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Freeze-out temperature from net-kaon fluctuations at energies available at the BNL Relativistic Heavy Ion Collider

R. Bellwied, J. Noronha-Hostler, P. Parotto, I. Portillo Vazquez, C. Ratti, and J. M. Stafford
Phys. Rev. C 99, 034912 – Published 29 March 2019

Abstract

We compare the mean-over-variance ratio of the net-kaon distribution calculated within the hadron resonance gas model to the latest experimental data from the Beam Energy Scan at the Relativistic Heavy Ion Collider by the STAR Collaboration. Our analysis indicates that it is not possible to reproduce the experimental results using the freeze-out parameters from the existing combined fit of net-proton and net-electric charge mean over variance. The strange mesons need about 15 MeV higher temperatures than the light hadrons at the highest collision energies. In view of the future Λ fluctuation measurements, we predict the Λ variance over mean and skewness times variance at the light and strange chemical freeze-out parameters. We observe that the Λ fluctuations are sensitive to the difference in the freeze-out temperatures established in this analysis. Our results have implications for other phenomenological models in the field of relativistic heavy ion collisions.

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  • Received 19 June 2018

DOI:https://doi.org/10.1103/PhysRevC.99.034912

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI. Funded by SCOAP3.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

R. Bellwied1, J. Noronha-Hostler2, P. Parotto1, I. Portillo Vazquez1, C. Ratti1,*, and J. M. Stafford1

  • 1Department of Physics, University of Houston, Houston, Texas 77204, USA
  • 2Department of Physics and Astronomy, Rutgers University, Piscataway, New Jersey 08854, USA

  • *Corresponding author: cratti@uh.edu

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Issue

Vol. 99, Iss. 3 — March 2019

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