Quasi-Equilibrium Structures of General Relativistic Binary Neutron Star Systems -- a New Approach Without the Conformally Flat Condition

Details Quasi-Equilibrium Structures of General Relativistic Binary Neutron Star Systems -- a New Approach Without the Conformally Flat Condition Quasi-Equilibrium Structures of General Relativistic Binary Neutron Star Systems -- a New Approach Without the Conformally Flat Condition

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002nmgm.meet.2303u&link_type=abstract

"THE NINTH MARCEL GROSSMANN MEETING On Recent Developments in Theoretical and Experimental General Relativity, Gravitation and R

Physics

Scientific paper

One of the most important problems for theorists of relativistic astrophysics is constructing reliable models for quasiequilibrium configurations of binary neutron star systems. This is because such systems are the most promising sources of gravitational waves (GW) which can be observed by the GW detectors under construction all over the world...

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