How GR Resolves the Conservation of Momentum and Energy

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The discussion centers on the implications of Noether's theorem for the conservation of energy and momentum in general relativity (GR). It highlights that while energy and momentum are conserved in flat spacetime due to time and space translational invariance, this is complicated in curved spacetimes where Killing vector fields may not exist. The presence of active diffeomorphisms can disrupt these Killing vector fields, leading to questions about the physical meaning of energy and momentum in GR. Rovelli's work emphasizes the challenges in defining a vacuum state when energy lacks a clear interpretation, suggesting a need to rethink traditional physics concepts. Ultimately, the conversation underscores the nuanced relationship between geometry, energy, and the fundamental principles of GR.
  • #31
PeterDonis said:
Hmm. I found this paper by Rovelli on arxiv, entitled "Loop Quantum Gravity and the Meaning of Diffeomorphism Invariance":

http://arxiv.org/pdf/gr-qc/9910079v2.pdf

Section 4 specifically talks about passive and active diffeomorphism invariance. Let me see if I understand what it's saying by giving two examples. Both examples start with the standard Schwarzschild exterior coordinate chart on the exterior vacuum region of Schwarzschild spacetime (i.e., the region outside the horizon). Call that spacetime S and that chart SC.

(1) A passive diffeomorphism is a transformation from SC to some other chart on the same manifold, for example the ingoing Painleve chart, PC. The statement that GR is invariant under passive diffeomorphisms is that the transformation SC -> PC does not change the underlying geometry of S; SC and PC may assign different coordinate 4-tuples to the same events, but all geometric invariants will be the same in both. And, of course, SC on S and PC on S will both be solutions of the EFE; on the surface they will look like different solutions, but computing the geometric invariants tells us that they both describe the same underlying geometry.

(2) An active diffeomorphism is a transformation that retains SC but changes the underlying spacetime from S to something else. For example, we could retain SC but change the underlying spacetime to Minkowski spacetime, M. After this transformation, the metric, and hence all geometric invariants, will look very different in terms of SC on M than they did in terms of SC on S. However, the statement that GR is invariant under active diffeomorphisms means that, if SC on S is a solution of the EFE, so is SC on M. They are *different* solutions, with different geometric invariants, but they're both solutions. So now we have two different geometries described using the same chart.

Am I understanding this correctly?

Your understanding of diffeomorphism was correct until you read Rovelli. Rovelli (as always) talks about a "dead fish in the sea". How about asking him for a mathematical (without reference to any (fuzzy) physics) definitions of passive and active Diff.
What is called diffeomorphism in mathematics, physicists call the Group of general coordinate transformations.
If active Diff (what ever that may be) is not equivalent to passive Diff (what ever that may be) then your math is wrong.
So, you better off without Rovelli and his "dead fish".

Sam
 
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  • #32
julian said:
Local notion of time is always defined? If you formally go from the action principle to the Hamiltonian princple of GR you find that the Hamiltonian (which generates time evolution) vanishes, implying there is no time evolution. This is why you get comments like the whole universe happans at once and the so-called 'problem of time' in quantum gravity. (This is related to the hole argument by the way).

You're mixing up two different things. The hamiltonian in the hamiltonian form of GR is not the same as the stress-energy tensor, which is what people normally mean by energy (roughly speaking, it's the masses of particles, plus their kinetic energies, plus the energies of the various fields). The stress-energy tensor is the source of gravitational curvature.

The stress-energy tensor is well defined at every point in spacetime.
 
  • #33
julian said:
Local notion of time is always defined? If you formally go from the action principle to the Hamiltonian princple of GR you find that the Hamiltonian (which generates time evolution) vanishes, implying there is no time evolution...

You need to read about time-evolution in constraiant systems. No time evolution means no dynamics. I hope you know that GR and all other gauge theories DO describe time evolution.

Sam
 
  • #34
julian said:
However, GR is invariant under active diffeomorphisms (Einstein's Hole argument) and general active diffeomorphisms will destroy any Killing vector field.

