BH-NS Simulations via characteristic evolutions

Details BH-NS Simulations via characteristic evolutions BH-NS Simulations via characteristic evolutions

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aps..aprq20006l&link_type=abstract

American Physical Society, April Meeting, April 29-May 2, 2000 Long Beach, CA, abstract #Q20.006

Astronomy and Astrophysics

Astrophysics

Scientific paper

The characteristic formulation of the Einstein equations provides a rather unique tool for numerical relativity. It has been used recently to good effect in three dimensional evolutions of vacuum black hole using the concept of excision. In conjunction with hydrodynamical evolution one would hope to tackle a range of interesting astrophysical problems involving dynamic black holes. I will describe a collaborative work aimed in this direction.

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