Polytrope-Black Hole simulations in full GR

Details Polytrope-Black Hole simulations in full GR Polytrope-Black Hole simulations in full GR

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aps..apre12001l&link_type=abstract

American Physical Society, April Meeting, Jointly Sponsored with the High Energy Astrophysics Division (HEAD) of the American As

Astronomy and Astrophysics

Astrophysics

Scientific paper

The characteristic formulation of GR has succesfully been used by us to evolve single black hole spacetimes stably. We here extend this implementation to handle non-vacuum spacetimes targeting one containing a black hole and a polytrope. Preliminar results will be shown and the challenges faced for an accurate simulation under this formulation discussed.

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