| Autor: |
Deirdre Shoemaker, K. Camarda, Stuart L. Shapiro, W. Landry, Steven R. Brandt, M. F. Huq, Bela Szilagyi, Edward Seidel, Manish Parashar, Siddhartha Mitra, M. H. P. M. van Putten, Pablo Laguna, Luciano Rezzolla, Arlen Anderson, Scott Klasky, James W. York, Saul A. Teukolsky, Jeffrey Winicour, J. Lenaghan, Peter Anninos, Richard A. Matzner, M. E. Rupright, Randall R. Correll, Geoffrey C. Fox, Philippos Papadopoulos, Charles R. Evans, Joan Masso, F. Saied, Luis Lehner, R. L. Marsa, Gregory B. Cook, Andrew M. Abrahams, Mark A. Scheel, Larry Smarr, Nigel T. Bishop, Larry Kidder, Roberto Gomez, Tomasz Haupt, Lee Samuel Finn, P. E. Saylor, James C. Browne, P. Walker, Matthew W. Choptuik, Thomas W. Baumgarte |
| Předmět: |
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| Zdroj: |
Scopus-Elsevier |
| Popis: |
We present a method for extracting gravitational radiation from a three-dimensional numerical relativity simulation and, using the extracted data, to provide outer boundary conditions. The method treats dynamical gravitational variables as nonspherical perturbations of Schwarzschild geometry. We discuss a code which implements this method and present results of tests which have been performed with a three dimensional numerical relativity code. |
| Databáze: |
OpenAIRE |
| Externí odkaz: |
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