Black Hole - Neutron Star Binary Mergers
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.
Resources
| Name |
Format |
Description |
Link |
|
21 |
catalog.html |
http://astrogravs.gsfc.nasa.gov/docs/catalog.html#bhns |
|
21 |
catalog.html |
https://asd.gsfc.nasa.gov/archive/astrogravs/docs/catalog.html#bhns |
Tags
- astronomy
- gravitational-waves
- neutron-stars
- binary
- black-hole
- ligo
- space-science