How far away is far enough for extracting numerical waveforms, and how much do they depend on the extraction method?
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Publication:5293868
DOI10.1088/0264-9381/24/12/S22zbMath1117.83036arXivgr-qc/0612149WikidataQ59830063 ScholiaQ59830063MaRDI QIDQ5293868
Enrique Pazos, Alessandro Nagar, Manuel Tiglio, Ernst Nils Dorband, Erik Schnetter, Carlos Palenzuela
Publication date: 4 July 2007
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/gr-qc/0612149
Computational methods for problems pertaining to relativity and gravitational theory (83-08) Gravitational waves (83C35)
Related Items (4)
Extraction of gravitational waves in numerical relativity ⋮ Quasinormal modes from Penrose limits ⋮ Characteristic evolution and matching ⋮ Continuum and discrete initial-boundary value problems and Einstein's field equations
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