Post-Newtonian SPH simulations of binary neutron stars

Details Post-Newtonian SPH simulations of binary neutron stars Post-Newtonian SPH simulations of binary neutron stars

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..586..775f&link_type=abstract

RELATIVISTIC ASTROPHYSICS: 20th Texas Symposium. AIP Conference Proceedings, Volume 586, pp. 775-780 (2001).

Astronomy and Astrophysics

Astrophysics

Neutron Stars, Binary And Multiple Stars, Hydrodynamics, Mathematical Procedures And Computer Techniques, Flow Instabilities, Post-Newtonian Approximation, Perturbation Theory, Related Approximations

Scientific paper

Using our Post-Newtonian SPH (smoothed particle hydrodynamics) code, we
study the final coalescence and merging of neutron star (NS) binaries.
We find that the gravity wave signals can be computed accurately for
irrotational systems in calculations of sufficient resolution, even in
the presence of Kelvin-Helmholtz instabilities. .

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