English

Higher order cumulants of net baryon-number distributions at non-zero $\mu_B$

High Energy Physics - Lattice 2021-02-03 v1 High Energy Physics - Phenomenology Nuclear Theory

Abstract

Using recent results on higher order cumulants of conserved charge fluctuations from lattice QCD, we construct mean, variance, skewness, kurtosis, hyper-skewness and hyper-kurtosis of net-baryon number distributions for small baryon chemical potentials μB\mu_B. For the strangeness neutral case (μS=0\mu_S=0) at fixed ratio of electric charge to baryon number density (nQnB=0.4\frac{n_Q}{n_B}=0.4), which is appropriate for a comparison with heavy ion collisions, we present results for κBσB2\kappa_B \sigma_B^2, SBσB3/MBS_B \sigma_B^3/M_B, κBHσB4\kappa^{H}_{B}\sigma_{B}^4 and SBHσB5/MBS^{H}_{B}\sigma^5_{B}/M_{B} on the crossover line for the chiral transition, Tpc(μB)T_{pc}(\mu_B). Continuum extrapolations for this pseudo-critical transition line have recently been reported by HotQCD up to baryon chemical potentials μB300\mu_B\simeq 300 MeV [arXiv:1812.08235]. These cumulant ratios are of direct relevance for comparisons with corresponding ratios measured by STAR in the BES-I and II runs at beam energies sNN20\sqrt{s_{NN}}\ge 20 GeV. In particular, we point out that recent high statistics results on skewness and kurtosis of net-baryon number distributions obtained by STAR at sNN=54.4\sqrt{s_{NN}} = 54.4 GeV put strong constraints on freeze-out parameters and are consistent with predictions from thermal QCD.

Keywords

Cite

@article{arxiv.2002.01837,
  title  = {Higher order cumulants of net baryon-number distributions at non-zero $\mu_B$},
  author = {Dennis Bollweg and Frithjof Karsch and Swagato Mukherjee and Christian Schmidt},
  journal= {arXiv preprint arXiv:2002.01837},
  year   = {2021}
}

Comments

4 pages, 6 figures, Contribution to the Quark Matter 2019 Conference Proceedings