Moments of inertia of neutron stars in relativistic mean field theory: The role of the isovector scalar channel

With the inclusion of the isovector scalar channel in the meson-nucleon couplings, taking DD-ME δ as an effective interaction, the moments of inertia of neutron stars possessing various stellar masses are studied within the density dependent relativistic mean field (RMF) theory. The isovector scalar...

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Veröffentlicht in:	Science China. Physics, mechanics & astronomy mechanics & astronomy, 2018-08, Vol.61 (8), p.082011, Article 082011
Hauptverfasser:	Qian, Zhuang, Xin, RuoYu, Sun, BaoYuan
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Classical and Continuum Physics Couplings Equations of state Inertia Mean field theory Moments of inertia Neutron stars Neutrons Nucleons Observations and Techniques Physics Physics and Astronomy Pulsars Relativistic effects Relativistic theory Stars
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