Black Hole - Neutron Star Binary Mergers

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 (through the index gamma), and point-mass gravitational radiation back reaction, which is switched off in the simulation once the star is tidally disrupted. All the simulations are 3D, done using SPH.

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Additional Info

Field	Value
Maintainer	William Henry Lee
Last Updated	March 31, 2025, 18:48 (UTC)
Created	March 31, 2025, 18:48 (UTC)
accessLevel	public
accrualPeriodicity	irregular
bureauCode	{026:00}
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catalog_@id	https://data.nasa.gov/data.json
catalog_conformsTo	https://project-open-data.cio.gov/v1.1/schema
catalog_describedBy	https://project-open-data.cio.gov/v1.1/schema/catalog.json
describedBy	http://astrogravs.gsfc.nasa.gov/docs/waveforms/LEE/README
harvest_object_id	b034d187-ac97-4a49-b6aa-61feda33a604
harvest_source_id	61638e72-b36c-4866-9d28-551a3062f158
harvest_source_title	DNG Legacy Data
identifier	NASA-0000023
issued	2018-06-25
landingPage	https://asd.gsfc.nasa.gov/archive/astrogravs/docs/catalog.html#bhns
modified	2024-08-16
programCode	{026:016}
publisher	National Aeronautics and Space Administration
resource-type	Dataset
source_datajson_identifier	true
source_hash	d106deb3c63f7e60e6f9ef32f4ad50fc42ff7b354323f4e79feb5d7d99254a58
source_schema_version	1.1
temporal	2000-01-01/2014-01-01