B How do Black Holes Grow? A Far-Away Observer's Perspective

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Black holes are prevalent in astrophysics, with discussions often focusing on their appearance and the behavior of objects falling into them. From the perspective of a far-away observer, objects approaching a black hole appear to slow down and never actually cross the event horizon, raising questions about how black holes grow if nothing seems to fall in. The conversation highlights the distinction between the reality of falling into a black hole and the observer's perception, emphasizing that while an observer may not see the object cross the horizon, it indeed does fall in. The Schwarzschild solution describes a vacuum spacetime, and to understand black hole growth, models like the Oppenheimer-Snyder spacetime or numerical solutions are necessary. Ultimately, the discussion underscores the complexities of general relativity and the importance of distinguishing between coordinate systems and physical reality.
  • #61
Rene Dekker said:
If it is part of reality, there should be events that happen at the same time as events on Earth. I cannot understand that you can simply whip that into or out of existence by changing coordinate systems.
The counterintuitive thing here is buried in that phrase "at the same time". "At the same time" is just an informal way of saying "has the same time coordinate", so its meaning depends on the way that we assign time coordinates to events.

This is true even in a perfectly boring flat spacetime, no gravity, no curvature: Google for "relativity of simultaneity" to see how it works.

Or for a quick handwaving explanation: Say a bomb at rest relative to you explodes one light-second away from you, and the light from the explosion reaches your eyes when your wristwatch reads 12:00. It is absolutely natural (to the point that it would be perverse to suggest otherwise) to say that the explosion happened at the same time that your wristwatch read 11:59:59 and then the light took one second to get you, right? That's basically how we assign time coordinates to events not right under our nose. Well, someone moving relative to you, looking at your wristwatch through a telescope and using the same "time I see it, minus light travel time" logic will find that events "explosion" and "wristwatch read 11:59:59" did not happen at the same time.
 
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  • #62
Rene Dekker said:
What I am definitely confused by, is the habit of changing coordinate system if they don't suit your needs. In my mind, coordinates are related to measurements
You have already been taught that this is incorrect. Coordinates are basically just arbitrary labels, and they do not have any intrinsic relationship to measurements.

Rene Dekker said:
and you can only (and must) change a coordinate system, if it does not correspond to the measurements you are making.
You can adopt any smooth and invertible mapping as your coordinate system at any time for any reason or no reason. Usually we pick a coordinate system for convenience. Usually convenience is determined by how well it simplifies the math.

Rene Dekker said:
But the measurements (distances, proper time, etc) that you calculate with those coordinates should be the same. The should reflect reality.
Indeed, the measurements are invariant and any coordinate chart that covers a region will agree on the outcome of any measurements in that region. The problem is that the Schwarzschild coordinate chart does not cover the event horizon. So it cannot be used to make any statements about the horizon.

Rene Dekker said:
The event horizon is either part of reality or it isn't.
It is part of reality, but coordinates are not. So it is not a reflection on reality if a given coordinate chart does not cover the event horizon.

Rene Dekker said:
If it is part of reality, there should be events that happen at the same time as events on Earth
There have been studies that show that the single most difficult concept in learning relativity is understanding that the concept of “at the same time” is a human concept. It is not part of reality. The idea of “now” is part of the coordinates (simultaneity) so it is not a part of nature. This is a hard thing to accept, but it is well founded both experimentally and theoretically.

I don't know that we can make this easier, but we can teach correct principles and sympathize with your struggle in learning this difficult concept
 
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  • #63
Rene Dekker said:
What I am definitely confused by, is the habit of changing coordinate system if they don't suit your need
When you visit a new city do you use their addresses or what they would be in your home town? (Let's see...12 North Avenue would be 1,005,872 South Street and....)
 
