Is 'charged black hole' an oxymoron?

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The discussion centers on the concept of charged black holes (BH) and whether the notion of a "charged black hole" is an oxymoron, particularly from the perspectives of General Relativity (GR) and Quantum Electrodynamics (QED). Key points include the established view that the net charge of a BH remains invariant regardless of the position of infalling charged matter, as determined by Gauss's law. However, participants express skepticism about this invariance, arguing that the local charge-to-mass ratio may not be reflected in remote observations, especially as the event horizon (EH) is approached. The implications of gravitational redshift on charge and the potential failure of global charge invariance in the presence of gravity are also debated. Ultimately, the conversation highlights a need for further exploration of the physical consequences of these theoretical frameworks.
  • #241
Trenton said:
It would be very nice to park an ion-engine in orbit round a black hole and pump a few tones of protons at it to see what would happen. If there is an inner horizon (spacetime infall is arrested by sufficient force) then when this horizon meets the outer horizon a mini big bang will occur.
As I understand it, it's actually very difficult for a black hole to acquire a significant charge. A positively charged black hole would repel any protons near it, so those protons would have to be fired inwards with a very high kinetic energy to overcome the electrical repulsion. If absorption is achieved, the kinetic energy contributes to the mass of the black hole (via E=mc2), and eventually you reach a point where each proton adds more mass than charge. Therefore it's postulated (I think) that the two horizons might never meet.
 
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  • #242
DrGreg said:
As I understand it, it's actually very difficult for a black hole to acquire a significant charge. A positively charged black hole would repel any protons near it, so those protons would have to be fired inwards with a very high kinetic energy to overcome the electrical repulsion. If absorption is achieved, the kinetic energy contributes to the mass of the black hole (via E=mc2), and eventually you reach a point where each proton adds more mass than charge. Therefore it's postulated (I think) that the two horizons might never meet.

What type of measurement would distinguish between a charged and an uncharged black hole?
 
  • #243
GAsahi said:
What type of measurement would distinguish between a charged and an uncharged black hole?
The motion of charged vs uncharged particles.
 
  • #244
Originally Posted by Austin0

So this increase would seem to indicate an increase of some kind of mass or a decrease of energy output of the means of propulsion ?


DaleSpam said:
Or an increase in the gravitational force on the same mass.

OK but I thought that the concept of downward force has been eliminated from GR ??

Unless it was an upward acceleration without actual motion. Stationary on the ground eg.
 
  • #245
DaleSpam said:
The motion of charged vs uncharged particles.

How would charge escape from the hole if light cannot?
 
  • #246
Austin0 said:
How would charge escape from the hole if light cannot?
You can perform those experiments outside the EH.
 
  • #247
Austin0 said:
OK but I thought that the concept of downward force has been eliminated from GR ??
It isn't eliminated, it is just a fictitious force in GR. I.e. the force of gravity is equivalent to the fictitious force in an accelerating reference frame.
 
  • #248
Update. Why not simply apply the well known notion of effective refractive index to this situation. At least for static gravity case, coordinate transverse light speed reduction and redshift in electrostatic/magnetostatic energy is obtained by having vacuum permittivity ε0 and permeability μ0 equally altered according to ε,μ = (1/√-gtt)(ε00), with -gtt = (1-2GM/(cr2)). This alteration is a coordinate determination and not locally observed. It naturally leads to the picture of charge being effectively screened by an increased vacuum dielectric constant, which gives a more consistent picture than that of simply depressing charge. Final result of applying this view is still that charge invariance globally fails and in particular no BH exterior electric field should exist.
 
  • #249
I don't know Q-reeus. I have been going through the math for several days now, and I can show that the redshifting depends primarily on the rank and type of the tensor. Since charge and invariant mass are scalars (rank 0 tensor), the idea of either of them redshifting is, I think, incorrect. I am not quite done working on the math yet, but I don't think that any of the conclusions based on the idea that mass redshifts are going to be valid.
 
