Quartic cumulant of baryon number in the presence of a QCD critical point

D. Mroczek, A. R. Nava Acuna, J. Noronha-Hostler, P. Parotto, C. Ratti, and M. A. Stephanov
Phys. Rev. C 103, 034901 – Published 4 March 2021

Abstract

In the context of the ongoing search for the QCD critical point at the Relativistic Heavy-Ion Collider, we study the equation of state near the critical point in the temperature and baryon chemical potential plane. We use the parametric representation introduced in earlier literature, which maps the universal three-dimensional Ising equation of state onto the QCD phase diagram using several non-universal parameters. We focus on the quartic cumulant of the baryon number, or baryon number susceptibility χ4B, which can be accessed experimentally via net-proton fluctuation kurtosis measurements. It was originally predicted, through universality arguments based on the leading singular contribution, that χ4B and net-proton kurtosis should show a specific nonmonotonic behavior due to the critical point. In particular, when following the freeze-out curve on the phase diagram by decreasing beam energy, the kurtosis is expected to dip, and then peak, when the beam energy scan passes close to the critical point. We study the effects of the nonuniversal and thus far unknown parameters of the Ising-to-QCD mapping on the behavior of χ4B. We find that, while the peak remains a solid feature, the presence of the critical point does not necessarily cause a dip in χ4B on the freeze-out line below the transition temperature. The critical point contribution to the dip appears only for a narrow set of mapping parameters, when subleading singular terms are sufficiently suppressed.

  • Figure
  • Figure
  • Figure
  • Figure
  • Received 8 September 2020
  • Accepted 22 February 2021

DOI:https://doi.org/10.1103/PhysRevC.103.034901

©2021 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

D. Mroczek

  • Illinois Center for Advanced Studies of the Universe, Department of Physics, University of Illinois at Urbana-Champaign, Urbana, Illinois 61801, USA

A. R. Nava Acuna

  • Department of Physics, University of Houston, Houston, Texas 77204, USA

J. Noronha-Hostler

  • Illinois Center for Advanced Studies of the Universe, Department of Physics, University of Illinois at Urbana-Champaign, Urbana, Illinois 61801, USA

P. Parotto*

  • Department of Physics, University of Wuppertal, Wuppertal D-42119, Germany

C. Ratti

  • Department of Physics, University of Houston, Houston, Texas 77204, USA

M. A. Stephanov

  • Physics Department, University of Illinois at Chicago, Chicago, Illinois 60607, USA

  • *Corresponding author: parotto@uni-wuppertal.de

Article Text (Subscription Required)

Click to Expand

References (Subscription Required)

Click to Expand
Issue

Vol. 103, Iss. 3 — March 2021

Reuse & Permissions
Access Options
CHORUS

Article Available via CHORUS

Download Accepted Manuscript
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review C

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×