Negative potential energy and negative mass

In summary: No matter how far apart I move the objects it will always require the addition of more energy to move them farther apart; so the potential energy at infinity is always greater than the energy at any finite distance, no matter how large. Thus, if...In summary, gravitational potential energy is normally negative because Ep = -G•M•m/r. This means that a system consisting of two widely separated objects will have a slightly greater mass than if the same two objects were close together.
  • #36
PeterDonis said:
whenever there is more than one gravitating mass present, strictly speaking, the spacetime is not stationary

I forgot to mention that I was speakting about the stationary case where the objects are fixed in their positions. Otherwise the equation for the total energy wouldn't be complete and the problem would be much ore complex.

PeterDonis said:
In practice, for cases where gravity is weak everywhere and everything is moving slowly compared to the speed of light, the expression you give for ##E## is a reasonable approximation if we define ##V = - GmM / r##.

The situation we are talking about (E<0) would require a distance of

[itex]r_0 < \frac{{r_s }}{8}[/itex]

between the objects, where rs is the Schwarzschild radius of the system. That means that ##V = - GmM / r## is definitely not a reasonable approximation.
 
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  • #37
DrStupid said:
I forgot to mention that I was speakting about the stationary case where the objects are fixed in their positions. Otherwise the equation for the total energy wouldn't be complete and the problem would be much ore complex.
The situation we are talking about (E<0) would require a distance of

[itex]r_0 < \frac{{r_s }}{8}[/itex]

between the objects, where rs is the Schwarzschild radius of the system. That means that ##V = - GmM / r## is definitely not a reasonable approximation.
You can have the objects or BH initially stationary but you could not keep them so. Thus the spacetime could not be stationary while satisfying the EFE - which imply the equations of motion. Only for a stationary spacetime is gravitational potential function possible in GR. Also only with BH could you have prayer of getting close enough to be interesting. That is why I felt what I suggested is necessary to approach this in GR
 
  • #38
PeterDonis said:
In practice, for cases where gravity is weak everywhere and everything is moving slowly compared to the speed of light, the expression you give for ##E## is a reasonable approximation if we define ##V = - GmM / r##. But note that for that case, we are no longer free to redefine the "zero point" of ##V##, because ##E## is now the total energy of the system as measured from the outside, and that measurement will have a definite result; we can't just arbitrarily adjust it by changing the zero point of ##V##. We have to use the zero point of ##V## that correctly predicts what the outside measurement will be, and that zero point is ##V \rightarrow 0## as ##r \rightarrow \infty##.

If I'm correctly reading between the lines of OP's post, then I think this is probably the most helpful response so far. I asked a similar question here a few months ago precisely because of the inconsistency between a "fixed" amount of rest energy on the one hand (a quantity that includes potential energies internal to the system!) and the "arbitrary" zero-point for potential energy on the other. Your replies in that thread cleared things up for me.

Maybe this will help OP, too:

##E = E_0 + E_k##

where ##E## is a system's total energy, ##E_0## is its rest energy (an "invariant" quantity that all observers agree on), and ##E_k## is its kinetic energy (energy related to the system's aggregate motion).

Rest energy is the total energy a system has as measured in its rest frame (the frame in which it has no momentum [or, equivalently, no kinetic energy]). It is simply the sum of all rest energy, kinetic energy, and potential energy that's "internal" to the system.

Einstein showed that rest energy and mass are the same thing, just measured in different units: ##E_0 = mc^2##.
 
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  • #39
DrStupid said:
I forgot to mention that I was speaking about the stationary case where the objects are fixed in their positions.

As @PAllen pointed out, the problem with this is that it's not a solution of the equations of motion. If you have gravitating bodies, they will fall towards each other unless something holds them in place. If something holds them in place, it must be exerting a force and must have energy, and that energy needs to be included.
 
  • #40
SiennaTheGr8 said:
Einstein showed that rest energy and mass are the same thing, just measured in different units: ##E_0 = mc^2##.
I didn't know dat. So, if two objects get closer, their mass is modified?
 
  • #41
Vicara said:
I didn't know dat. So, if two objects get closer, their mass is modified?

Yes, if by "their mass" you mean "the mass of the two-object system." The mass of each individual object remains fixed.

