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    Macroscopic properties of neutron stars including deformation

    Zdeněk Stuchlík · 01 února, 2012 · Fyzika · 0 comments
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    Publication date: Feb 2012

    Abstract:
    We used the equations of state 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. We calculated the central pressure and density and
    correspondingly the possible radius and mass both with and without
    allowance for hyperons first, and compared these results with recent
    astronomical observations, and, finally, we included effect of
    deformation and rotation.

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

    http://adsabs.harvard.edu/abs/2012JPhCS.337a2021U

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