I don't see this.

Commutators of vector fields are preserved by push-forwards of diffeomporphisms, so push-forwards preserve Lie derivatives and thus Killing's equation.
 
  • #35
samalkhaiat said:
You need to read about time-evolution in constraiant systems. No time evolution means no dynamics. I hope you know that GR and all other gauge theories DO describe time evolution.

Sam

I understand that GR is a completely constrained system and you must identify a dynamical variable as the 'clock'...there is realtional evolution but not absolute...see Rovelli 'forget time'. It's great if you can deparamerterise a constrained system but this isn't always possible globally.
 
  • #36
George Jones said:
I don't see this.

Commutators of vector fields are preserved by push-forwards of diffeomporphisms, so push-forwards preserve Lie derivatives and thus Killing's equation.

It occurred to me yesterday that the transformation rule under active diffeomorphims is very similar in mathematical form to coordinate transformations and that I could be wrong on this point...thanks.
 
  • #37
samalkhaiat said:
No time evolution means no dynamics. I hope you know that GR and all other gauge theories DO describe time evolution.

Sam

No GR is a fully constrained system...it predicts the relationship between measurable quantities...see Rovelii 'partial and complete observables' or whatever it's called. This relationship is determined by the constraints imposed on the system.
 
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  • #38
julian said:
No GR is a fully constrained system...there are no dymanics in the usual sense. Like Thiemann stated about the Friedmann equations for cosmology ... they are gauge transformation equations and not evolution equations as most people think...

You can choose philosophically to view any deterministic system that evolves with time as fully constrained, I think. I don't like to discuss philosophy a lot because the arguments tend to be endless.

It's probalby best to say that ADM methods certainly treat GR as a system that evolves with time, where you specify it as an initial value problem along some particular space-like hypersurface, and see how the geometry evolves with time.
 
  • #39
pervect said:
You can choose philosophically to view any deterministic system that evolves with time as fully constrained, I think. I don't like to discuss philosophy a lot because the arguments tend to be endless.

It's probalby best to say that ADM methods certainly treat GR as a system that evolves with time, where you specify it as an initial value problem along some particular space-like hypersurface, and see how the geometry evolves with time.

It's not philosophy, any dynamical system can be written as a constrained system. This is called parameterisation. The opposite process is called deparameterisation...not all constrained systems are deparameterisable - they have to be of a specific mathematical form.
 
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  • #40
pervect said:
It's probalby best to say that ADM methods certainly treat GR as a system that evolves with time, where you specify it as an initial value problem along some particular space-like hypersurface, and see how the geometry evolves with time.

But as Thiemann comments on the Friedmann equations - they are gauge transformation equations and not real evolution equations. Let me find the reference.
 
  • #41
From the paper "Solving the Problem of Time in General Relativity and Cosmology with Phantoms and k -- Essence" - http://arxiv.org/pdf/astro-ph/0607380.pdf

Couple of quotes:

"By “the problem of time” in General Relativity (GR) one means that GR is a completely parametrised system. That is, there is no natural notion of time due to the diffeomorphism invariance of the theory
and therefore the canonical Hamiltonian which generates time reparametrisations vanishes."

and

"...the time evolution described by the FRW equations is obtained from the Hamiltonian equations of motion generated by the Hamiltonian constraint and not by an actual Hamiltonian. This is due to the fact that the “Hamiltonian” used to derive the FRW equations is actually constrained to vanish by one of the Einstein equations. The “evolution equations” generated by a constraint must therefore be interpreted as gauge transformations and those,..."
 
  • #42
The Hole arguemnt isn't just philosophy...to have a natural notion of time the constraint equations have to be of a specific mathematical form...but the GR equations, in general, aren't of this mathematical form...I think Rovelli claims this is the whole point of his book...maybe...dont quote me.
 
  • #43
Plus if you are to identify some dynamical variable that would work locally as a clock, this would necessarily be a real material object and thus be subject to quantum fluctuations itself - there is no absolute time that ticks away and which we could use to forumulate QM in the usual way - again probably see Rovelli.
 
