Abstract

The self-consistent mean field approximation of two-flavor NJL model, which introduces a free parameter $\alpha$ ($\alpha$ reflects the weight of different interaction channels), is employed to investigate the contributions of the vector-channel at finite isospin chemical potential $\mu_I$ and zero baryon chemical potential $\mu_B$ and zero temperature $T$. The calculations show that the consideration of the vector-channel contributions leads to lower value of pion condensate in superfluid phase, compared with the standard Lagrangian of NJL model ($\alpha=0$). In superfluid phase, we also obtain lower isospin number density, and the discrepancy is getting larger with the increase of isospin potential. Compared with the recent results from Lattice QCD, the isospin density and energy density we obtained with $\alpha=0.5$ agree with the data of lattice well. In the phase diagram in the $T-\mu_I$ plane for $\mu_B=0$, we can see that the difference of the critical temperatures of phase transition between the results with $\alpha=0$ and $\alpha=0.5$ is up to $3\%-5\%$ for a fixed isospin potential. All of these indicate that the vector channels play an important role in isospin medium.

Highlights

  • The study of thermodynamics of strongly interacting system under extreme conditions is helpful for us to develop a better understanding to the physical scene shortly after the big bang [1,2], the structure of compact stars [3,4], and heavy-ion collision experiments [5,6]

  • We will show our results with different α’s, α 1⁄4 0 represents the standard NJL model [26], α 1⁄4 0.5 is found to be in good agreement with recent lattice data, α 1⁄4 0.9 is adopted from Ref. [35], and α 1⁄4 1.044 is taken from Ref. [34]

  • We find that in superfluid phase (π ≠ 0), the lower value of the pion condensate and the higher value of the σ condensate appear with the increasing α compared with that of the α 1⁄4 0 case, and the largest difference of the pion condensate occurs at μI ∼ 1.5mπ

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Summary

Introduction

The study of thermodynamics of strongly interacting system under extreme conditions is helpful for us to develop a better understanding to the physical scene shortly after the big bang [1,2], the structure of compact stars [3,4], and heavy-ion collision experiments [5,6]. The probe of the properties of strongly interacting matter at such large temperatures and densities is carried on at CERN, BNL, and GSI, etc.

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