Published March 23, 1998
| Submitted + Published
Journal Article
Open
Boosted Three-Dimensional Black-Hole Evolutions with Singularity Excision
- Creators
- Cook, G. B.
- Huq, M. F.
- Klasky, S. A.
-
Scheel, M. A.
- Abrahams, A. M.
- Anderson, A.
- Anninos, P.
- Baumgarte, T. W.
- Bishop, N. T.
- Brandt, S. R.
- Browne, J. C.
- Camarda, K.
- Choptuik, M. W.
- Correll, R. R.
- Evans, C. R.
- Finn, L. S.
- Fox, G. C.
- Gómez, R.
- Haupt, T.
-
Kidder, L. E.
- Laguna, P.
- Landry, W.
- Lehner, L.
- Lenaghan, J.
- Marsa, R. L.
- Masso, J.
- Matzner, R. A.
- Mitra, S.
- Papadopoulos, P.
- Parashar, M.
- Rezzolla, L.
- Rupright, M. E.
- Saied, F.
- Saylor, P. E.
- Seidel, E.
-
Shapiro, S. L.
- Shoemaker, D.
- Smarr, L.
- Suen, W. M.
- Szilágyi, B.
-
Teukolsky, S. A.
- van Putten, M. H. P. M.
- Walker, P.
- Winicour, J.
- York, J. W., Jr.
- Binary Black Hole Grand Challenge Alliance
Chicago
Abstract
Binary black-hole interactions provide potentially the strongest source of gravitational radiation for detectors currently under development. We present some results from the Binary Black Hole Grand Challenge Alliance three-dimensional Cauchy evolution module. These constitute essential steps towards modeling such interactions and predicting gravitational radiation waveforms. We report on single black-hole evolutions and the first successful demonstration of a black hole moving freely through a three-dimensional computational grid via a Cauchy evolution: a hole moving near 6M at 0.1c during a total evolution of duration near 60M.
Additional Information
© 1998 The American Physical Society. Received 26 November 1997. This work was supported by the NSF Binary Black Hole Grand Challenge Grants No. NSF PHY/ASC 93-18152 (ARPA supplemented), No. NSF PHY 93-10083, and Metacenter Grant No. MCA94P015N. Computations were performed at NPAC (Syracuse University), at NCSA (University of Illinois at Urbana-Champaign), and at the Pittsburgh Supercomputing Center.Attached Files
Published - PhysRevLett.80.2512.pdf
Submitted - 9711078.pdf
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Additional details
- Eprint ID
- 99177
- Resolver ID
- CaltechAUTHORS:20191009-084004889
- NSF
- PHY/ASC 93-18152
- NSF
- PHY 93-10083
- Metacenter
- MCA94P015N
- Created
-
2019-10-09Created from EPrint's datestamp field
- Updated
-
2021-11-16Created from EPrint's last_modified field