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  • #250
but I don't think that any of the conclusions based on the idea that mass redshifts are going to be valid...

I'm unsure exactly what you are doing, but Marcus was able to offer some insights on this question which I raised.

Summary: the deBroglie wavelength [of a matter particle] redshifts just like light, except that with a matter particle it slows down while light maintains c locally while it redshifts.

Is the Universe leaking Energy?
http://www.physics.uq.edu.au/downloa...iAm_Energy.pdf

and she said the following [approximately]:

Photons traveling in an expanding universe appear to lose energy via cosmological redshift. What about matter: You find that the de Broglie wavelength of particles increases by exactly the same proportion as a photon’s wavelength does! Thus light and matter seem to behave in exactly the same way when it comes to 'energy loss'.

where Marcus noted:
...expansion causes things to lose momentum relative to the CMB...
'things' here meaning matter particles and photon redshift

the discussion begins here:
https://www.physicsforums.com/showthread.php?t=614297&page=2 with post #32...

As the discussion unfolds Marcus cites a Weinberg and Zang paper and notes "momentum goes as one over the scale factor", p proportional to 1/a...

Hope that helps.

edit: this is FLRW spacetime.
 
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  • #251
Interesting. I will check if the same holds true in Schwarzschild spacetime.
 
  • #252
Austin0:
How would charge escape from the hole if light cannot?

[side comment: I think that's a question lacking proper perspective. For another thing, beside the above answer, a charged black hole will have more gravitational curvature due to the energy of the electromagnetic field.]

One view from Roger Penrose:

There is no mass as we know it (inside); inside all particles have been destroyed and gravitational effects remain outside the event horizon along with a few characteristics (electric charge, spin, etc).


from a loooong discussion in these forums [sorry, I did not save a link]

...the "source" of the observed EM field around a charged BH is the charge-current density in the collapsing matter; i.e., the observed field at any event in the exterior region is entirely determined by field propagation from charge-current density in the past light cone of that event.
[sounds like a PeterDonis, maybe??]
 
  • #253
Naty1 said:
[sounds like a PeterDonis, maybe??]

Yes, that was me, and yes, I was taking the same position that Penrose is taking in the quote from him. AFAIK that is the standard answer to the question "how does the charge get out of the BH?" (i.e., it doesn't have to), similar to the standard answer to the question "how does gravity get out of the BH?" There would also be an analogous question, "how does the angular momentum get out of the BH?", but for some reason nobody ever asks that one. :wink:
 
  • #254
DaleSpam said:
I don't know Q-reeus. I have been going through the math for several days now, and I can show that the redshifting depends primarily on the rank and type of the tensor. Since charge and invariant mass are scalars (rank 0 tensor), the idea of either of them redshifting is, I think, incorrect. I am not quite done working on the math yet, but I don't think that any of the conclusions based on the idea that mass redshifts are going to be valid.
Good to know you've been beavering away on it DaleSpam! You are surely aware I and one or two others have been using 'redshift' in a loose way wrt mass/energy and charge. We know lowering any form of mass/energy of coordinate rest energy m down the potential well of some isolated massive body of rest energy M results in a net increase in gravitating mass to M+m√-gtt, less than M+m owing to 'redshift' of m. Which can be more or less directly linked to the mass 'redshift'by in principle annihilating m or rather m√-gtt and recovering the requisite redshifted radiation to infinity. The factor is the same regardless of tensor rank. E=hf makes the linkage rather good. As for charge, the huge problem with standard view is to reconcile that field energy does depress by redshift factor (non-free-fall case), yet field strength supposedly experiences no diminution whatsoever. Which btw also logically demands charge field lines remain exactly flat spacetime Coulombic in form regardless of how gravitationally warped things are for everything else. Strange indeed. No way I can see a sensible reconciliation without allowing effective charge screening as per last post. :zzz:
 
  • #255
Naty1 said:
Summary: the deBroglie wavelength [of a matter particle] redshifts just like light, except that with a matter particle it slows down while light maintains c locally while it redshifts.
There is some similarity but clearly not a 1:1 correspondence. A light ray will always outrun and outlast an outgoing particle whose local deBroglie wavelength goes infinite at it's turn-around point for instance.
 
