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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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Complete Metadata
| @type | dcat:Dataset |
|---|---|
| accessLevel | public |
| accrualPeriodicity | irregular |
| bureauCode |
[
"026:00"
]
|
| contactPoint |
{
"fn": "William Henry Lee",
"@type": "vcard:Contact",
"hasEmail": "mailto:wlee@astroscu.unam.mx"
}
|
| describedBy | http://astrogravs.gsfc.nasa.gov/docs/waveforms/LEE/README |
| description | 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. |
| distribution |
[
{
"@type": "dcat:Distribution",
"format": "HTML",
"mediaType": "text/html",
"downloadURL": "https://asd.gsfc.nasa.gov/archive/astrogravs/docs/catalog.html#bhns"
}
]
|
| identifier | NASA-0000023 |
| issued | 2018-06-25 |
| keyword |
[
"astronomy",
"binary",
"black-hole",
"gravitational-waves",
"ligo",
"neutron-stars",
"space-science"
]
|
| landingPage | https://asd.gsfc.nasa.gov/archive/astrogravs/docs/catalog.html#bhns |
| modified | 2025-03-31 |
| programCode |
[
"026:016"
]
|
| publisher |
{
"name": "National Aeronautics and Space Administration",
"@type": "org:Organization"
}
|
| temporal | 2000-01-01/2014-01-01 |
| title | Black Hole - Neutron Star Binary Mergers |
