Web site of EOS for Neutron Star Matter
--- CQMC model within relativistic Hartree-Fock approximation and Thomas-Fermi model ---

Abstract

This web site provides equation of state (EOS) for neutron star matter. The chiral quark-meson coupling (CQMC) model within relativistic Hartree-Fock approximation is adopted for uniform nuclear matter. All octet baryons are considered in the core region, while only Ξ- appears in neutron stars. In the crust region, nuclei are taken into account within the Thomas-Fermi calculation. For the details, see Miyatsu et al. (2013), Astrophys. J. 777 (2013) 4, arXiv:1308.6121 [astro-ph.HE]. This EOS table is open for general use in any numerical simulations for astrophysics, provided that our paper is referenced in your publication.

User's Guide (read me first)


EOS tables


Key parameters

Note: There are two diffinitions of symmetry energy. See Section 3.2 and Table 2 of our paper for the details.

Contact


Reference

Please reference the following paper when you publish scientific articles using this EOS.


Last up date, May 14, 2016.