  • #256
DaleSpam said:
Interesting. I will check if the same holds true in Schwarzschild spacetime.

It looks like marcus was talking about the change in scale factor with expansion in FRW spacetime, and how it affects photons vs. massive particles. I'm not sure how relevant that will be to Schwarzschild spacetime, except for the general point that the observed energy of an object is the contraction of the object's 4-momentum with the observer's 4-velocity. But the particular effect marcus was talking about as "losing momentum relative to the CMB" does not happen in Schwarzschild spacetime because there is no expansion.
 
  • #257
PeterDonis:
It looks like marcus was talking about the change in scale factor with expansion in FRW spacetime, and how it affects photons vs. massive particles. I'm not sure how relevant that will be to Schwarzschild spacetime,

Correct regarding Marcus. I edited my post above to highlight FLRW spacetime.
...the particular effect marcus was talking about as "losing momentum relative to the CMB" does not happen in Schwarzschild spacetime because there is no expansion.

exactly...I did not know Dalespam was working in Schwarzschild coordinates; On the other hand redshift is redshift, gravitational or 'expansion distance based', so it will be interesting to see if anything worthwhile appears.

Is this the issue where it was recently discussed 'why free fall has no redshift' or somesuch?? I just realized that might be where this discussion resides...I don't recall those coordinates. Sorry if I detoured the discussion.
 
  • #259
Q-reeus said:
We know lowering any form of mass/energy of coordinate rest energy m down the potential well of some isolated massive body of rest energy M results in a net increase in gravitating mass to M+m√-gtt, less than M+m owing to 'redshift' of m.
I don't know that, do you have a reference or derivation?

I am also not sure of the relevance to most of the thought experiments proposed here, which have seemed to focus on test masses and charges interacting with each other rather than altering the field of the gravitating mass. I think that assuming the two things are equal is sketchy.
 
  • #260
Q-reeus said:
We know lowering any form of mass/energy of coordinate rest energy m down the potential well of some isolated massive body of rest energy M results in a net increase in gravitating mass to M+m√-gtt, less than M+m owing to 'redshift' of m. Which can be more or less directly linked to the mass 'redshift'by in principle annihilating m or rather m√-gtt and recovering the requisite redshifted radiation to infinity.

I see DaleSpam has commented on this as well; this way of putting things conceals a lot of interpretation of ambiguous terms. We've gone into this in previous threads, and somewhat in this one, but perhaps it's worth some further comments to capture the thoughts I've come up with:

Suppose I am "hovering" at some large distance above a Schwarzschild black hole, and I measure its mass, M, by putting test objects into orbits about the hole, measuring their orbital parameters, and applying Kepler's Third Law. Then I drop an object of mass m, where I determine m locally by some similar procedure, into the hole. (All objects so far are electrically neutral; I'll talk about the charged BH/charged object case later in this post.) There are at least three possible ways I can do this:

(1) If I just let the object free-fall into the hole, and it doesn't give off any radiation, then the hole's mass, measured by me in the same way as before, will increase by m.

(2) If I slowly lower the object into the hole, extracting work from the process as I do so, then I can make the mass increase of the hole as small as I want by lowering the object closer and closer to the horizon before I finally have to release it and let it free-fall the rest of the way. In principle, how close to the horizon I can lower the object and still extract work depends on how I lower it and the strength of the materials I use to do so; ultimately it depends on what (finite) proper acceleration the lower end of the mechanism for lowering, the one attached to the object, can withstand. The final mass increase of the hole, for an idealized process where I extract the maximum amount of work possible while lowering the object to some radius r > 2M, will be m \sqrt{1 - 2M / r}.

