Abstract

We present a dynamical description of (anti)proton number fluctuations cumulants and correlation functions in central Au-Au collisions at $\sqrt{s_{\rm NN}} = 7.7-200$ GeV by utilizing viscous hydrodynamics simulations. The cumulants of proton and baryon number are calculated in a given momentum acceptance analytically, via an appropriately extended Cooper-Frye procedure describing particlization of an interacting hadron resonance gas. The effects of global baryon number conservation are taken into account using a generalized subensemble acceptance method. The experimental data of the STAR collaboration are consistent at $\sqrt{s_{\rm NN}} \gtrsim 20$ GeV with simultaneous effects of global baryon number conservation and repulsive interactions in baryon sector, the latter being in line with the behavior of baryon number susceptibilities observed in lattice QCD. The data at lower collision energies show possible indications for sizable attractive interactions among baryons. The data also indicate sizable negative two-particle correlations between antiprotons that are not satisfactorily described by baryon conservation and excluded volume effects. We also discuss differences between cumulants and correlation functions (factorial cumulants) of (anti)proton number distribution, proton versus baryon number fluctuations, and effects of hadronic afterburner.

Highlights

  • Proton number fluctuations are one of the key observables in the beam energy scan (BES) program at RHIC [1]

  • The results presented that incorporate the effect of global baryon conservation have all been obtained using subensemble acceptance method (SAM)-2.0

  • The cumulants have been calculated in the momentum acceptance where experimental measurements have been performed by the STAR Collaboration

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Summary

INTRODUCTION

Proton number fluctuations are one of the key observables in the beam energy scan (BES) program at RHIC [1]. The STAR Collaboration has recently presented measurements of (net-)proton number cumulants up to fourth order from BES-I [9,10]. We calculate the cumulants of (anti)proton number distribution emitted from the hypersurface subject to global baryon conservation analytically For this purpose we use a recently developed subensemble acceptance method 2.0 (SAM-2.0) [40], which allows one to perform a correction of cumulants of accepted protons for the effect of exact global baryon conservation analytically.

CUMULANTS FROM HYDRODYNAMICS
Hydrodynamics
Cumulants of baryon-proton number distribution at particlization
Correction for global baryon conservation
RESULTS
Rapidity distributions
Net proton cumulants
Acceptance dependence
Centrality dependence
Protons versus baryons
DISCUSSION AND SUMMARY
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