Black Hole - Neutron Star Binary Mergers

Metadata Updated: July 8, 2015

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.

Access & Use Information

Public: This dataset is intended for public access and use. License: U.S. Government Work

Downloads & Resources


Metadata Created Date October 8, 2014
Metadata Updated Date July 8, 2015
Data Update Frequency irregular

Metadata Source

Harvested from NASA Data.json

Additional Metadata

Resource Type Dataset
Metadata Created Date October 8, 2014
Metadata Updated Date July 8, 2015
Publisher National Aeronautics and Space Administration
Unique Identifier NASA-0000023
William Henry Lee
Maintainer Email
Id {$oid: 55942a78c63a7fe59b4974aa}
Public Access Level public
Data Update Frequency irregular
Bureau Code 026:00
Metadata Context
Schema Version
Catalog Describedby
Data Dictionary
Harvest Object Id 158ab895-f87f-4d8e-b869-ea0979613c1d
Harvest Source Id 39e4ad2a-47ca-4507-8258-852babd0fd99
Harvest Source Title NASA Data.json
Homepage URL
Language en-US
Data Last Modified 2014-05-01
Program Code 026:000
Source Datajson Identifier True
Source Hash 6807ef521d760670c5f41118cda226954379d513
Source Schema Version 1.1
Temporal 2000-01-01/2014-01-01

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