Properties of Rotating Neutron Stars Using Density Dependent Relativistic Hadron Field Theory

Details Properties of Rotating Neutron Stars Using Density Dependent Relativistic Hadron Field Theory Properties of Rotating Neutron Stars Using Density Dependent Relativistic Hadron Field Theory

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aas...209.9103r&link_type=abstract

2007 AAS/AAPT Joint Meeting, American Astronomical Society Meeting 209, #91.03; Bulletin of the American Astronomical Society, V

Astronomy and Astrophysics

Astronomy

Scientific paper

We present properties of rotating, fully relativistic neutron stars for equations of state computed in the framework of the density dependent relativistic Brueckner-Hartree-Fock hadron field theory. Particular emphasis is put on the hyperon composition of neutron stars, which changes dramatically with rotational frequency. This may have important consequences for rotational instability modes in rapidly spinning neutron stars, as will be pointed out.

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