Abstract

Thermodynamic properties of systems with repulsive interactions, are considered in the grand canonical ensemble. The analytic structure of the excluded-volume model in the complex plane of the system chemical potential (fugacity) is elaborated, based on the fact that the pressure function can be given in terms of the Lambert W-function. Even though the excluded volume model has no phase transitions at real values of the chemical potential, it does exhibit a branch cut singularity in the complex plane, thus limiting the convergence range of the Taylor expansion in the chemical potential. Close similarities to analytic properties of the other models with repulsive interactions, such as a cluster expansion model, the mean-field model, and the ideal Fermi gas model, are pointed out. As an example, repulsive baryonic interactions in a hadron gas, with a focus on the fugacity/virial and Taylor expansion methods used in lattice QCD, are presented. The asymptotic behavior of the Fourier expansion coefficients in these various models suggests that the singular part of net baryonic density can to leading order be universally expressed in terms of polylogarithms.

Highlights

  • Properties of strongly interacting matter and determination of its different phases are the key questions that drive the heavy-ion collision experiments as well as finite-temperature lattice QCD simulations

  • The indirect lattice methods to probe finite baryon densities are based on extrapolations such as analytic continuation from imaginary chemical potential [1,2,3] or the Taylor expansion method [4,5,6,7,8]

  • The convergence ranges of the Taylor expansion method are often restricted just by pressure function singularities, which are not at all related to physical phase transitions

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Summary

INTRODUCTION

Properties of strongly interacting matter and determination of its different phases are the key questions that drive the heavy-ion collision experiments as well as finite-temperature lattice QCD simulations. The indirect lattice methods to probe finite baryon densities are based on extrapolations such as analytic continuation from imaginary chemical potential [1,2,3] or the Taylor expansion method [4,5,6,7,8]. Both methods are sensitive to the analytic properties of the pressure function in the complex chemical potential plane, in particular its singularities.

SINGLE-COMPONENT EXCLUDED-VOLUME MODEL
Excluded-volume HRG model
Taylor expansion properties
Fourier coefficients
COMPARISON TO OTHER APPROACHES
Mean-field approach
Cluster expansion model
Ideal Fermi gas
Some remarks on the radius of convergence
Modeling the singular part of net baryon density with polylogarithms
Findings
SUMMARY
Full Text
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