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

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

V. Dexheimer
(
- Kent State U.
)

Aug 28, 2017

6 pages

Published in:

Publ.Astron.Soc.Austral. 34 (2017) E006

e-Print:

1708.08342 [astro-ph.HE]

DOI:

10.1017/pasa.2017.61 (publication)

View in:

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Abstract: (arXiv)

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.

Note:

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

tabulated equation of state
neutron star
chiral symmetry
hyperon
quark deconfinement
mean field approximation: chiral
star: compact
neutron star
equation of state
supernova: collapse

References(46)

Figures(0)

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