(3) If I let the object free-fall towards the hole, but at some radius r > 2M, I capture all its kinetic energy and convert that to outgoing radiation (say, for example, it hits a large mirror which stops it, converts its kinetic energy into heat, and then reflects all the heat outward as it radiates away), I can in principle make the mass increase of the hole as small as I want, just as in #2 above, by moving the stopping point closer to the horizon. The only difference, from my point of view, is that I am now not capturing the difference between m and m \sqrt{1 - 2M / r} as work; it's just radiating away as heat.

There's another subtle point about the above three scenarios: how do we define the "energy at infinity" present? The three applicable quantities are the Komar mass, the ADM mass, and the Bondi mass. Here's how I see those for the three scenarios above (all three scenarios assume that all masses except that of the hole and the object dropped/lowered in are negligible):

Starting state: all three masses are M + m. Mass M is the hole, mass m is the object we're about to drop/lower in, which is at some finite radius so all three masses will include it.

#1: All three are unchanged; the only change is that M + m is now all contained in the hole.

#2: All three are unchanged: the only change is that M + m \sqrt{1 - 2M / r} is contained in the hole, and the remainder of m is still at our finite radius, where we recaptured it as work extracted from the lowering process.

#3: The ADM mass and Komar mass are still M + m; however, the Bondi mass is now decreased to M + m \sqrt{1 - 2M / r}, the new mass of the hole, because it will not include the mass (energy) of the radiation that escaped to infinity.

Now, suppose we do similar experiments to the above, but with a charged (R-N) black hole and a charged object. We have two possible cases, opposite charges and like charges. I am not presently working the math in detail as DaleSpam is, but it looks to me like the following are key points:

First, there should be a sort of ADM charge/Komar charge/Bondi charge for the spacetime as a whole, definable similar to the way the corresponding masses are defined. For the case we're considering, this total would include *both* the charge Q of the hole *and* the charge q of the object that's going to be dropped or lowered in. We, at a large finite radius, would measure the charge Q of the hole using charged test objects, similar to the way we measured its mass M by Keplerian orbits; we would also locally measure the charge q of the object to be dropped/lowered in similar to the way we measured its mass m locally.

Second, at the starting state, all three of the ADM/Komar/Bondi charges should be equal, just as the masses are; they should all be Q + q. However, at the end state for *any* of the three scenarios, *all three* charges should still be unchanged, *unlike* the case for masses above. This is because there is no way to radiate charge "away to infinity" as we can with mass by converting it into radiation. This is a key difference between mass and charge. (Note: it *is* possible for the charge q of the object dropped into cancel some or even all of the charge Q of the hole. However, if that is the case, all three of the ADM/Komar/Bondi charges *already* comprehend that; they already "see" the net charge, Q + q, which will be less than Q if q is of opposite sign.)

Third, if the object I am going to drop/lower into the hole is charged, then there is an extra energy e present in the spacetime as a whole, i.e., in the starting ADM/Komar/Bondi energy, due to the extra potential energy due to the charges Q and q being separated. So the total starting energy is M + m + e.

Note that as I've just defined it, e is positive if Q and q are of opposite sign--in this case, if I do a process like #2 or #3 above, I can in principle capture up to m + e of energy as work, or have that much energy radiate away to infinity, instead of it going into the hole. The final mass of the hole will be M + (m + e) * sqrt(1 - 2M/r), where r is the radius of the "stopping point", with the remainder of m + e captured as work or radiated away to infinity. The ADM/Komar mass will not change, and the Bondi mass will decrease to the new mass of the hole.

If Q and q are of the same sign, e will be *negative*. Depending on how large e is compared to m, it may be possible to do processes #1, #2, or #3 above, but capturing less energy than m (instead of more, as above); or it may not be possible to do them at all, because the electrical repulsion between the hole and the object is enough to require work to be *added* to the object to make it fall below the horizon.

Sorry for the long post, but I wanted to get all that down while it was fresh in my mind.
 
