Solution sequences of close binary neutron star systems

Details Solution sequences of close binary neutron star systems Solution sequences of close binary neutron star systems

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.466u&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

We have succeeded in developing a new numerical method to calculate irrotational binary systems composed of compressible gaseous stars in Newtonian gravity. Such irrotational configurations of binary systems are appropriate models for realistic neutron star binaries composed of inviscid gases, just prior to coalescence of two stars caused by emission of gravitational waves. Our numerical solutions are so accurate that we can compute reliable models for fully deformed final stationary configurations. This method is also applicable to the general relativistic case.

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