Physics
Scientific paper
May 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990stin...9029269w&link_type=abstract
Presented at the International Conference on Medium- and High-Energy Physics, Taipei, Taiwan, 14-18 May 1990
Physics
Equations Of State, Hartree Approximation, Neutron Stars, Relativity, Stellar Rotation, Matter (Physics), S Matrix Theory
Scientific paper
The properties of non-rotating as well as rotating neutron stars are investigated in the framework of Einstein's theory of general relativity. The nuclear equation of state of neutron star matter (electrically charge neutral many-baryon/lepton system) is calculated for the relativistic Hartree- and Hartree-Fock approximations. The influence of two-particle correlations on the equation of state is taken into account, too. An important result is that the limiting rotational frequency of a neutron star is set by instability modes caused by gravitational radiation reaction, which set in well below the Kerplerian frequency.
Glendenning Norman K.
Weber Fridolin
Weigel Manfred K.
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