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• Organization: National Aeronautics and Space Administration
• Updated: 2025-07-17 | Harvested: October 25, 2025 at 09:33 PM

Numerically-generated gravitational waveforms for circular inspiral into Kerr black holes. These waveforms were developed using Scott Hughes' black hole perturbation theory code (the "Teukolsky code").

• Organization: National Aeronautics and Space Administration
• Updated: 2025-03-31 | Harvested: October 19, 2025 at 07:14 PM

Numerically-generated gravitational waveforms for binary neutron stars.

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• Organization: National Aeronautics and Space Administration
• Updated: 2025-03-31 | Harvested: June 28, 2025 at 11:21 AM

Numerically-generated gravitational waveforms for binary black holes.

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• Organization: National Aeronautics and Space Administration
• Updated: 2025-03-31 | Harvested: August 30, 2025 at 12:11 AM

Numerically-generated gravitational waveforms for circular inspiral into Kerr black holes. These waveforms were developed using Scott Hughes' black hole perturbation theory code (the 'Teukolsky code').

• html

• Organization: National Aeronautics and Space Administration
• Updated: 2025-03-31 | Harvested: June 28, 2025 at 01:51 PM

Gravitational radiation waveforms for black hole-neutron star coalescence calculations. The physical input is Newtonian physics, an ideal gas equation of state with varying compressibility...

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