Title of article
How far is normal nuclear matter from the chiral symmetry restoration?
Author/Authors
Mishustin، نويسنده , , I.N. and Satarov، نويسنده , , L.M. and Greiner، نويسنده , , W.، نويسنده ,
Pages
18
From page
363
To page
380
Abstract
Properties of cold nuclear matter are studied within a generalized Nambu–Jona–Lasinio model formulated on the level of constituent nucleons. The model parameters are chosen to reproduce simultaneously the observed nucleon and pion masses in vacuum as well as saturation properties of nuclear matter. The strongest constraints on these parameters are given by the empirical values of the nucleon effective mass and compression modulus at nuclear saturation density. A preferable value of the cutoff momentum, determining density of active quasinucleon states in the Dirac sea, is estimated to about 400 MeV/c. With the most reasonable choice of model parameters we have found a first-order phase transition of the liquid–gas type at subsaturation densities and the gradual restoration of chiral symmetry at about three times the saturation density. Fluctuations of the scalar condensate around its mean-field value are estimated and shown to be large in the vicinity of chiral transition.
Keywords
chiral symmetry restoration , Nuclear matter
Journal title
Astroparticle Physics
Record number
2002975
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