Merger of Binary Neutron Stars in Fully General Relativistic Simulation

Details Merger of Binary Neutron Stars in Fully General Relativistic Simulation Merger of Binary Neutron Stars in Fully General Relativistic Simulation

Sep 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002grg..conf..294s&link_type=abstract

GENERAL RELATIVITY AND GRAVITATION. Proceedings of the 16th International Conference. Held 15-21 July 2001 in Durban, South Afri

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We review recent progress in the numerical study on the last phase of coalescing binary neutron stars in the general relativistic framework. First, current status for computation of quasiequilibrium states for binary neutron stars in close circular orbits is reviewed. Then, current status of numerical simulation for binary neutron star merger is summarized. Some numerical results recently computed are also presented.

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