  • #261
DrGreg said:
As I understand it, it's actually very difficult for a black hole to acquire a significant charge. A positively charged black hole would repel any protons near it, so those protons would have to be fired inwards with a very high kinetic energy to overcome the electrical repulsion. If absorption is achieved, the kinetic energy contributes to the mass of the black hole (via E=mc2), and eventually you reach a point where each proton adds more mass than charge. Therefore it's postulated (I think) that the two horizons might never meet.

DrGreg,

I too have heard this but I am not sure quite how to view it. If, due to infall of space, nothing can be at rest inside the outer horizon because to do so would mean it was, in effect, traveling outwards at greater than C, then how can a charged particle do it? How indeed can a charged particle ever experience an electric field until it got to the singularity. Or is it that a charged black hole does not have a singularity but a dense entity bound by the inner horizon?

This last point arises from the idea that a spinning BH has a ring singularity. Spin distorts from a point to a ring. Charge if it distorts at all must be to a sphere - The only problem with that is it is no longer singular. One way at least to erradicate the naked singularity!
 
  • #262
PeterDonis said:
there should be a sort of ADM charge/Komar charge/Bondi charge for the spacetime as a whole, definable similar to the way the corresponding masses are defined.

Having run some formulas, let me be more definite about what I was proposing in the above quote. I emphasize that I have not seen this in any standard literature in this form, although what I'm proposing for the "ADM charge" is basically Gauss's law in integral form, slightly rewritten and taken to an appropriate limit.

(1) ADM charge: the integral for the ADM mass can be expressed as follows (note that I am leaving out constant factors involving pi and so forth, I'm only trying to look at the structure of the formulas, not give exact results):

M = \lim_{S \rightarrow i^{0}} \int g^{uv} \left( g_{ua, v} - g_{uv, a} \right) n^{a} d S

as given, for example, in this paper (which I believe references some of the original ADM papers):

http://arxiv.org/pdf/gr-qc/0609079v1.pdf

But we can rewrite this in a more general form:

M = \lim_{S \rightarrow i^{0}} \int m_{a} n^{a} d S

m_{a} = g^{uv} \left( g_{ua, v} - g_{uv, a} \right)

where now we have clearly separated out two distinct things: (1) defining a 2-sphere surface dS with outward pointing normal n^{a}, which we will then "take to infinity" in the limit; and (2) defining a 1-form m_{a} that represents "what we want to integrate" over the 2-surface. We will define "ADM charge" by keeping (1) the same but varying (2).

In the case of the ADM mass, what we are integrating over the 2-surface is basically the effect of the "mass" inside the surface on the metric at the surface. For charge, we want to integrate the effect of the charge inside the surface, over the surface. But we know how to do this: it's just Gauss's law. All we need to do is define a 1-form representing the "lines of force" going through the surface, which will be defined by the electric field normal to the surface. So we can write:

Q = \lim_{S \rightarrow i^{0}} \int F_{a0} n^{a} d S

This is basically Gauss's law, expressed in the "Schwarzschild" type coordinates we have been using for the R-N metric, taken to the limit at spatial infinity. But there's still one flaw: we've picked out a specific component of the EM field tensor, the "0" component. We can make the formula invariant by using the timelike Killing vector field of the spacetime, which will pick out the same "0" component in Schwarzschild coordinates, but which now allows the formula to be generalized to any chart, just like the ADM mass formula:

Q = \lim_{S \rightarrow i^{0}} \int F_{ab} n^{a} u^{b} d S

where u^{b} is a timelike unit vector (in this case, the "time translation" unit vector of R-N spacetime). It looks to me like, modulo constant factors, the value of this integral should equal the "Q" parameter in the standard R-N metric. I'll work on checking that explicitly.

(2) Komar charge: Actually, what I just wrote down above should *be* the Komar charge, as well as the ADM charge, because the "use a timelike vector field to make the integral formula invariant" trick is the same trick that's used for the standard Komar mass formula. There is one wrinkle: I haven't written down any analogue to the stress-energy tensor for charge. I think there's a way to finesse that by using Maxwell's equations to equate the expression F_{ab} n^{a} u^{b} to an expression involving the charge-current 4-vector. But I need to check that as well.

