- #1
Christian Thom
- 38
- 6
- TL;DR Summary
- The presence of a big mass in the vicinity of a BH must have an effect on the shape of the event horizon. When the system is rotating, it would lead to tidal effects on the horizon that would disclose internal material of the BH.
The presence of a big mass (BH or neutron star) in the vicinity of a BH must have an effect on the shape of the event horizon, an indentation comes logically to mind. When the system is rotating, it would lead to tidal effects on the horizon that would disclose internal material of the BH. This would even allow some of it to possibly escape to free space or to fall in the second massive body. This maybe would also, on the contrary, ease the capture of the content of an potential accretion disk. Or is these too Newtonian speculations ?