Neutron stars: from the inner crust to the core with the (Extended) Nambu-Jona-Lasinio model
arXiv:1603.01239 · doi:10.1103/PhysRevC.93.065805
Abstract
Nucleonic matter is described within a su(2) extended Nambu-Jona-Lasinio model. Several parametrizations with different nuclear matter saturation properties are proposed. At subsaturation, nuclear pasta phases are calculated within two methods: the coexistence-phases approximation and the compressible liquid drop model, with the surface tension coefficient determined using a geometrical approach at zero temperature. An unified equation of state of stellar matter for the inner crust, with the nuclear pasta phases, and the core is calculated. The mass and radius of neutron stars within this framework are obtained for several families of hadronic and hybrid stars. The quark phase of hybrid stars is described within the su(3) NJL model including a vector term. Stellar macroscopic properties are in accordance with some of the recent results in the literature.
13 pages, 10 figures, published version
References in corpus (21)
- Shapiro delay measurement of a two solar mass neutron star
- A Massive Pulsar in a Compact Relativistic Binary
- The Dense Matter Equation of State from Neutron Star Radius and Mass Measurements
- A new quark-hadron hybrid equation of state for astrophysics - I. High-mass twin compact stars
- Core-crust transition in neutron stars: predictivity of density developments
- The symmetry energy at subnuclear densities and nuclei in neutron star crusts
- Improved Mass and Radius Constraints for Quiescent Neutron Stars in Omega Cen and NGC 6397
- Formation of Nuclear "Pasta" in Supernovae
- Neutron Star Radii, Universal Relations, and the Role of Prior Distributions
- The effect of accretion on the measurement of neutron star mass and radius in the low-mass X-ray binary 4U 1608-52
- The mass and the radius of the neutron star in the transient low mass X-ray binary SAX J1748.9-2021
- Neutron stars with hyperon cores: stellar radii and EOS near nuclear density
- Stability of CFL cores in Hybrid Stars
- Effects of the symmetry energy on properties of neutron star crusts near the neutron drip density
- Nuclear matter in the crust of neutron stars derived from realistic NN interactions
- Light clusters, pasta phases and phase transitions in core-collapse supernova matter
- Cluster formation in compact stars: relativistic versus Skyrme models
- Repulsive Vector Interaction in Three Flavor Magnetized Quark and Stellar Matter
- Impact of nuclear "pasta" on neutrino transport in collapsing stellar cores
- On the compactness of neutron stars
- The pasta phase and its consequences on neutrino opacities
Cited by in corpus (18)
- Surface tension of dense matter at the chiral phase transition
- Two-solar-mass hybrid stars: a two model description with the Nambu-Jona-Lasinio quark model
- Broken SU(6) symmetry and massive hybrid stars
- A Neutron Star is born
- Nuclear Statistical Equilibrium Equation of State for Core Collapse
- Dense Matter in Neutron Stars with eXTP
- The effect of the energy functional on the pasta-phase properties of catalysed neutron stars
- Hadron-quark phase transition in the SU(3) local Nambu-Jona-Lasinio (NJL) model with vector interaction
- Regularization of the Nambu-Jona Lasinio model under a uniform magnetic field and the role of the anomalous magnetic moments
- Hyperon threshold and stellar radii
- Pasta phases within the QMC model
- Symmetry energy and neutron star properties in the saturated Nambu-Jona-Lasinio model
- Hyperons in the pasta phase
- A general framework to diagonalize vector--scalar and axial-vector--pseudoscalar transitions in the effective meson Lagrangian
- Nambu-Jona-Lasinio description of hadronic matter from a Bayesian approach
- Hadron-quark phase transition: the QCD phase diagram and stellar conversion
- Neutron star equation of state: identifying hadronic matter characteristics
- Symmetry potentials and in-medium nucleon-nucleon cross sections within the Nambu-Jona-Lasinio model in relativistic impulse approximation