Tabulated Neutron Star Equations of State Modelled 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.
- Publication:
-
Publications of the Astronomical Society of Australia
- Pub Date:
- December 2017
- DOI:
- 10.1017/pasa.2017.61
- arXiv:
- arXiv:1708.08342
- Bibcode:
- 2017PASA...34...66D
- Keywords:
-
- astroparticle physics;
- dense matter;
- equation of state;
- stars: neutron;
- Astrophysics - High Energy Astrophysical Phenomena;
- Astrophysics - Solar and Stellar Astrophysics;
- Nuclear Theory
- E-Print:
- PASA special issue on the Neutron Stars, related to the Compstar conference in Warsaw