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  • #44
George Jones said:
I don't see this.

Commutators of vector fields are preserved by push-forwards of diffeomporphisms, so push-forwards preserve Lie derivatives and thus Killing's equation.
I think I am either misunderstanding you or misunderstanding what an active diffeomorphism is.

My understanding is that an active diffeomorphism is a change in the manifold without a change in the coordinates. E.g. Changing from a Schwarzschild spacetime to a Kerr spacetime, but both in Schwarzschild coordinates. Clearly the Killing vectors are different.
 
  • #45
DaleSpam said:
I think I am either misunderstanding you or misunderstanding what an active diffeomorphism is.

My understanding is that an active diffeomorphism is a change in the manifold without a change in the coordinates. E.g. Changing from a Schwarzschild spacetime to a Kerr spacetime, but both in Schwarzschild coordinates. Clearly the Killing vectors are different.

Let there be a diffeomorphism between differentiable manifolds M and N, and let g be a "metric" tensor field for M. w is a Killing vector field on M iff L_w g = 0 (Lie derivative of the metric in the direction of w is zero).

The active diffeomorphism pushes forward fields w and g to fields w* and g* on N. Becasuse w is a Killing vector field for (M , g), w* is a Killing vector field for (N , g*), i.e., L_w* g* = 0. It is true that when N = M, w* will not, in general, be a Killing vector for g, but all fields get shuffled around (including g to g*) by the diffeomorphism, not just w to w*.
 
  • #46
George Jones said:
The active diffeomorphism pushes forward fields w and g to fields w* and g* on N. Becasuse w is a Killing vector field for (M , g), w* is a Killing vector field for (N , g*), i.e., L_w* g* = 0. It is true that when N = M, w* will not, in general, be a Killing vector for g, but all fields get shuffled around (including g to g*) by the diffeomorphism, not just w to w*.

To pick up on DaleSpam's example, this would mean that, if M is Schwarzschild spacetime and N is Kerr spacetime, the same active diffeomorphism that pushes forward the Schwarzschild metric on M (g) to the Kerr metric on N (g*) would also push forward every Killing vector field on M to a Killing vector field on N?

This seems plausible for the time translation Killing vector field, \partial_{t}; but does it also work for the angular ones? That seems odd, because in Schwarzschild spacetime there is a full 2-sphere's worth of angular Killing vector fields, so to speak, whereas in Kerr spacetime there is only one, \partial_{\phi}, since the spacetime is only axisymmetric, not spherically symmetric, correct?
 
  • #47
DaleSpam said:
Changing from a Schwarzschild spacetime to a Kerr spacetime, but both in Schwarzschild coordinates. Clearly the Killing vectors are different.
PeterDonis said:
To pick up on DaleSpam's example, this would mean that, if M is Schwarzschild spacetime and N is Kerr spacetime, the same active diffeomorphism that pushes forward the Schwarzschild metric on M (g) to the Kerr metric on N (g*) would also push forward every Killing vector field on M to a Killing vector field on N?

Kerr and Schwarzschild are not the same as topological spaces, and therefore they can't be diffeomorphic.
 
  • #48
George Jones said:
Kerr and Schwarzschild are not the same as topological spaces, and therefore they can't be diffeomorphic.

Ah--so that makes me wonder which spacetimes *could* be transformed into one another via an active diffeomorphism. Could you do Schwarzschild to Minkowski or vice versa? I'm guessing not because of the singularity in the former. If so, the conditions for being able to do an active diffeomorphism between different spacetimes would seem to be pretty restrictive.

Also, could you still do an active diffeomorphism taking just a portion of one manifold to a portion of another? For example, the portions of Schwarzschild and Kerr exterior to their respective horizons? Or does it have to be entire manifolds?
 
  • #49
Also, where does GR's "diffeomorphism invariance" among the EFE solutions go, if you don't even obtain topologically equivalent spaces?
 
