How Can We Observe Black Holes Growing?

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Discussion Overview

The discussion revolves around the observation of black holes and their growth, particularly focusing on the dynamics of matter falling into black holes and the perspectives of different observers. It touches on theoretical aspects of general relativity, the behavior of particles with varying angular momentum, and the implications of Schwarzschild coordinates.

Discussion Character

  • Debate/contested
  • Technical explanation
  • Conceptual clarification

Main Points Raised

  • Some participants assert that from a distant observer's perspective, it appears that matter takes an infinite amount of time to fall into a black hole, raising questions about how black holes can absorb matter.
  • Others argue that matter can fall into a black hole if it loses angular momentum, typically through processes in an accretion disk.
  • One participant claims that particles with zero angular momentum fall into the black hole in finite time according to their own clocks, challenging the notion that they take infinite time from a distant perspective.
  • There is a discussion about the misconceptions surrounding the role of distant observers and the nature of events in curved spacetime, with some participants emphasizing that just because an event is not observed does not mean it does not occur.
  • Participants discuss the concept of "when" in the context of crossing the event horizon, noting that there is no unique time that can be universally applied across different reference frames.
  • Some participants express frustration over perceived misunderstandings and emphasize the importance of clarity in discussing these concepts.

Areas of Agreement / Disagreement

There is no consensus in the discussion, as multiple competing views remain regarding the nature of black hole absorption, the role of observers, and the implications of general relativity on time and events.

Contextual Notes

Participants highlight limitations in understanding due to the complexities of general relativity, particularly regarding the definitions of time and the behavior of objects in curved spacetime. There are unresolved mathematical steps and assumptions that influence the discussion.

  • #91
Can one observe expansion of the EH even if one cannot ever get a light signal from whatever fell in confirming that it fell in?
 
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  • #92
Grinkle said:
Can one observe expansion of the EH even if one cannot ever get a light signal from whatever fell in confirming that it fell in?
In a sense, yes. There are computer generated images of what you would see against background stars as a neutron star or small BH merges with a bigger one, resulting in a single larger BH visible against background stars. However none of what see comes from at or inside a horizon.
 
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  • #93
Grinkle said:
Can one observe expansion of the EH even if one cannot ever get a light signal from whatever fell in confirming that it fell in?
Depends what you mean by "observe". You could measure a black hole's mass by descending to some ##r## coordinate slightly above the horizon and hovering and measuring the acceleration needed to do so. Then dump in a load of mass and repeat. You'll find the same acceleration at a larger ##r##. Or you could look at gravitational lensing.

But none of that is really observing the event horizon - it's just measuring the mass. You can't really observe the horizon because it isn't a thing, just a null surface.
 
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  • #94
PAllen said:
In a sense, yes.

I am very likely missing something deep about curved space-time, but to me, that is the same thing as grossly / coarsely seeing something cross the EH.

The fact that I can't ever get photons from at or beyond the EH and the fact that photons redshift asymptotically as they are emitted from closer and closer to the EH are measurement limitations.

If I can see the EH expand by watching what it obscures or lenses, I observed something cross it with a measurement that doesn't depend on photons from the in-falling object, no? I guess its not really a claim that I saw that "thing" cross the EH - but in principle one can measure the total in-fall over time for a BH and if one has enough information on whatever is falling in one can construct a sequence of the in-falling events.
 
  • #95
@Ibix If I read your post first I wouldn't have bothered with mine - thanks!
 
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  • #96
I mean, one issue here is using the Schwarzschild metric and test particles falling into the black hole of that. This is not really a physical scenario because it does not actually describe the spacetime of anything with appreciable mass falling into a black hole. It just happens to be a relatively good approximation for many situations when the contribution of the infalling object to the spacetime geometry is negligible. This is certainly not the situation in the merger of two similar sized black holes.
 
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  • #97
Grinkle said:
I am very likely missing something deep about curved space-time, but to me, that is the same thing as grossly / coarsely seeing something cross the EH.

The fact that I can't ever get photons from at or beyond the EH and the fact that photons redshift asymptotically as they are emitted from closer and closer to the EH are measurement limitations.

If I can see the EH expand by watching what it obscures or lenses, I observed something cross it with a measurement that doesn't depend on photons from the in-falling object, no? I guess its not really a claim that I saw that "thing" cross the EH - but in principle one can measure the total in-fall over time for a BH and if one has enough information on whatever is falling in one can construct a sequence of the in-falling events.
Here is a dertailed, accurate, simulation of what would be seen against a stellar background for two equal size BH. It is easy to imagine how it would look for other cases:

 
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