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Role of the conserved charges in the chiral symmetry restoration phase transition

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arxiv 2009.01781 v1 pith:BIN2GIMB submitted 2020-09-03 hep-ph nucl-th

Role of the conserved charges in the chiral symmetry restoration phase transition

classification hep-ph nucl-th
keywords matterchargechargesconserveddenseformationinteractionphase
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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The effect of conserved baryon, isospin and strangeness charges on the behavior of phase transitions in dense matter is studied. Baryonic matter is described within the three-flavor Polyakov$-$Nambu$-$Jona-Lasinio model and several charge fractions $Y_Q$ are considered. The role of the vector interaction, which can be important to describe dense systems, is discussed. Special attention is given to the case with charge fraction $Y_Q=0.4$, due to its importance in heavy-ion collisions and core-collapse supernova matter. It is shown that the possible formation of chiral-symmetric quark matter in the laboratory will be favored in asymmetric matter. Besides, the inclusion of the vector interaction reinforces the formation of quark matter at lower densities.

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