Abstract

Hot and dense quark matter with isospin and chiral imbalances is investigated in the framework of the (3+1)-dimensional Nambu–Jona-Lasinio model (NJL) in the large-N_c limit (N_c is the number of quark colors). Its phase structure is considered in terms of barion – mu _B, isospin – mu _I and chiral isospin – mu _{I5} chemical potentials. It is shown in the paper that (i) in the chiral limit there is a duality between chiral symmetry breaking (CSB) and charged pion condensation (PC) phenomena. (ii) At the physical point, i.e. at nonzero bare quark mass m_0, and temperature this duality relation is only approximate, although rather accurate. (iii) We have shown that the chiral isospin chemical potential mu _{I5} in dense quark matter generates charged pion condensation both at zero and nonzero m_0, and at mu _{I5}ne 0 this phase might be observed up to temperatures as high as 100 MeV. (iv) Pseudo-critical temperature of the chiral crossover transition rises in the NJL model with increasing mu _{I5}. (v) It has been found an agreement between particular sections of the phase diagram in the framework of NJL model and corresponding ones in lattice QCD simulations. Two different plots from different lattice simulations that are completely independent and are not connected at the first sight are in reality dual to each other, it means that lattice QCD simulations support the hypothesis that in real quark matter there exists the (approximate) duality between CSB and charged PC. Moreover, we can reverse the logic and we can predict the increase of pseudo-critical temperature with chiral chemical potential, the much debated effect recently, just by the duality notion, hence bolster confidence in this result (lattice QCD showed this feature for unphysically large pion mass) and put it on the considerably more solid ground.

Highlights

  • At normal (Earth) conditions, protons and neutrons form atomic nuclei, and the latter, together with their orbital electrons, form the ordinary matter of our environment

  • It is worth to note that the phase structure of the isospin imbalanced quark matter below the threshold is an important question because even small nonzero μI could double the critical endpoint of a phase diagram and affects the results of heavy-ion collision experiments [12,41,42]. It has been shown in the framework of the massless (3+1)-dimensional Nambu–Jona-Lasinio model (NJL) model that chiral imbalance promotes charged pion condensation (PC) phase in dense matter at zero temperature [43,44] and responsible for the existence of the duality between chiral symmetry breaking (CSB) and charged PC phases

  • Another purpose is to study in the framework of the NJL4 model the fate of the duality observed in the chiral limit [43] between CSB and charged PC phenomena in the leading large-Nc order: we investigate the influence of the bare quark mass and temperature on this effect, etc

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Summary

Introduction

At normal (Earth) conditions, protons and neutrons form atomic nuclei, and the latter, together with their orbital electrons, form the ordinary matter of our environment. One of the aims of our present work is to check the robustness of the charged PC phase generated by chiral imbalance under the influence of these destructive factors Another purpose is to study in the framework of the NJL4 model the fate of the duality observed in the chiral limit [43] (where it is an exact symmetry) between CSB and charged PC phenomena in the leading large-Nc order: we investigate the influence of the bare quark mass and temperature on this effect, etc. In addition to charged PC phase, in the present paper we investigate in the framework of the NJL4 model at m0 = 0 the dependence of the (pseudo-)critical temperature, which characterizes the chiral cross-over region of the phase diagram, on the chiral isospin chemical potential μI 5 and compare our results with other effective model investigations and lattice simulations on this topic. Some technical details and issues not directly related to this work are relegated to “Appendices A and B”

Lagrangian and symmetries
Thermodynamical potential
Thermodynamical potential: non-zero temperature case
Technical details
Phase structure of the model
Summary and discussion
Full Text
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