Actually, there's an additional subtlety: if by "get closer" you mean that the objects accelerate toward each other because of an attractive force (e.g., electrostatic [opposite charges] or gravitational*), then the mass of the whole system (including the field associated with the force) doesn't change, since the kinetic energy of the objects increases so as to counterbalance the decrease in the system's potential energy.

But if you're asking about comparing two different configurations in which the objects start at rest relative to one another (say), then the configuration with the objects closer together will have less mass, assuming that the force in question is indeed attractive. If the force is repulsive (e.g., the objects have the same charge), then the configuration with the objects closer together will have more mass. As @PeterDonis said, for these purposes we must define the zero-point for potential energy ##V \rightarrow 0## as ##r \rightarrow \infty##. For an attractive force, ##V < 0##. For a repulsive force, ##V > 0##.

*technically I shouldn't include gravity here, but I think it's okay as long as the gravitational field isn't so strong that we need general relativity to model it. Someone correct me if I'm wrong.
 
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  • #42
SiennaTheGr8 said:
Actually, there's an additional subtlety: if by "get closer" you mean that the objects accelerate toward each other because of an attractive force (e.g., electrostatic [opposite charges] or gravitational*), then the mass of the whole system (including the field associated with the force) doesn't change, since the kinetic energy of the objects increases so as to counterbalance the decrease in the system's potential energy.
I was talking about a system without kinetic energy
And what do you mean when you say that the entire mass of the system decreases but the individual masses don't? If somebody inside the system measures the mass of une object individually in diferent distances, there's no difference?
 
  • #43
Vicara said:
I was talking about a system without kinetic energy
And what do you mean when you say that the entire mass of the system decreases but the individual masses don't? If somebody inside the system measures the mass of une object individually in diferent distances, there's no difference?

Mass isn't additive. The mass of a system is not the sum of the masses of the system's constituents.

Mass is nothing but rest energy (expressed in different units). And rest energy is the total energy of a system as measured in the system's rest frame (the frame in which the system has no aggregate momentum). Rest energy includes all energy "internal" to the system: the rest energies (masses) of the system's constituents, the kinetic energy associated with their motion, and the potential energy associated with their relative positions. In everyday situations, the rest energies (masses) of the system's constituents are by far the greatest contributors to the system's rest energy (mass), so much so that the kinetic and potential contributions are often completely negligible or even undetectable. So mass is (approximately) additive in the classical limit.

But there are certainly situations in which the kinetic and potential contributions to a system's rest energy are not negligible. This mainly happens at atomic and nuclear scales.
 
  • #44
Vicara said:
I was talking about a system without kinetic energy
And what do you mean when you say that the entire mass of the system decreases but the individual masses don't? If somebody inside the system measures the mass of une object individually in diferent distances, there's no difference?

Look at Post #30 again. The mass of the system you introduced is given by $$m + M - G \frac{{mM}}{rc^2}.$$

The energy that binds the two constituents together lowers the mass of the system. Thus mass is not a measure of the quantity of matter in a system.
 
  • #45
PAllen said:
You can have the objects or BH initially stationary but you could not keep them so.

Why not?
 
  • #46
PeterDonis said:
If something holds them in place, it must be exerting a force and must have energy, and that energy needs to be included.

That's why I added the comment, that V doesn't need to be limited to gravity. It also includes the potential energy resulting from any additional interaction involved.
 
  • #47
DrStupid said:
Why not?
If you evolve the initial state using the EFE, the objects would move closer together. If you add extra elements to keep them apart, you have a different problem scenario than the intended one. In any case, I don't see any down side to treating as initially stationary rather than stationary. ADM mass is conserved from initial conditions. You keep the whole problem as close as possible to Newtonian case
 
  • #48
PAllen said:
If you evolve the initial state using the EFE, the objects would move closer together.

Even in a co-rotating frame of reference?

PAllen said:
If you add extra elements to keep them apart, you have a different problem scenario than the intended one.

Are additional interactions excluded in the intended scenario? I didn't read the original question that way.
 
  • #49
DrStupid said:
Even in a co-rotating frame of reference?
Are additional interactions excluded in the intended scenario? I didn't read the original question that way.
I don't see any relevance to a corotating frame - there wouldn't be orbital motion in the idealized set up. The BH would move directly toward each other.

If you add e.g. a repulsive force field to keep the bodies static, that would add a positive potential function, cancelling the very effect the OP was trying to get at.
 
