2+1 flavors QCD equation of state at zero temperature within Dyson-Schwinger equations
arXiv:1506.06846 · doi:10.1142/S0217751X15502176
Abstract
Within the framework of Dyson-Schwinger equations (DSEs), we discuss the equation of state (EOS) and quark number densities of 2+1 flavors, that is to say, , , and quarks. The chemical equilibrium and electric charge neutrality conditions are used to constrain the chemical potential of different quarks. The EOS in the cases of 2 flavors and 2+1 flavors are discussed, and the quark number densities, the pressure, and energy density per baryon are also studied. The results show that there is a critical chemical potential for each flavor of quark, at which the quark number density turns to nonzero from 0; and furthermore, the system with 2+1 flavors of quarks is more stable than that with 2 flavors in the system. These discussion may provide some useful information to some research fields, such as the studies related to the QCD phase transitions or compact stars.
arXiv comment7 pages, 6 figures
References in corpus (52)
- QCD Phenomenology based on a Chiral Effective Lagrangian
- NJL-model analysis of dense quark matter
- Dyson-Schwinger Equations and the Application to Hadronic Physics
- Full result for the QCD equation of state with 2+1 flavors
- Chiral effective model with the Polyakov loop
- The QCD transition temperature: results with physical masses in the continuum limit
- Phases of QCD: lattice thermodynamics and a field theoretical model
- Is there still any Tc mystery in lattice QCD? Results with physical masses in the continuum limit III
- Critical point of QCD at finite T and μ, lattice results for physical quark masses
- Dyson-Schwinger Equations: Density, Temperature and Continuum Strong QCD
- On the Phase Diagram of QCD
- Dyson-Schwinger equations: a tool for hadron physics
- The QCD Equation of State with almost Physical Quark Masses
- Phase diagrams in the three-flavor Nambu--Jona-Lasinio model with the Polyakov loop
- Bethe-Salpeter Study of Vector Meson Masses and Decay Constants
- Astrophysical Measurement of the Equation of State of Neutron Star Matter
- The transition temperature in QCD
- EXO 0748-676 Rules out Soft Equations of State for Neutron Star Matter
- Small, Dense Quark Stars from Perturbative QCD
- Explanation and Prediction of Observables using Continuum Strong QCD
- The equation of state in lattice QCD: with physical quark masses towards the continuum limit
- Analytic properties of the Landau gauge gluon and quark propagators
- Quark matter in compact stars?
- QCD Thermodynamics with Three Flavors of Improved Staggered Quarks
- Interaction model for the gap equation
- The Equation of State of Deconfined Matter at Finite Chemical Potential in a Quasiparticle Description
- Hadron Properties and Dyson-Schwinger Equations
- Non-perturbative comparison of QCD effective charges
- Reconstructing the Neutron-Star Equation of State from Astrophysical Measurements
- Modern compact star observations and the quark matter equation of state
- Thermodynamics of the PNJL model
- Critical endpoint in the Polyakov-loop extended NJL model
- Equation of state for neutron stars in SU(3) flavor symmetry
- QCD equation of state with 2+1 flavors of improved staggered quarks
- Confinement Phenomenology in the Bethe-Salpeter Equation
- QCD effective charges from lattice data
- Quark stars within relativistic models
- The chiral phase transition with a chiral chemical potential in the framework of Dyson-Schwinger equations
- Locate QCD Critical End Point in a Continuum Model Study
- The calculation of the equation of state of QCD at finite chemical potential and zero temperature
- Flavour symmetry breaking in the kaon parton distribution amplitude
- New Class of Compact Stars at High Density
- Equation of state in 2+1 flavor QCD with improved Wilson quarks by the fixed scale approach
- End Point of a First-Order Phase Transition in Many-Flavor Lattice QCD at Finite Temperature and Density
- Connecting neutron star observations to the high density equation of state of quasi-particle model
- The Wigner Solution and QCD Phase Transitions in a Modified PNJL Model
- Studies of two-solar-mass hybrid stars within the framework of Dyson-Schwinger equations
- Nonlinear susceptibilities under the framework of Dyson-Schwinger equations
- Dynamical chiral symmetry breaking in the NJL model with a constant external magnetic field
- Continuum study of various susceptibilities within thermal QED
- Influence of gauge boson mass on the staggered spin susceptibility
- Nature of chiral phase transition in QED at zero density
Cited by in corpus (7)
- QCD at finite temperature and chemical potential from Dyson-Schwinger equations
- Baryon number fluctuations in the QCD phase diagram from Dyson-Schwinger equations
- Hybrid and quark star matter based on a non-perturbative equation of state
- Nonperturbative quark matter equations of state with vector interactions
- Thermodynamics from the quark condensate
- Detectability of a phase transition in neutron star matter with third-generation gravitational wave interferometers
- QCD phase transition and equation of state of stellar strong interaction matter via Dyson-Schwinger equation approach