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  • #64
Dale said:
Sure. You can use the simultaneity convention of any of the following:

https://en.m.wikipedia.org/wiki/Kruskal–Szekeres_coordinates

https://en.m.wikipedia.org/wiki/Lemaître_coordinates

https://en.m.wikipedia.org/wiki/Eddington–Finkelstein_coordinates

https://en.m.wikipedia.org/wiki/Gullstrand–Painlevé_coordinates

Or any other simultaneity convention you like. Your simultaneity convention is arbitrary.
I see your point. However, I would like to point out that these simultaneity conventions cannot be interpreted as synchronization conventions. A synchronization convention is an experimental procedure, while these simultaneity conventions cannot be used to experimentally synchronize two clocks, one outside and the other inside the black hole. It does not imply that these simultaneity conventions are wrong, but to avoid confusion (including my own) it is important to keep in mind the difference between simultaneity conventions and synchronization conventions.
 
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  • #65
Demystifier said:
I see your point. However, I would like to point out that these simultaneity conventions cannot be interpreted as synchronization conventions. A synchronization convention is an experimental procedure, while these simultaneity conventions cannot be used to experimentally synchronize two clocks, one outside and the other inside the black hole. It does not imply that these simultaneity conventions are wrong, but to avoid confusion (including my own) it is important to keep in mind the difference between simultaneity conventions and synchronization conventions.
They're distinct from synchronization conventions available to permanently external observers, yes. Free-falling observers (see Gullstrand-Painleve coordinates) may well synchronise clocks using these conventions, since they cross the horizon themselves. They can't complete the synchronisation process while the clocks are on opposite sides of the horizon, but they can cross the horizon before, during, or after it.
 
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  • #66
Rene Dekker said:
What I am definitely confused by, is the habit of changing coordinate system if they don't suit your needs. In my mind, coordinates are related to measurements, and you can only (and must) change a coordinate system, if it does not correspond to the measurements you are making.
Coordinates are not related to measurements. They are just arbitrary parameters mapping the spacetime manifold locally to open sets of ##\mathbb{R}^4##. From a mathematical point of view the "general covariance" of relativity, i.e., the local diffeomorphism invariance, is a gauge symmetry and in this sense coordinates are gauge-dependent mathematical entities and thus cannot be directly observables.

To cover a spacetime completely you usually need more than one such map ("coordinate chart"), i.e., an atlas in the sense of differentiable manifolds. As with an atlas consisting of maps of the Earth there are many possible atlasses of a spacetime, which itself however is independent of the choice of a specific atlas.
Rene Dekker said:
I can fully understand that different coordinate systems can describe the same reality in different ways, like cartesian and polar coordinates. But the measurements (distances, proper time, etc) that you calculate with those coordinates should be the same. The should reflect reality.
Exactly! I.e., only (local) gauge-invariant quantities (tensors) directly describe observables. It's as in electrodynamics: The four-potential is not directly an observable, because it's gauge dependent. You can calculate observables from it, i.e., the electromagnetic field, which is a tensor, which is independent of the choice of gauge.
 
  • #67
Demystifier said:
I see your point. However, I would like to point out that these simultaneity conventions cannot be interpreted as synchronization conventions. A synchronization convention is an experimental procedure
Oh, interesting. I have never seen this distinction before. It is a reasonable distinction, but it is novel to me.

Demystifier said:
these simultaneity conventions cannot be used to experimentally synchronize two clocks, one outside and the other inside the black hole
I would need to see a proof that this is true. Of course, you cannot use Einstein's synchronization procedure to do so, but to say that there exists no possible experimental synchronization procedure seems like quite a stretch.

I would think that it suffices to have one master clock broadcast a time signal and other clocks adjust their clocks accordingly by solving the null geodesic equation in the given coordinates. I.e. Einstein synchronization is based on knowing that the speed of light is c in inertial coordinates while in other coordinates it is not necessarily c but is nevertheless known. But I don't have a proof of the generality of such a procedure, nor a counter-proof.
 
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  • #68
Dale said:
I would think that it suffices to have one master clock broadcast a time signal and other clocks adjust their clocks accordingly by solving the null geodesic equation in the given coordinates.
It seems that you are right. Originally I thought that synchronization should involve an exchange of information between two clocks, but there is actually no need for that, one way information should be enough. If the master clock is outside the black hole, it should work. More precisely, it would work for physical black hole created in a gravitational collapse, but it would not work for a maximal Kruskal extension containing both the black and the white hole.
 

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