Cluster Expansion Model for QCD Baryon Number Fluctuations: No Phase Transition at $\mu_B / T < \pi$
Volodymyr Vovchenko, Jan Steinheimer, Owe Philipsen, Horst Stoecker

TL;DR
This paper introduces a Cluster Expansion Model for QCD baryon fluctuations, matching lattice data and predicting no phase transition at baryochemical potential over temperature less than pi, with implications for understanding QCD phase structure.
Contribution
The paper develops a relativistic cluster expansion model for QCD baryon fluctuations, accurately fitting lattice data and analyzing the convergence of pressure expansions without indicating a phase transition below rac{rac{rac{rac{pi}
Findings
Excellent agreement with lattice data for baryon susceptibilities
Predicted higher order susceptibilities not yet available from lattice
No evidence of phase transition at rac{rac{rac{rac{pi}
Abstract
A Cluster Expansion Model (CEM), representing a relativistic extension of Mayer's cluster expansion, is constructed to study baryon number fluctuations in QCD. The temperature dependent first two coefficients, corresponding to the partial pressures in the baryon number and sectors, are the only model input, which we fix by recent lattice data at imaginary baryochemical potential. All other coefficients are constructed in terms of the first two and required to match the Stefan-Boltzmann limit at . The CEM allows calculations of the baryon number susceptibilities to arbitrary order. We obtain excellent agreement with available lattice data for the baryon fluctuation measures , , and predict higher order susceptibilities, that are not yet available from Lattice QCD. The calculated susceptibilities are then used to…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
