Tabulated Neutron Star Equations of State Modeled within the Chiral Mean Field Model

Abstract

In this special issue article, I review some of the accomplishments of the chiral mean field (CMF) model, which contains nucleon, hyperon, and quark degrees of freedom, and its applications to proto-neutron and neutron stars. I also present a set of equation of state and particle population tables built using the CMF model subject to physical constraints necessary to reproduce different environments, such as those present in cold neutron stars, core-collapse supernova explosions and different stages of compact star mergers.

PASA special issue on the Neutron Stars, related to the Compstar conference in Warsaw

References in corpus (8)

• Shapiro delay measurement of a two solar mass neutron star
• A Massive Pulsar in a Compact Relativistic Binary
• The order of the quantum chromodynamics transition predicted by the standard model of particle physics
• Proto-Neutron and Neutron Stars in a Chiral SU(3) Model
• Hyperon Puzzle, Hadron-Quark Crossover and Massive Neutron Stars
• Neutron stars within the SU(2) parity doublet model
• The axial anomaly and the phases of dense QCD
• A self-consistent study of magnetic field effects on hybrid stars

Cited by in corpus (17)

• The Science of the Einstein Telescope
• On the Deconfinement Phase Transition in Neutron-Star Mergers
• Proto-neutron stars with heavy baryons and universal relations
• Finite-temperature extension for cold neutron star equations of state
• Future Physics Perspectives on the Equation of State from Heavy Ion Collisions to Neutron Stars
• The slope, the hill, the drop, and the swoosh: Learning about the nuclear matter equation of state from the binary Love relations
• Equations of state for hot neutron stars -- II. The role of exotic particle degrees of freedom
• EoS for hot neutron stars
• High-Energy Phase Diagrams with Charge and Isospin Axes under Heavy-Ion Collision and Stellar Conditions
• Efficient Learning of Accurate Surrogates for Simulations of Complex Systems
• Radial and Non-Radial Oscillations of Inverted Hybrid Stars
• How Macroscopic Limits on Neutron Star Baryon Loss Yield Microscopic Limits on Non-Standard-Model Baryon Decay
• Transport coefficients of magnetized neutron star cores
• Multimessenger signal from phase transition of neutron star to quark star
• The impact of hyperons on neutron star mergers: gravitational waves, mass ejection and black hole formation
• Projecting the likely importance of weak-interaction-driven bulk viscosity in neutron star mergers
• Tracing the Trace Anomaly of Dense Matter inside Neutron Stars