The Σ Well Depth and the Proto Neutron Star Matter View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

2013-02

AUTHORS

Xian-Feng Zhao, Li Zhang

ABSTRACT

The effect of the Σ well depth on a proto neutron star (PNS) is examined within the framework of relativistic mean field theory for the baryon octet system. It is found that the well depth will affect the structures of the PNS. With the well depth growing from 0 to 30 MeV, the field strength of meson ρ, the chemical potentials of electrons and neutrons, the relative number density of p, e, μ, Λ, Ξ0, the mass and the pressure of a PNS all increase while the relative number density of n, Ξ−, Σ−, Σ0, Σ+ decrease. It is also found that the larger changes of the hyperon coupling constants, which is connected to the Σ well depth , will lead to the smaller changes in the neutron star mass and this shows the mass of PNS is not very sensitive to the hyperon coupling constants. More... »

PAGES

429-440

References to SciGraph publications

  • 2010-08. Kaon properties in (proto-)neutron star matter in THE EUROPEAN PHYSICAL JOURNAL A
  • Identifiers

    URI

    http://scigraph.springernature.com/pub.10.1007/s10773-012-1349-6

    DOI

    http://dx.doi.org/10.1007/s10773-012-1349-6

    DIMENSIONS

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