Disks around merging binary black holes: From GW150914 to supermassive black holes
We perform magnetohydrodynamic simulations in full general relativity of disk accretion onto nonspinning black hole binaries with mass ratio q = 29/36. We survey different disk models which differ in their scale height, total size and magnetic field to quantify the robustness of previous simulations...
| Main Authors: | , , , |
|---|---|
| Other Authors: | |
| Language: | en |
| Published: |
AMER PHYSICAL SOC
2018
|
| Online Access: | http://hdl.handle.net/10150/627161 http://arizona.openrepository.com/arizona/handle/10150/627161 |