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 |
|---|---|---|---|
| Web Page | HTML | catalog.html | Open resource |
| Web Page | HTML | catalog.html | Open resource |