Nonlocal PNJL models and heavy hybrid stars (CROSBI ID 597591)
Prilog sa skupa u zborniku | izvorni znanstveni rad | međunarodna recenzija
Podaci o odgovornosti
Blaschke, David ; Alvarez Castillo, David A. ; Benić, Sanjin ; Contrera, Gustavo ; Lastowiecki, Rafal
engleski
Nonlocal PNJL models and heavy hybrid stars
Nonlocal PNJL models allow for a detailed description of chiral quark dynamics with running quark masses and wave function renormalization in accordance with lattice QCD (LQCD) in vacuum. Their generalization to finite temperature T and chemical potential m allows to reproduce the m-dependence of the pseudocritical temperature from LQCD when a nonvanishing vector meson coupling is adjusted. This restricts the region for the critical endpoint in the QCD phase diagram and stiffens the quark matter equation of state (EoS). It is demonstrated that the construction of a hybrid EoS for compact star applications within a two-phase approach employing the nonlocal PNJL EoS and an advanced hadronic EoS leads to the masquerade problem. A density dependence of the vector meson coupling is suggested as a possible solution which can be adjusted in a suitable way to describe hybrid stars with a maximum mass in excess of 2 M⊙ with a possible early onset of quark deconfinement even in the cores of typical (M ∼ 1.4 M⊙) neutron stars.
compact stars; QCD phase diagram; quark models
nije evidentirano
nije evidentirano
nije evidentirano
nije evidentirano
nije evidentirano
nije evidentirano
Podaci o prilogu
249-8.
2012.
objavljeno
Podaci o matičnoj publikaciji
Podaci o skupu
10th Conference on Quark Confinement and the Hadron Spectrum
predavanje
08.10.2012-12.10.2012
München, Njemačka