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astroparticle physics – dense matter – equation of state – stars: neutron

Publications of the Astronomical Society of Australia (1)

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Tabulated Neutron Star Equations of State Modelled within the Chiral Mean Field Model
V. Dexheimer
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Publications of the Astronomical Society of Australia / Volume 34 / 2017

Published online by Cambridge University Press:

06 December 2017, e066
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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.