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.
Complete Metadata
| bureauCode |
[ "026:00" ] |
|---|---|
| describedBy | http://astrogravs.gsfc.nasa.gov/docs/waveforms/LEE/README |
| identifier | NASA-0000023 |
| issued | 2018-06-25 |
| landingPage | https://asd.gsfc.nasa.gov/archive/astrogravs/docs/catalog.html#bhns |
| programCode |
[ "026:016" ] |
| temporal | 2000-01-01/2014-01-01 |
