success: (a) a reasonable EOS exhibiting the hard and soft features of the QCD phase transition, (b) thermal hadronization at the phase boundary, and (c) subsequent hadronic rescattering. Some features of the RHIC data are readily explained: (i) the observed elliptic flow and its dependence on $p_{T}$ and mass, (ii) the anomalous $\bar{p}/π^{-}$ ratio for $p_{T} \approx 2.0$ GeV, (iii) the difference in the slope parameters measured by the STAR and PHENIX collaborations, and (iv) the respectively strong and weak impact parameter dependence of the $\bar{p}$ and $φ$ slope parameters. For an EOS without the hard and soft features of the QCD phase transition, the broad consistency with the data is lost.
