Published December 15, 2002
| Version Published + Submitted
Journal Article
Open
Toward stable 3D numerical evolutions of black-hole spacetimes
Creators
-
1.
California Institute of Technology
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2.
Cornell University
Abstract
Three dimensional (3D) numerical evolutions of static black holes with excision are presented. These evolutions extend to about 8000M, where M is the mass of the black hole. This degree of stability is achieved by using growth-rate estimates to guide the fine tuning of the parameters in a multiparameter family of symmetric hyperbolic representations of the Einstein evolution equations. These evolutions were performed using a fixed gauge in order to separate the intrinsic stability of the evolution equations from the effects of stability-enhancing gauge choices.
Additional Information
© 2002 The American Physical Society. Received 30 September 2002; published 17 December 2002. Some computations were performed on the IA-32 Linux cluster at NCSA. This research was supported in part by NSF grant PHY-0099568 and NASA grant NAG5-10707 at California Institute of Technology and NSF grants PHY-9800737 and PHY-9900672 at Cornell University.Attached Files
Published - SCHEprd02.pdf
Submitted - 0209115.pdf
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0209115.pdf
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Additional details
Identifiers
- Eprint ID
- 3017
- Resolver ID
- CaltechAUTHORS:SCHEprd02
Related works
- Describes
- https://arxiv.org/abs/gr-qc/0209115 (URL)
Funding
- NSF
- PHY-0099568
- NASA
- NAG5-10707
- NSF
- PHY-9800737
- NSF
- PHY-9900672
Dates
- Created
-
2006-05-11Created from EPrint's datestamp field
- Updated
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2021-11-08Created from EPrint's last_modified field