  • #50
PeterDonis said:
Also, could you still do an active diffeomorphism taking just a portion of one manifold to a portion of another? For example, the portions of Schwarzschild and Kerr exterior to their respective horizons? Or does it have to be entire manifolds?
I don't think so, that would work if you just wanted to do a local diffeomorphism, wouldn't it? I believe "active diffeomorphisms" are not local.
 
  • #51
George Jones said:
Kerr and Schwarzschild are not the same as topological spaces
Oh. Is that because the Schwarzschild spacetime has a point singularity and the Kerr spacetime has a ring singularity?

EDIT: if so, then can't we restrict the manifolds e.g. to the region outside the EH. Then Kerr and Schwarzschild should have the same topology (that of R4 minus an open ball) while preserving the killing vector fields of each. Then we could do an active diffeomorphism between these two restricted manifolds.
 
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  • #52
TrickyDicky said:
Also, where does GR's "diffeomorphism invariance" among the EFE solutions go, if you don't even obtain topologically equivalent spaces?

Well, if you can't even do a diffeomorphism in the first place between topologically inequivalent spacetimes, then the question of invariance doesn't even arise, so it can't exactly be violated. :rolleyes:

But it does make me wonder what all the fuss over "active diffeomorphisms" is about, if the conditions for even being able to do them in the first place are so strict.
 
  • #53
PeterDonis said:
Well, if you can't even do a diffeomorphism in the first place between topologically inequivalent spacetimes, then the question of invariance doesn't even arise, so it can't exactly be violated. :rolleyes:

But it does make me wonder what all the fuss over "active diffeomorphisms" is about, if the conditions for even being able to do them in the first place are so strict.
I wonder too, but it can't be overlooked that diffeomorphism invariance (a.k.a. general covariance) is in all texts about GR as a defining property of the theory, what's the point if diffeomorphisms aren't even allowed? It's like saying that in Newton theory Lorentz invariance can't be violated because in a Euclidean space you can't even make a Lorentz transformation and then go on to say Newton's theory main feature is Lorentz invariance, pretty absurd ain't it?

It's an intriguing situation (perhaps George Jones can clarify) or at least I surely don't get it, how is it possible that physicists in general and relativists in particular don't even have a mnimum consensus on whether the distinction between active and passive diffeomorphism has any physical consequences, I have read about the same number of mainstream experts saying it is an important distinction physically (most LQG researchers like Rovelli) as those saying it is obvious it is exactly the same thing.
 
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  • #54
TrickyDicky said:
I wonder too, but it can't be overlooked that diffeomorphism invariance (a.k.a. general covariance) is in all texts about GR as a defining property of the theory, what's the point if diffeomorphisms aren't even allowed?

The general statements about diffeomorphism invariance apply to passive diffeomorphisms as well as active ones. Passive diffeomorphisms are just changes in coordinate chart; AFAICT everybody agrees that GR solutions are invariant under changes of coordinate chart. It's only active diffeomorphisms that appear to cause issues.
 
  • #55
I think that it is clear that GR is invariant over active diffeomorphisms also, but I have previously simply been of the opinion that active diffeomorphisms are non-physical. Now I am not so sure, but I don't think that I understand what they are so well.
 
  • #56
PeterDonis said:
The general statements about diffeomorphism invariance apply to passive diffeomorphisms as well as active ones. Passive diffeomorphisms are just changes in coordinate chart; AFAICT everybody agrees that GR solutions are invariant under changes of coordinate chart. It's only active diffeomorphisms that appear to cause issues.

Yes, that is the situation that has me perplexed with physicists not agreeing about. My own opinion is that this issue is mostly artificial, I don't see the distinction active/passive when applied to diffeomorphisms, by definition they are bijective and every diffeomorphism can have associated a coordinate transformation and its inverse (call'em active and passive if you like), at least this is how mathematicians seem to view it and if you look to math texts the active/passive distinction wrt diffeomorphism almost never shows up.
Leaving this aside and going back to my previous question I still can't see how certain GR solutions can have diffeomorphism invariance if as George Jones said they are not diffeomorphic manifolds. If two manifolds are not diffeomorphic I'd say one can't be obtained from the other thru a coordinate transformation, is this correct?
 
