Publications (9)8.89 Total impact
 [Show abstract] [Hide abstract]
ABSTRACT: The recent measurements of the masses of the pulsars PSR J16142230 and PSR J03480432 provide independent proof for the existence of neutron stars with masses in range of 2 $M_\odot$. This fact has significant implications for the physics of high density matter and it challenges the hypothesis that the cores of NS can be composed of deconfined quark matter. In this contribution we study a description of quark matter based on the NambuJonaLasinio effective model and construct the equation of state for matter in beta equilibrium. This equation of state together with the hadronic DiracBruecknerHartreeFock equation of state is used here to describe neutron star and hybrid star configurations. We show that compact stars masses of 2 $M_\odot$ are compatible with the possible existence of deconfined quark matter in their core.  [Show abstract] [Hide abstract]
ABSTRACT: We study the role of finitesize effects at the hadronquark phase transition in a new hybrid equation of state constructed from an abinitio Br\"ucknerHartreeFock equation of state with the realistic BonnB potential for the hadronic phase and a covariant nonlocal NambuJonaLasinio model for the quark phase. We construct static hybrid star sequences and find that our model can support stable hybrid stars with an onset of quark matter below $2 M_\odot$ and a maximum mass above $2.17 M_\odot$ in agreement with recent observations. If the finitesize effects are taken into account the core is composed of pure quark matter. Provided that the quark vector channel interaction is small, and the finite size effects are taken into account, quark matter appears at densities 23 times the nuclear saturation density. In that case the proton fraction in the hadronic phase remains below the value required by the onset of the direct URCA process, so that the early onset of quark matter shall affect on the rapid cooling of the star.  [Show abstract] [Hide abstract]
ABSTRACT: We study the possibility that the transition from hadron matter to quark matter at vanishing temperatures proceeds via crossover, similar to the crossover behavior found with lattice QCD studies at high temperatures. The purpose is to examine astrophysical consequences of this postulate by constructing hybrid star sequences fulfilling current experimental data.  [Show abstract] [Hide abstract]
ABSTRACT: 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 \mu{} allows to reproduce the \mudependence 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 twophase 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_sun with a possible early onset of quark deconfinement even in the cores of typical (M ~ 1.4 M_sun) neutron stars.  [Show abstract] [Hide abstract]
ABSTRACT: We discuss a threeflavor NambuJonaLasinio model for the quark matter equation of state with scalar diquark interaction, isoscalar vector interaction and KobayashiMaskawa’t Hooft interaction. We adopt a phenomenological scheme to include possible effects of a change in the gluon pressure at finite baryon density by including a parametric dependence of the Polyakovloop potential on the chemical potential. We discuss the results for the massradius relationships for hybrid neutron stars constructed on the basis of our model EoS in the context of the constraint from the recently measured mass of (1.97 ± 0.04) M ⊙ for the pulsar PSR J16142230.  [Show abstract] [Hide abstract]
ABSTRACT: The measurement of the mass 1.97 +/ 0.04 M_sun for PSR J16142230 provides a new constraint on the equation of state and composition of matter at high densities. In this contribution we investigate the possibility that the dense cores of neutron stars could contain strange quarks either in a confined state (hyperonic matter) or in a deconfined one (strange quark matter) while fulfilling a set of constraints including the new maximum mass constraint. We account for the possible appearance of hyperons within an extended version of the densitydependent relativistic meanfield model, including the phimeson interaction channel. Deconfined quark matter is described by the color superconducting threeflavor NJL model.  [Show abstract] [Hide abstract]
ABSTRACT: Large neutron star masses as the recently measured $1.97\pm0.04$ M$_\odot$ for PSR J16142230 provide a valuable lower limit on the stiffness of the equation of state of dense, nuclear and quark matter. Complementary, the analysis of the elliptic flow in heavy ion collisions suggests an upper limit on the EoS stiffness. We illustrate how this dichotomy permits to constrain parameters of effective EoS models which otherwise could not be derived unambiguously from first principles.  [Show abstract] [Hide abstract]
ABSTRACT: We discuss a threeflavor NambuJonaLasinio (NJL) type quantum field theoretical approach to the quark matter equation of state (EoS) with scalar diquark condensate, isoscalar vector mean field and KobayashiMaskawa't Hooft (KMT) determinant interaction. While often the diquark and vector meson couplings are considered as free parameters, we will fix them here to their values according to the Fierz transformation of a onegluon exchange interaction. In order to estimate the effect of a possible change in the vacuum pressure of the gluon sector at finite baryon density we exploit a recent modification of the Polyakovloop NJL (mPNJL) model which introduces a parametric density dependence of the Polyakovloop potential also at T=0, thus being relevant for compact star physics. We use a DiracBruecknerHartreeFock (DBHF) EoS for the hadronic matter phase and discuss results for massradius relationships following from a solution of the TOV equations for such a hybrid EoS in the context of observational constraints from selected objects.  [Show abstract] [Hide abstract]
ABSTRACT: We discuss a NambuJonaLasinio (NJL) type quantum field theoretical approach to the quark matter equation of state with color superconductivity and construct hybrid star models on this basis. It has recently been demonstrated that with increasing baryon density, the different quark flavors may occur sequentially, starting with downquarks only, before the second light quark flavor and at highest densities also the strange quark flavor appears. We find that color superconducting phases are favorable over nonsuperconducting ones which entails consequences for thermodynamic and transport properties of hybrid star matter. In particular, for NJLtype models no strange quark matter phases can occur in compact star interiors due to mechanical instability against gravitational collapse, unless a sufficiently strong flavor mixing as provided by the KobayashiMaskawa't Hooft determinant interaction is present in the model. We discuss observational data on massradius relationships of compact stars which can put constraints on the properties of dense matter equation of state. Comment: 7 pages, 2 figures, to appear in the Proceedings of the International Conference SQM2009, Buzios, Rio de Janeiro, Brazil, Sep.27Oct.2, 2009
Publication Stats
82  Citations  
8.89  Total Impact Points  
Top Journals
Institutions

20102014

University of Wroclaw
Vrotslav, Lower Silesian Voivodeship, Poland
