Moving black holes via singularity excision (original) (raw)

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Abstract

We present a singularity excision algorithm appropriate for numerical simulations of black holes moving throughout the computational domain. The method is an extension of the excision procedure previously used to obtain stable simulations of single, non-moving black holes. The excision procedure also shares elements used in recent work to study the dynamics of a scalar field in the background of a single, boosted black hole. The excision method is tested with single black-hole evolutions using a coordinate system in which the coordinate location of the black hole, and thus the excision boundary, moves throughout the computational domain.

Publication:

Classical and Quantum Gravity

Pub Date:

August 2003

DOI:

10.1088/0264-9381/20/16/313

10.48550/arXiv.gr-qc/0301111

arXiv:

arXiv:gr-qc/0301111

Bibcode:

2003CQGra..20.3729S

Keywords:

E-Print:

9 pages and 11 figures