Elliptic flow of charged pions, protons and strange particles emitted in Pb+Au collisions at top SPS energy

TL;DR

This study measures the elliptic flow of various charged particles in Pb+Au collisions at SPS energy, comparing results to hydrodynamic models and discussing implications for hadronic evolution and flow dynamics.

Contribution

It provides detailed measurements of elliptic flow spectra for multiple particle species at SPS energy and compares them with ideal hydrodynamics, highlighting the effects of hadronic stages.

Findings

Flow magnitudes decrease with decreasing pT, even below hydro predictions.

Proton v2(pT) shows a downward trend and negative values at low pT.

Pion flow asymmetry impacts proton flow but does not alter main conclusions.

Abstract

Differential elliptic flow spectra v2(pT) of \pi-, K0short, p, \Lambda have been measured at \sqrt(s NN)= 17.3 GeV around midrapidity by the CERN-CERES/NA45 experiment in mid-central Pb+Au collisions (10% of \sigma(geo)). The pT range extends from about 0.1 GeV/c (0.55 GeV/c for \Lambda) to more than 2 GeV/c. Protons below 0.4 GeV/c are directly identified by dE/dx. At higher pT, proton elliptic flow v2(pT) is derived as a constituent, besides \pi+ and K+, of the elliptic flow of positive pion candidates. The retrieval requires additional inputs: (i) of the particle composition, and (ii) of v2(pT) of positive pions. For (i), particle ratios obtained by NA49 were adapted to CERES conditions; for (ii), the measured v2(pT) of negative pions is substituted, assuming \pi+ and \pi- elliptic flow magnitudes to be sufficiently close. The v2(pT) spectra are compared to ideal-hydrodynamics calculations. In synopsis of the series \pi- - K0short - p - \Lambda, flow magnitudes are seen to fall with decreasing pT progressively even below hydro calculations with early kinetic freeze-out (Tf= 160 MeV) leaving not much time for hadronic evolution. The proton v2(pT) data show a downward swing towards low pT with excursions into negative v2 values. The pion-flow isospin asymmetry observed recently by STAR at RHIC, invalidating in principle our working assumption, is found in its impact on proton flow bracketed from above by the direct proton flow data, and not to alter any of our conclusions. Results are discussed in perspective of recent viscous dynamics studies which focus on late hadronic stages.