Study of nuclear matter properties for Hybrid EoS
arXiv:2003.06101 · doi:10.1088/1361-6471/aba116
Abstract
We study the nuclear matter properties like symmetry energy, slope parameter, curvature, skewness and incompressibility for Hybrid EoS. The hybrid EoS is constructed using the recently proposed Effective-Field-Theory motivated Relativistic Mean-Field model (E-RMF) for the hadron phase with different parameter sets and MIT Bag model for the quark phase with different Bag constants to construct hybrid EoS. The mixed-phase formed by the hadron-quark phase transition is studied using the Gibbs construction. The nuclear matter properties for hybrid EoS are calculated and their variation with the bag constant is determined.
arXiv comment22 pages, 12 figures
References in corpus (49)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Shapiro delay measurement of a two solar mass neutron star
- A Massive Pulsar in a Compact Relativistic Binary
- Neutron Star Structure and the Equation of State
- GW190425: Observation of a Compact Binary Coalescence with Total Mass
- A New Parameterization for the Lagrangian Density of Relativistic Mean Field Theory
- Determination of the Equation of State of Dense Matter
- NJL-model analysis of dense quark matter
- Masses, Radii, and Equation of State of Neutron Stars
- Equations of state for supernovae and compact stars
- Neutron Star Structure and the Neutron Radius of 208Pb
- Using gravitational-wave observations and quasi-universal relations to constrain the maximum mass of neutron stars
- From hadrons to quarks in neutron stars: a review
- Neutron-Rich Nuclei in Heaven and Earth
- Skyrme Interaction and Nuclear Matter Constraints
- The Equation of State of Hot, Dense Matter and Neutron Stars
- Nuclear symmetry energy probed by neutron skin thickness of nuclei
- Neutron Radii in Mean-Field Models
- Neutron skin of 208Pb, nuclear symmetry energy, and the parity radius experiment
- Measuring the neutron star equation of state using X-ray timing
- Relativistic effective interaction for nuclei, giant resonances, and neutron stars
- Constraining the neutron-proton effective mass splitting using empirical constraints on the density dependence of nuclear symmetry energy around normal density
- The equation of state for dense nucleonic matter from a metamodeling. I. Foundational aspects
- Connecting Neutron Star Observations to Three-Body Forces in Neutron Matter and to the Nuclear Symmetry Energy
- Composition, Structure and Evolution of Neutron Stars with Kaon Condensates
- The hadron-quark phase transition in dense matter and neutron stars
- Analysis of Chiral Mean-Field Models for Nuclei
- Relativistic mean field interaction with density dependent meson-nucleon vertices based on microscopical calculations
- Nuclear Matter in Relativistic Mean Field Theory with Isovector Scalar Meson
- Searching for isovector signatures in the neutron-rich oxygen and calcium isotopes
- Nuclear symmetry energy and its density slope at normal density extracted from global nucleon optical potentials
- Quark deconfinement in high-mass neutron stars
- A survey of the parameter space of the compressible liquid drop model as applied to the neutron star inner crust
- Symmetry energy from the nuclear collective motion: constraints from dipole, quadrupole, monopole and spin-dipole resonances
- Quark-Hadron Phase Transitions in Young and Old Neutron Stars
- Neutron stars and quark phases in the NJL model
- New relativistic effective interaction for finite nuclei, infinite nuclear matter and neutron stars
- New parameterization of the effective field theory motivated relativistic mean field model
- Tidal deformability of neutron and hyperon star with relativistic mean field equations of state
- Quark Hadron Phase Transition and Hybrid Stars
- Generic Constraints on the Relativistic Mean-Field and Skyrme-Hartree-Fock Models from the Pure Neutron Matter Equation of State
- Symmetry Energy Constraints from Giant Resonances: A Theoretical Overview
- Versatility of field theory motivated nuclear effective Lagrangian approach
- Asymmetric nuclear matter in the relativistic mean field approach with vector cross-interaction
- Quark deconfinement transition in neutron stars with the field correlator method
- Phase transition and properties of compact star
- Fundamental quantum limits to waveform detection
- The effect of isoscalar-isovector coupling in infinite nuclear matter
- Effects of quark-matter symmetry energy on hadron-quark coexistence in neutron-star matter