$K^-$ and $\bar p$ Spectra for Au+Au Collisions at $\sqrt{s}$ = 200 GeV from STAR, PHENIX and BRAHMS in Comparison to Core-Corona Model Predictions
C. Schreiber, K. Werner, J. Aichelin

TL;DR
This paper extends the core-corona model to analyze the centrality dependence of $K^-$ and $ar{p}$ spectra in Au+Au collisions at 200 GeV, highlighting data discrepancies among experiments and questioning collective expansion interpretations.
Contribution
It applies the core-corona model to new particle spectra and discusses the impact of experimental differences on model parameters and interpretations.
Findings
Model describes centrality dependence of spectra well for some particles.
Data discrepancies affect model parameter extraction.
Centrality dependence of average momentum varies with particle species.
Abstract
Based on results obtained with event generators we have launched the core-corona model. It describes in a simplified way but quite successfully the centrality dependence of multiplicity and of identified particles observed in heavy-ion reaction at beam energies between = 17 GeV and 200 GeV. Also the centrality dependence of the elliptic flow, , for all charged and identified particles could be explained in this model. Here we extend this analysis and study the centrality dependence of single particle spectra of and measured by the PHENIX, STAR and BRAHMS collaborations. We find that also for these particles the analysis of the spectra in the core-corona model suffers from differences in the data published by the different experimental groups, notably for the pp collisions. As for protons and for each experience the data agree well with the…
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