EQUATION OF STATE FOR MASSIVE NEUTRON STARS

Using the relativistic Hartree-Fock approximation, we investigate the properties of neutron-star matter in detail. In the present calculation, we consider not only the tensor coupling of vector mesons to octet baryons and the form factors at interaction vertices but also the change in the internal (...

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Veröffentlicht in:The Astrophysical journal. Supplement series 2012-12, Vol.203 (2), p.1-14
Hauptverfasser: Katayama, Tetsuya, MIYATSU, TSUYOSHI, Saito, Koichi
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Sprache:eng
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