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    Influence of strange matter admixtures on macroscopic properties of neutron stars

    Zdeněk Stuchlík · 01 října, 2011 · Fyzika · 0 comments
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    Publication date: Oct 2011

    Abstract:
    We used the equations of state (EoS) of dense nuclear matter to
    construct the macroscopic properties of neutron stars and test them
    using available observational results. The Dirac-Brueckner-Hartree-Fock
    mean field calculations approximated by their parameterized form are the
    basis of our calculations for the star interior. We calculated the
    central pressure, density, radius and mass both without and with
    allowance for hyperons, and compared these results with astronomical
    observations.

    Authors:
    Urbanec, M.; Běták, E.; Stuchlík, Z.;

    http://adsabs.harvard.edu/abs/2011AIPC.1377..275U

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