Tidal effects on event horizon of binary rotating BHs

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Christian Thom
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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 ?
 
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  • #2
Christian Thom said:
internal material of the BH
There is no such thing. A BH is vacuum.

Christian Thom said:
Or is these too Newtonian speculations ?
Basically, yes. A black hole is not an ordinary object, and the horizon is not an ordinary surface.

There are no known exact solutions for a massive object near a BH, either orbiting or falling in, so cases like this have to be studied numerically. However, heuristically I think the following is a reasonable description:

(1) If the massive object is orbiting, it has to be orbiting far enough from the hole that effects on the hole's horizon are negligible.

(2) If the massive object is falling in, the horizon grows, it doesn't shrink, so any intuitions based on the massive object "pulling" against the pull of the hole obviously don't apply.
 
  • #3
Thank you for your reply.
I nevertheless would not be so positive about the vacuity of the BH. It is true that the Schwarzchild are only valid for vacuum space, but that doesn't mean that the actual BH are of this kind.
As for the tidal waves, we have a some evidence for them : gravitational waves that have been detected during fusion events.
 
  • #4
I am having a hard time distinguishing your response from "I am not going to do the calculation myself, but I think you're just wrong" or possibly "maybe GR is just wrong in some unspecified way".

If this isn't where you are coming from, it would be helpful if you would clarify. Ideally with calculations.
 
  • #5
Christian Thom said:
I nevertheless would not be so positive about the vacuity of the BH.
You should be. While it is true that actual BHs are formed by the collapse of massive objects, so there will be a portion of the spacetime inside the horizon that is not vacuum, it is clear both from exact solutions like the Oppenheimer-Snyder model and numerical simulations that the non-vacuum portion of the interior plays no significant role once the hole is formed. So treating actual BHs as vacuum is still the best model.

Christian Thom said:
It is true that the Schwarzchild are only valid for vacuum space, but that doesn't mean that the actual BH are of this kind.
As far as anything we can detect from the outside is concerned, actual BH will be described, except for the portion of the spacetime occupied by the collapsing matter (which, as above, plays no significant role once the hole is formed) by a solution in the Kerr-Newman family of solutions, which are vacuum. This has been a known theorem since, IIRC, the late 1960s.

Christian Thom said:
As for the tidal waves, we have a some evidence for them : gravitational waves that have been detected during fusion events.
We have detected gravitational waves from mergers, yes. But these are nothing like what you describe in your OP.
 
  • #6
Christian Thom said:
but that doesn't mean that the actual BH are of this kind.
Semi-realistic models of stellar collapse such as Oppenheimer-Snyder have an interior that is mostly vacuum. There are no models I'm aware of where there's matter hanging around just inside the event horizon, anyway. Certainly not in vanilla GR.
Christian Thom said:
As for the tidal waves, we have a some evidence for them : gravitational waves that have been detected during fusion events.
Yes, and they match GR predictions to the best precision available - so we are talking of event horizons that reach towards each other and cannot reveal anything that's crossed them.
 
  • #7
Thank you all. I surrender !
 

FAQ: Tidal effects on event horizon of binary rotating BHs

What are tidal effects in the context of binary rotating black holes?

Tidal effects refer to the gravitational interactions between two massive objects, such as black holes, which can distort their shapes and influence their dynamics. In the context of binary rotating black holes, these effects can lead to complex gravitational wave patterns and changes in the event horizons of the black holes.

How do tidal forces affect the event horizon of a rotating black hole in a binary system?

Tidal forces can distort the event horizon of a rotating black hole in a binary system by stretching and compressing it due to the gravitational pull from the companion black hole. This can lead to the event horizon becoming elongated or deformed, especially as the black holes approach each other.

Can tidal interactions in binary black hole systems lead to observable gravitational waves?

Yes, tidal interactions in binary black hole systems can lead to the emission of gravitational waves. These waves carry information about the masses, spins, and orbital dynamics of the black holes, including the effects of tidal distortions. Advanced detectors like LIGO and Virgo can observe these waves, providing insights into the nature of such systems.

Do tidal effects influence the merger process of binary rotating black holes?

Tidal effects play a significant role in the merger process of binary rotating black holes. As the black holes spiral closer, tidal forces can transfer angular momentum and energy between them, affecting their orbital evolution and the final merger dynamics. These interactions can also impact the final spin and mass of the resulting black hole.

What role does the spin of black holes play in tidal interactions within a binary system?

The spin of black holes significantly influences tidal interactions within a binary system. Rotating black holes, or Kerr black holes, have more complex gravitational fields compared to non-rotating ones. The interaction between their spins and the orbital motion can lead to phenomena such as frame-dragging, which further complicates the tidal effects and can alter the gravitational wave signals emitted during their inspiral and merger.

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