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  • #50
PAllen said:
If you add e.g. a repulsive force field to keep the bodies static, that would add a positive potential function, cancelling the very effect the OP was trying to get at.

Can you prove that?
 
  • #51
DrStupid said:
Can you prove that?
See post #41
 
  • #52
PAllen said:
See post #41

I don't see the prove in post #41. Could you be more specific please?
 
  • #53
DrStupid said:
I don't see the prove in post #41. Could you be more specific please?
What is it you want proved? That potential has to be positive for a repulsive force? I thought 41 did that perfectly well. Note, I did not state the potentials would exactly cancel, only that they would have cancellation I.e. work in opposite direction so as to make the problem not just different but much harder to possibly realize the effect the OP was after.

Can you answer why on Earth you want to introduce this at all, since it only obscures the issue?
 
  • #54
PAllen said:
What is it you want proved? That potential has to be positive for a repulsive force?
The potential does not have to be positive for a force field that happens to be repulsive near radius r.
 
  • #55
PAllen said:
What is it you want proved?

This:

PAllen said:
If you add e.g. a repulsive force field to keep the bodies static, that would add a positive potential function, cancelling the very effect the OP was trying to get at.

The fact that the potential of the repulsive force is always positive is not sufficient to prove this claim. As a counter example let's assume the total potential

[itex]V = \frac{k}{6} \cdot \left( {\frac{{18}}{{r^2 }} - \frac{{22}}{{r^3 }} + \frac{9}{{r^4 }}} \right) - \frac{k}{r}[/itex]

where the first term is the potential of the repulsive interaction (which is always positive) and the second the classical gravitational potential (wich is always negative). The total potential has two local minima. When the system switches from the initial stable state r=3 to the final stable state r=1 the potential and therefore the total energy will be reduced. To my understanding the OP asked if something like this can result in a negative total energy.

PAllen said:
Can you answer why on Earth you want to introduce this at all, since it only obscures the issue?

PeterDonis already answered that question in #35:

PeterDonis said:
[...] whenever there is more than one gravitating mass present, strictly speaking, the spacetime is not stationary, and in a non-stationary spacetime there is no way to define a potential ##V##.

The repulsive interaction is requiered to keep the system static.
 
  • #56
DrStupid said:
This:
The fact that the potential of the repulsive force is always positive is not sufficient to prove this claim. As a counter example let's assume the total potential

[itex]V = \frac{k}{6} \cdot \left( {\frac{{18}}{{r^2 }} - \frac{{22}}{{r^3 }} + \frac{9}{{r^4 }}} \right) - \frac{k}{r}[/itex]

where the first term is the potential of the repulsive interaction (which is always positive) and the second the classical gravitational potential (wich is always negative). The total potential has two local minima. When the system switches from the initial stable state r=3 to the final stable state r=1 the potential and therefore the total energy will be reduced. To my understanding the OP asked if something like this can result in a negative total energy.
PeterDonis already answered that question in #35:
The repulsive interaction is requiered to keep the system static.
I already answered the points before the last previously. Perhaps I should have said obscure or reduce rather than cancel, because I never meant or said exact cancellation.

[ deleted misunderstanding]

Peter's point is if you want to introduce a GR valid potential function, you need this. But the closer you posit the bodies, the stronger the opposing potential you need, making it impossible to say you've proved anything about impossibility of total energy becoming negative. I argued that all of this is pointless because ADM mass includes the effects of system gravitational potential energy, globally. Then you only need initially stationary. What you lose is a localizable potential function. But what you gain is much more important - not having to introduce major extraneous elements that work against the effect you are trying to maximize.
 
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  • #57
When I asked the question I was thinking about a system of two static bodies without kinetic energy (and I know that can't be possible or estable without any oter force or structure to keep them apart, but it was the simplest way to explain how "negative mass could exist")
 
  • #58
Vicara said:
When I asked the question I was thinking about a system of two static bodies without kinetic energy (and I know that can't be possible or estable without any oter force or structure to keep them apart, but it was the simplest way to explain how "negative mass could exist")
Right, and what I answered about was two bodies initially stationary, considering this situation from ever closer starting points. This gets at your goal in pure form in a way that is possible, without having to introduce extra elements that add to total energy.
 