(3) Bondi charge: The formula for this would look the same as for the ADM charge, except that the limit would be taken as S goes to future null infinity instead of spatial infinity. Since there is no way for charge to radiate away to infinity, as I said before, this does not change the result at all, so Bondi charge = ADM charge.

Edit: Changed to timelike unit vector field in the above formulas (instead of timelike Killing vector field).
 
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  • #263
Austin0:

How would charge escape from the hole if light cannot?

Naty1 said:
[side comment: I think that's a question lacking proper perspective. For another thing, beside the above answer, a charged black hole will have more gravitational curvature due to the energy of the electromagnetic field.]

You may be quite right about perspective but your comment was a little indefinite to be really helpful ;-)

One view from Roger Penrose:

There is no mass as we know it (inside); inside all particles have been destroyed and gravitational effects remain outside the event horizon along with a few characteristics (electric charge, spin, etc).



...the "source" of the observed EM field around a charged BH is the charge-current density in the collapsing matter; i.e., the observed field at any event in the exterior region is entirely determined by field propagation from charge-current density in the past light cone of that event.

Could you elaborate on this concept of field propagation from past light cone?
_
Thanks_________________
 
  • #264
Austin0 said:
Could you elaborate on this concept of field propagation from past light cone?

I believe Naty1 got this from me originally; it actually came up in another thread earlier today, and I posted this:

https://www.physicsforums.com/showpost.php?p=3965324&postcount=17

It talks about gravity, not charge, but the reasoning for charge is similar; the only difference is that the "source" that has to be somewhere in the past light cone is the charge-current density 4-vector (the source in Maxwell's equations) instead of the stress-energy tensor (the source in the EFE).
 
  • #265
PeterDonis said:
I haven't written down any analogue to the stress-energy tensor for charge. I think there's a way to finesse that by using Maxwell's equations to equate the expression F_{ab} n^{a} u^{b} to an expression involving the charge-current 4-vector.

I should have seen this one at once; it's just the generalized Stokes Theorem plus Maxwell's equation with source. We have:

\int F_{ab} n^{a} u^{b} dS = \int \nabla_{c} F_{ab} g^{ac} u^{b} dV = \int J_{b} u^{b} dV

where it's technically the charge-current 1-form instead of the vector appearing, but that's a minor point. The only other potential issue is how to properly define the integration measure; I think there should be a \sqrt{-g} somewhere in there, but it may be that the appearance of the charge-current 1-form instead of the vector already implicitly takes that into account. But in any event I believe this shows how the "Komar charge" integral does in fact connect back to the source of the EM field, just as the Komar mass integral connects back to the source of gravity.
 
  • #266
PeterDonis said:
I believe Naty1 got this from me originally; it actually came up in another thread earlier today, and I posted this:

https://www.physicsforums.com/showpost.php?p=3965324&postcount=17

It talks about gravity, not charge, but the reasoning for charge is similar; the only difference is that the "source" that has to be somewhere in the past light cone is the charge-current density 4-vector (the source in Maxwell's equations) instead of the stress-energy tensor (the source in the EFE).

so we would have to go a billion years into the Earth's past light cone to find the "source" of the gravity the Earth feels at this instant--but the gravity itself, the effect, would be the same if the Sun's mass were the same, because the way the field from the collapsing object "propagates" through the empty vacuum region outside it is static--it stays the same for all time (again,

The basic past light cone analogy is self evident wrt the Earth-Sol system.
But if an electromagnetic or gravitational field is dependent on propagation, renewal from charged particles or mass, then the idea of a static propagation is a little obscure.
this would seem to imply that if the mass was moved somehow, the field could remain behind independent of a necessary source.
In the case of gravity it makes sense that the field would still be there. Possible that gravity itself is somehow exempt and still could emanate from the mass. But with charge, as Penrose said the source of charge , particles no longer exist at that point so the idea of a field remaining, extending to infinity with no source whatever is hard to understand.
As you might guess I am just starting to pay attention to black holes ;-)
 
  • #267
Austin0 said:
But if an electromagnetic or gravitational field is dependent on propagation, renewal from charged particles or mass, then the idea of a static propagation is a little obscure.
this would seem to imply that if the mass was moved somehow, the field could remain behind independent of a necessary source.

