Three-dimensional adaptive evolution of gravitational waves in numerical relativity

Adaptive techniques are crucial for successful numerical modeling of gravitational waves from astrophysical sources such as coalescing compact binaries, since the radiation typically has wavelengths much larger than the scale of the sources. We have carried out an important step toward this goal: th...

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Veröffentlicht in:	Physical review. D, Particles and fields Particles and fields, 2000-10, Vol.62 (8), Article 084039
Hauptverfasser:	New, Kimberly C. B., Choi, Dae-Il, Centrella, Joan M., MacNeice, Peter, Huq, Mijan F., Olson, Kevin
Format:	Artikel
Sprache:	eng
Schlagworte:	CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS GRAVITATIONAL WAVES RADIATIONS RESOLUTION SIMULATION WAVELENGTHS
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