Physics
Scientific paper
Oct 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..586..796c&link_type=abstract
RELATIVISTIC ASTROPHYSICS: 20th Texas Symposium. AIP Conference Proceedings, Volume 586, pp. 796-798 (2001).
Physics
Neutron Stars, Binary And Multiple Stars, Post-Newtonian Approximation, Perturbation Theory, Related Approximations, Relativistic Stars: Structure, Stability, And Oscillations, Physics Of Black Holes, Black Holes
Scientific paper
We present numerical studies of coalescing neutron star pairs with Newtonian hydrodynamics coupled to the 2.5 Post-Newtonian radiation reaction of Blanchet, Damour, and Schäfer [1]. Our simulations evolve the Euler equations using a modification of the ZEUS 2-D algorithm [2] and use a Fast Fourier Transformation method for solving the Poisson equation for the gravitational and radiation reaction potentials. We find that the radiation reaction produces a significant effect on a neutron star pair when compared to a purely Newtonian simulation. .
Calder Alan C.
Swesty Frank Douglas
Wang Edward Yung Ming
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