  • #59
PAllen said:
But the closer you posit the bodies, the stronger the opposing potential you need, making it impossible to say you've proved anything about impossibility of total energy becoming negative.

As I generalized the question to any potential (not only resulting from gravity), it doesn't matter how strong the opposing potential is. The original scenario with the gravitational potential energy is included in this question as a special case.

PAllen said:
Then you only need initially stationary.

Then you need to explain how to reach such a state. Fixing the system with an external field and then releasing it doesn't work, because this field cannot be switched off instantaneous.
 
  • #60
DrStupid said:
Then you need to explain how to reach such a state. Fixing the system with an external field and then releasing it doesn't work, because this field cannot be switched off instantaneous.

Then switch it off gradually while they move apart. Gravity will then slow them down until they reach a maximum separation distance before they start to approach each other.
 
  • #61
Mister T said:
Then switch it off gradually while they move apart. Gravity will then slow them down until they reach a maximum separation distance before they start to approach each other.

Gravity needs to be very strong in the scenaro we are talking about and would therefore slow them down very fast. What makes you sure that the external field can be sitched off gradually without letting the objects moving too fast and emitting gravitational waves?
 
  • #62
Mister T said:
Then switch it off gradually while they move apart. Gravity will then slow them down until they reach a maximum separation distance before they start to approach each other.
Yep, that's a good way. But you could also just posit it as initial conditions. To use ADM methods in GR, all you need is conditions specified on one Cauchy surface. So it is not actually necessary to answer the question at all.
 
  • #63
PAllen said:
all you need is conditions specified on one Cauchy surface.

Is that the case for your initial conditions? Apart from the question for with observer the bodies come to rest for the same time - can you simply define that the space-time is static as well?
 
  • #64
DrStupid said:
Then you need to explain how to reach such a state. Fixing the system with an external field and then releasing it doesn't work, because this field cannot be switched off instantaneous.
No I don't. ADM methods in GR only require specification of conditions on some Cauchy surface. In this case, the most direct precursor history, if you insist, is not physically plausible, but is mathematically consistent in GR: just time reverse the forwrard evolution. This woul describe strong GW incoming from infinity, splitting a BH in two, with BF slowing and incoming GW decreasing until the Cauchy surface is reached. Then, outgoing GW start as the BH approach each other. ADM mass is constant the whole time, but implicitly has different componts due to potential energy, GW, and kinetic energy at different times.
 
  • #65
DrStupid said:
Is that the case for your initial conditions? Apart from the question for with observer the bodies come to rest for the same time - can you simply define that the space-time is static as well?
I don't define that it is static or stationary. I have stated it is not quite a few times already. Initial conditions must include first derivatives of metric quantities, so I simply posit, in some chosen harmonic coordinates, conditions such that the first derivative of separation between the BH is zero on Cauchy surface.
 
  • #66
That sounds like we could get an answer this way but it would be limited to a Cauchy surface that includes your initial conditions. This would be sufficient if the answer is yes, negative total energy is possible. If we get the answer No, negative total energies are not possible with these special conditions we would need to check other conditions as well (e.g. stable systems).
 
  • #67
PAllen said:
I simply posit, in some chosen harmonic coordinates, conditions such that the first derivative of separation between the BH is zero on Cauchy surface.

That's what I mean with "static".
 
  • #68
DrStupid said:
That sounds like we could get an answer this way but it would be limited to a Cauchy surface that includes your initial conditions. This would be sufficient if the answer is yes, negative total energy is possible. If we get the answer No, negative total energies are not possible with these special conditions we would need to check other conditions as well (e.g. stable systems).
My claim is any stable system would have a harder time achieving negative total energy because it would have additional positive components, which could then be removed to create an instance of my approach.
 
  • #69
DrStupid said:
That's what I mean with "static".
Oh, static has a very precise meaning in GR, and that is not it. Using it in a loose way is particularly confusing in a GR context.
 
  • #70
It occurs to me, that the question of this thread is covered by the Positive Energy Theorem, the best IMO proof of which was provided by Witten. The answer is then, no, you cannot do this without violating the dominant energy condition. At least in classical GR, one does not want to give this one up, because then geodesic motion no longer follows from the EFE, and it has even been shown that violation of the dominant energy condition makes possible to have small body that moves tachyonically. Many people interpret the dominant energy condition as simply saying physics alway looks consistent with SR locally.
 
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