If the mass is moved, its "arrangement" in everybody's past light cone will change as the information about the move propagates to them. That changes the observed field.

In the particular case we've been discussing, that effect is obscured because the spacetime is static; nothing changes with time. In a more realistic, dynamic spacetime, the field observed at a given point would change with time, as dynamic information about the movement of masses elsewhere propagated around.

Austin0 said:
In the case of gravity it makes sense that the field would still be there. Possible that gravity itself is somehow exempt and still could emanate from the mass.

No, gravity isn't exempt. But the mass it's "emanating" from isn't inside the black hole.

If you want to view the field at a given point in space, outside the hole, as "emanating" from something, then it is emanating from portions of the collapsing matter far in the past, closer and closer to the horizon; as the collapsing matter far in the past gets closer and closer to the horizon, the time delay for light signals from it to get out to some fixed radius increases without bound. So the gravity you are sensing now "emanates", if you want to look at it that way, from some small piece of the collapsing matter's worldline, say, 10 meters above the horizon; the gravity you will sense some time in the future will have emanated from a small piece of the collapsing matter's worldline, say, 9 meters above the horizon; and so on.

In the case of a static spacetime (after the hole forms), the "emanating" view just above is equivalent to the "static" view, where once the collapsing matter falls inward past a certain radius, the field at that radius becomes fixed for all future time. But in a dynamic spacetime, there is no "static" view, so yes, you would need to look for dynamic information about the movement of mass traveling around.

Austin0 said:
But with charge, as Penrose said the source of charge , particles no longer exist at that point so the idea of a field remaining, extending to infinity with no source whatever is hard to understand.

The same thing I said above goes for charge; it emanates from charge-current density in the past just as gravity emanates from stress-energy in the past. Gravity "extends to infinity" just as charge does; the mass of any gravitating body leaves an "imprint" on the spacetime far away. Even if the gravitating body collapses to a black hole, the "imprint" of its mass on the spacetime remains the same, because the imprint doesn't come from inside the hole; it comes from the past, before the object disappeared behind the horizon, as described above. The "imprint" of charge on the spacetime works the same way. Even if there is no charge-current density inside the black hole (or any nonzero stress-energy), since it's all been destroyed in the singularity, there is still charge-current density (and stress-energy) in the past.

The ADM, Komar, and Bondi masses I talked about in recent posts are ways of describing the "imprint" of mass on the spacetime far away; the similar stuff I proposed for charges captures the same thing.
 
  • #268
PeterDonis said:
Q-reeus: "We know lowering any form of mass/energy of coordinate rest energy m down the potential well of some isolated massive body of rest energy M results in a net increase in gravitating mass to M+m√-gtt, less than M+m owing to 'redshift' of m. Which can be more or less directly linked to the mass 'redshift'by in principle annihilating m or rather m√-gtt and recovering the requisite redshifted radiation to infinity."

#3: The ADM mass and Komar mass are still M + m; however, the Bondi mass is now decreased to M + m√(1−2M/r), the new mass of the hole, because it will not include the mass (energy) of the radiation that escaped to infinity.
Well I had hoped it would have been evident this definition is what was being implied in bit quoted - we are obviously discounting as gone from considered system energy extracted in lowering (and 'lowering' was deliberately the term used) mass m. All btw covered in #1.
Now, suppose we do similar experiments to the above, but with a charged (R-N) black hole and a charged object. We have two possible cases, opposite charges and like charges. I am not presently working the math in detail as DaleSpam is, but it looks to me like the following are key points:

First, there should be a sort of ADM charge/Komar charge/Bondi charge for the spacetime as a whole, definable similar to the way the corresponding masses are defined. For the case we're considering, this total would include *both* the charge Q of the hole *and* the charge q of the object that's going to be dropped or lowered in. We, at a large finite radius, would measure the charge Q of the hole using charged test objects, similar to the way we measured its mass M by Keplerian orbits; we would also locally measure the charge q of the object to be dropped/lowered in similar to the way we measured its mass m locally.

