Black Holes and Charged Particles

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Discussion Overview

The discussion revolves around the behavior of charged particles as they fall into a black hole, particularly focusing on the implications for charge conservation and the nature of electric fields in the context of general relativity. Participants explore theoretical aspects, including the Reissner-Nordström solution and the electromagnetic fields associated with charged black holes.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants propose that when charged particles fall into a black hole, the charge may be considered lost until the black hole decays.
  • Others argue that a charged black hole can exist, as described by the Reissner-Nordström solution, and that electric fields remain outside the event horizon despite the charge falling in.
  • There is a discussion about whether electric fields can escape the event horizon, with some asserting that they cannot since they are mediated by photons.
  • Some participants clarify that the electromagnetic field outside the black hole is determined by past sources, even if those sources have fallen into the black hole.
  • There is contention regarding the perception of objects crossing the event horizon, with differing views on whether an outside observer can see an object approach and appear to stop at the horizon.
  • One participant suggests that the definition of "outside observer" is crucial, as it changes once an observer crosses the event horizon.
  • Another point raised is whether the coordinate in-fall time for an external observer is affected in Reissner-Nordström spacetime, particularly concerning the electromagnetic field of the falling charged particle.

Areas of Agreement / Disagreement

Participants express multiple competing views regarding the nature of charge conservation in black holes, the behavior of electric fields, and the perception of objects at the event horizon. The discussion remains unresolved with no consensus reached on these points.

Contextual Notes

Limitations include the dependence on definitions of observers and the complexities of electromagnetic fields in curved spacetime. The discussion also highlights the need for precision in statements made in this advanced context.

  • #31
nikkkom said:
For the outside observer, this never happens, right? It takes infinite time, as observed from outside, to cross the horizon?

No. The outside observer will never see the particle cross the horizon. But the outside observer cannot deduce from that that the horizon crossing never happens or that it takes infinite time.
 
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  • #32
PeterDonis said:
No. The outside observer will never see the particle cross the horizon. But the outside observer cannot deduce from that that the horizon crossing never happens or that it takes infinite time.

Outside observer can bounce a radar pulse off the falling object.

There are practical problems both with trying to do that with the "object" being a single electron, with the long time to get the pulse come back, and with red/blueshifting ("radio" waves may be seen as gamma ray by the object, and even if they do bounce off it, they will be red-shifted on the way back), but theoretically existence of the falling object is not unobservable.
 
  • #33
nikkkom said:
Outside observer can bounce a radar pulse off the falling object.

There are practical problems both with trying to do that with the "object" being a single electron, with the long time to get the pulse come back, and with red/blueshifting ("radio" waves may be seen as gamma ray by the object, and even if they do bounce off it, they will be red-shifted on the way back), but theoretically existence of the falling object is not unobservable.
No they can’t. There is a well defined time after which any light pulse sent sent by outside observer towards infaller will reach infaller only inside the horizon or not at all
 
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  • #34
So this is much simpler than @PeterDonis is making it. The charge in the Reissner–Nordström metric is located at the singularity:
https://en.wikipedia.org/wiki/Reissner–Nordström_metric#Charged_black_holes
In the section above, the electromagnetic potential is defined:
4ba45013717872e4f0b756b4127e2ce1fa1ac79c


So yes, we know effectively where the charge is. We don't need to invoke a lot of obfuscating mumbo-jumbo.
 
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  • #35
dllahr said:
The charge in the Reissner–Nordström metric is located at the singularity

No, it isn't. The "singularity" isn't even a single point, and it's certainly not a spatial point at the "center" of the black hole. Spacetime geometry in this case does not work the way you are assuming it does.
 
  • #36
So I guess the equation is wrong?
 
  • #37
dllahr said:
So I guess the equation is wrong?
I think what Peter is saying is that you are interpreting r as a distance from a centre. It doesn't really have that meaning in black hole spacetimes, since it changes from a space like to a time like coordinate as r varies.
 
  • #38
Ibix said:
I think what Peter is saying is that you are interpreting r as a distance from a centre. It doesn't really have that meaning in black hole spacetimes

Yes, that's what I'm saying.

Ibix said:
since it changes from a space like to a time like coordinate as r varies

That's not the real reason, since that property depends on your choice of coordinates. The real reason is that the locus ##r = 0## is not a "point at the center of the black hole". If you look at a Penrose diagram of Reissner-Nordstrom spacetime, you will see that there are actually two timelike lines that both correspond to ##r = 0##, and they are both inside the inner horizon. In fact, in the maximally extended geometry, which we have to talk about if we talk about going inside the inner horizon at all, there are an infinite number of such pairs of timelike lines. And, for good measure, these timelike lines are not actually part of the spacetime at all; they are limit points that do not exist in the actual manifold.
 
  • #39
dllahr said:
So I guess the equation is wrong?

The equation is fine; it just doesn't mean what you think it means.

And with that, this thread is closed.
 

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