Properties of Hot Quark Matter with Neutrino Confinement in the NJL Model

被引:0
作者
G. S. Hajyan
G. B. Alaverdyan
机构
[1] Erevan State University,
来源
Astrophysics | 2022年 / 65卷
关键词
hot quark matter; neutrino confinement; NJL model; equation of state;
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摘要
The thermodynamic characteristics of hot β-equilibrium three-flavor quark matter with neutrino confinement are studied in terms of the local SU(3) Nambu-Jona-Lasinio (NJL) model, which also accounts for the ‘t Hooft interaction which leads to mixing of quark flavors. For different temperatures T ∈ [20 ÷100] MeV and baryon number densities nB ∈ [0 ÷ 1.8] fm-3 the constituent quark masses, quark condensates, and relative contributions of individual types of particles to the pressure and chemical potentials of the constituent particles are determined. In order to determine the role of neutrinos in the hot quark matter, the pressures and energies in states with and without neutrinos are compared.
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页码:126 / 136
页数:10
相关论文
共 23 条
[1]  
Hajyan GS(2021)undefined Astrophysics 64 370-undefined
[2]  
Alaverdyan GB(1961)undefined Phys. Rev. 122 345-undefined
[3]  
Nambu Y(1961)undefined Phys. Rev. 124 246-undefined
[4]  
Jona-Lasinio G(1976)undefined Phys. Rev. D 14 2755-undefined
[5]  
Nambu Y(1976)undefined Prog. Theor. Phys. 56 947-undefined
[6]  
Jona-Lasinio G(1996)undefined Phys. Rev. C 53 410-undefined
[7]  
Eguchi O(2005)undefined Phys. Rep. 407 205-undefined
[8]  
Kikkawa E(2006)undefined Usp. Fiz. Nauk 176 569-undefined
[9]  
Rehberg P(2021)undefined Symmetry 13 124-undefined
[10]  
Klevansky SP(1963)undefined Voprosy kosmogonii 9 91-undefined