# Baryon number fluctuations in chiral effective models and their   phenomenological implications

**Authors:** Gabor Almasi, Bengt Friman, Krzysztof Redlich

arXiv: 1703.05947 · 2017-08-02

## TL;DR

This paper investigates net-baryon-number fluctuations near the chiral phase transition using a QCD-inspired model, comparing results with experimental data and exploring effects of model assumptions and nonequilibrium dynamics.

## Contribution

It applies the Functional Renormalization Group to a Polyakov-loop extended Quark-Meson model to analyze baryon fluctuations and compares theoretical predictions with RHIC data.

## Key findings

- Model results agree with experimental data at higher energies.
- Discrepancy observed in the fourth cumulant below 19.6 GeV.
- Vector interactions influence the location of the critical endpoint.

## Abstract

We study the critical properties of net-baryon-number fluctuations at the chiral restoration transition in a medium at finite temperature and net baryon density. The chiral dynamics of quantum chromodynamics (QCD) is modeled by the Polykov-loop extended Quark-Meson Lagrangian, that includes the coupling of quarks to vector meson and temporal gauge fields. The Functional Renormalization Group is employed to properly account for the $O(4)$ criticality at the phase boundary. We focus on the properties and systematics of ratios of the net-baryon-number cumulants $\chi_B^n$, for ${1\leq n\leq 6}$, near the phase boundary. The results are presented in the context of the recent experimental data of the STAR Collaboration on fluctuations of the net proton number in heavy ion collisions at RHIC. We show that the model results for the energy dependence of the cumulant ratios are in good overall agreement with the data, with one exception. At center-of-mass energies below ${19.6\;\mathrm{GeV}}$, we find that the measured fourth-order cumulant deviates considerably from the model results, which incorporate the expected $O(4)$ and $Z(2)$ criticality. We assess the influence of model assumptions and in particular of repulsive vector-interactions, which are used to modify the location of the critical endpoint in the model, on the cumulants ratios. Finally, we discuss a possibility to test to what extent the fluctuations are affected by nonequilibrium dynamics by comparing certain ratios of cumulants.

## Full text

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## Figures

19 figures with captions in the complete paper: https://tomesphere.com/paper/1703.05947/full.md

## References

94 references — full list in the complete paper: https://tomesphere.com/paper/1703.05947/full.md

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Source: https://tomesphere.com/paper/1703.05947