  • #57
Please distinguish between a statement that the laws of physics are invariant under a certain symmetry group (actually it should be called a dynamic symmetry to be precise), and a particular solution being invariant.

Obviously you cannot deform a sheet of paper into a donut, no matter how many transformations you make, so of course coordinate charts in one will not map to coordinate charts in the other.

There is no big mystery between active and passive diffeomorphisms, they are essentially related by pullbacks and pushforwards, and only in the case where you have some complicated mathematical object that is not a manifold (without a metric structure like what might show up in quantum gravity) where you have to be a little careful b/c there might be a difference. This is analogous mathematically to how tangent and cotangent bundles arise in differential geometry.
 
  • #58
Haelfix said:
Please distinguish between a statement that the laws of physics are invariant under a certain symmetry group (actually it should be called a dynamic symmetry to be precise), and a particular solution being invariant.

Well, I'm not sure what you are asking for here. General relativity is a statement about the laws of physics (a true statement if you don't reject the theory), and that is made concrete thru the EFE in tensorial form. Solutions of those equation should share that feature of the theory, shouldn't they? Please clarify if you are not referring to this.
Haelfix said:
Obviously you cannot deform a sheet of paper into a donut, no matter how many transformations you make, so of course coordinate charts in one will not map to coordinate charts in the other.
Exactly, but we are dealing with spaces that are solutions of the EFE here.
Haelfix said:
There is no big mystery between active and passive diffeomorphisms, they are essentially related by pullbacks and pushforwards, and only in the case where you have some complicated mathematical object that is not a manifold (without a metric structure like what might show up in quantum gravity) where you have to be a little careful b/c there might be a difference. This is analogous mathematically to how tangent and cotangent bundles arise in differential geometry.
Completely agree with you about this, and yet there are still endless discussions about this among experts especially those in the Loop quantum gravity field.
 
  • #59
TrickyDicky said:
If two manifolds are not diffeomorphic I'd say one can't be obtained from the other thru a coordinate transformation, is this correct?

Correct; there is no diffeomorphism that converts Schwarzschild into Kerr spacetime, for example. But I can certainly define diffeomorphisms that convert Schwarzschild under one coordinate chart (say the Schwarzschild chart) into Schwarzschild under another coordinate chart (say the Painleve chart). And both are solutions of the EFE. I realize that that seems like a tautology, since both charts describe the same geometry; but the point is that formally, the metric written in Schwarzschild coordinates solves the EFE written in those coordinates, and the metric written in Painleve coordinates solves the EFE written in those coordinates. The metric and the coordinate chart transform together to keep the underlying geometry invariant. So GR is diffeomorphism invariant in this sense.
 
  • #60
TrickyDicky said:
Solutions of those equation should share that feature of the theory, shouldn't they? .

Absolutely not! Forget about GR for a second. It is not even true about classical mechanics.

For instance, laws of physics (eg special relativity) are invariant under translations! However a particular solution typically is NOT invariant. For instance, if you are in an everywhere empty universe except for one room with a wall, that particular solution explicitly breaks Lorentz invariance in one direction.

Another example more pertinent the real world. In general, the particular solution of the EFE that we live in is decidedly not invariant under all diffeomorphisms. It is not even invariant under changes of scale (which is a subgroup of the diffeomorphism group) due to the presence of massive particles (which explicitly break conformal symmetry).

Another example the Minkowski metric breaks an infinite amount of diffeomorphisms, and only leaves a finite amount of isometries unbroken (four rotations, three translations and three boosts)

In fact the only tensor that is invariant under all diffeomorphisms is the trivial metric with all coefficients zero, but this fails to be a metric b/c it is not invertible.

See what I mean?
 

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