High-accuracy waveforms for black hole-neutron star systems with spinning black holes
The availability of accurate numerical waveforms is an important requirement for the creation and calibration of reliable waveform models for gravitational wave astrophysics. For black hole-neutron star binaries (BHNS), very few accurate waveforms are however publicly available. Most recent models a...
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Veröffentlicht in: | Physical review. D 2021-03, Vol.103 (6), Article 064007 |
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Hauptverfasser: | , , , , , , , , , , , , |
Format: | Artikel |
Sprache: | eng |
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