Characteristic Evolution and Matching
Author:
Publisher
Springer Science and Business Media LLC
Subject
Physics and Astronomy (miscellaneous)
Link
http://link.springer.com/content/pdf/10.12942/lrr-2012-2
Reference312 articles.
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2. Abrahams, A.M. and Price, R.H., “Applying black hole perturbation theory to numerically generated spacetimes”, Phys. Rev. D, 53, 1963–1971, (1996). [DOI], [ADS], [arXiv:gr-qc/9508059]. (Cited on pages 7 and 58.)
3. Abrahams, A.M., Shapiro, S.L. and Teukolsky, S.A., “Calculation of gravitational waveforms from black hole collisions and disk collapse: Applying perturbation theory to numerical spacetimes”, Phys. Rev. D, 51, 4295–4301, (1995). [DOI], [ADS], [arXiv:gr-qc/9408036]. (Cited on pages 7 and 58.)
4. Abrahams, A.M. et al. (Binary Black Hole Grand Challenge Alliance), “Gravitational Wave Extraction and Outer Boundary Conditions by Perturbative Matching”, Phys. Rev. Lett., 80, 1812–1815, (1998). [DOI], [ADS], [arXiv:gr-qc/9709082]. (Cited on pages 7 and 58.)
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