Second, at the starting state, all three of the ADM/Komar/Bondi charges should be equal, just as the masses are; they should all be Q + q. However, at the end state for *any* of the three scenarios, *all three* charges should still be unchanged, *unlike* the case for masses above. This is because there is no way to radiate charge "away to infinity" as we can with mass by converting it into radiation. This is a key difference between mass and charge. (Note: it *is* possible for the charge q of the object dropped into cancel some or even all of the charge Q of the hole. However, if that is the case, all three of the ADM/Komar/Bondi charges *already* comprehend that; they already "see" the net charge, Q + q, which will be less than Q if q is of opposite sign.)

All that and your later points pretty well makes perfect sense *if* one starts off with the assumption of an RN BH that acts externally as a charged object - which however is what this thread set out to seriously question. I gave an updated argument involving effective charge screening in #248 which imo provides a level of conceptual consistency lacking in standard RN picture, as one or two of the bizarre consequences pointed out in #254 were meant to highlight. In fact apart from that added thought in #248 nothing substantially new has been added since #1 really. So I don't know, in the end it may simply come down to another fizzle/fadeout which at bottom amounts to "concensus/majority opinion ruulz - OK!" But no - sour grapes premature at this point. :-p
 
  • #269
Q-reeus said:
All that and your later points pretty well makes perfect sense *if* one starts off with the assumption of an RN BH that acts externally as a charged object - which however is what this thread set out to seriously question.

Well, everything I said would apply equally well to a charged massive object like a planet or star; DaleSpam recommended earlier that we start with that case, which avoids potential issues with what happens at or inside the R-N BH horizon, and if you're having problems with the BH case I would agree with his recommendation. The only difference with a planet or star vs. a BH is that the minimum radius r that you can lower something to is quite a bit larger than the horizon radius. But the ADM/Komar/Bondi charges I defined, just like their mass counterparts, are perfectly well-defined for a charged massive object, so they don't depend on having an R-N BH; they only depend on the exterior vacuum spacetime geometry of a charged massive object being R-N, i.e., only on R-N geometry outside some radius r greater than the horizon radius for the given mass and charge. I think the latter assumption is pretty safe.
 
  • #270
Q-reeus said:
a level of conceptual consistency lacking in standard RN picture, as one or two of the bizarre consequences pointed out in #254 were meant to highlight.

In #254, you say:

Q-reeus said:
the huge problem with standard view is to reconcile that field energy does depress by redshift factor (non-free-fall case), yet field strength supposedly experiences no diminution whatsoever.

I'm not sure what you mean by "field strength...experiences no diminution". Go back to scenario #2 in my previous post with a charged object, charged oppositely to the hole. The ADM/Komar/Bondi charge "at infinity" is Q + q always; but by hypothesis, you, at your finite radius, before you lower the charged object, see a field strength based on Q, *not* Q + q. After the object is lowered, you now see a reduced field strength, based on Q + q, which is less than Q, because that is now the charge you see on the hole. (Again, for "hole" read "central charged massive object" if that works better, see my previous post.)

Also remember that when you say "field energy does depress by redshift factor", what you really mean is that you are *extracting* energy from the lowering process. Where is that energy coming from? From the energy "at infinity" m + e of the charged object you are lowering. It does *not* come from the "energy of the hole", so it does not come from the "field energy" associated with the hole's charge Q. It comes only from "field energy" that is present because there is a second, opposite charge, q, which started out separated from Q, and then you brought them together. I don't see any problem or inconsistency anywhere in this.
 

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