A different way to evolve black hole-neutron star binaries

Details A different way to evolve black hole-neutron star binaries A different way to evolve black hole-neutron star binaries

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aps..aprh10003d&link_type=abstract

American Physical Society, 2008 APS April Meeting and HEDP/HEDLA Meeting, April 11-15, 2008, abstract #H10.003

Physics

Scientific paper

We give a status report on our simulations of comparable mass black hole-neutron star binaries. We evolve the full Einstein equations for the spacetime metric using multidomain pseudospectral methods, and we evolve the hydrodynamic variables using finite volume methods on a separate grid. Our two-grid approach allows us to model the inspiral with particular accuracy.

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