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Phrak
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Is General Relativity Time Symmetric?
Yes it is.Phrak said:Is General Relativity Time Symmetric?
To put it in more formal terminology, the field equations of GR are form-invariant under diffeomorphisms, and time-reversal is a diffeomorphism. Therefore any solution is also a solution under time-reversal.JustinLevy said:bcrowell: "Time-reversal is a smooth coordinate transformation."
Hmm... I think I see what you mean here by "smooth" : the mapping of old coordinates to new coordinates is a smooth function.
But I have also heard of parity or time-reversal to not be considered smooth transformations because one cannot smoothly transition from the initial to final coordinate maps by a series of infinitesimal steps (like rotations, or stretching/scaling, etc.).
I claim that it is rigorous, as expressed above.JustinLevy said:Anyway, how do we show this more rigorously?
I think what you've proved is that the standard model can't be written in terms of tensors. That is, I don't think the standard model is diffeomorphism invariant. (It doesn't have general covariance.) If it were diffeomorphism invariant, it would be expressed without a background spacetime; but the standard model is expressed with a certain assumed background spacetime (flat spacetime).JustinLevy said:Merely being able to write the equations in tensor notation doesn't seem sufficient, as we can do that for the standard model, but it isn't time reversal invariant.
You don't have to crank through the complete rederivation of the curvature tensors. The curvature tensors change under a change of coordinates according to the tensor transformation laws. Since both sides of the Einstein field equations are tensors, they transform identically, and a time-reversed solution is still a solution.JustinLevy said:Under time reversal, the metric g_uv -> g'_uv will change sign on the dx dt, dy dt, dz dt, pieces. This will effect some terms of the curvature, maybe? This looks like it will get complicated. I'm not sure how it will affect the field equations.
It's a scalar, so it's invariant under diffomorphisms, including time reversal.JustinLevy said:Is the ricci curvature scalar affected by a time reversal?
You are probably thinking in terms of the differentiable symmetries of Noether's theorem. Parity is not an infinitesimal transform of the sort that would indicate a differential symmetry, but it is a smooth transform that indicates another kind of symmetry.JustinLevy said:But I have also heard of parity or time-reversal to not be considered smooth transformations because one cannot smoothly transition from the initial to final coordinate maps by a series of infinitesimal steps (like rotations, or stretching/scaling, etc.).
nicksauce said:So I'm not so sure about this, but maybe I'm missing something. I figure it would be easy to imagine a metric, which is not invariant under t-> -t, (just put some term in the metric proportional to t, for example). As long as the stress tensor is not completely ridiculous, you'd end up with a solution that is not time symmetric.
bcrowell said:[EDIT] Actually this is not quite right, as I realized by asking some questions over in Beyond the Standard Model and browsing WP. You can have spontaneous symmetry breaking. In cosmological solutions, Lorentz invariance is spontaneously broken by the occurrence of a preferred frame (the CMB's frame, or the frame of the Hubble flow). I guess T symmetry is also broken in perpetually expanding cosmologies.
This paper might be relevant: http://arxiv.org/abs/gr-qc/0603087atyy said:Certainly at the level of the equations of motion every theory can be made diff invariant, and apparently even at the level of the action http://arxiv.org/abs/1010.2535: "The point here is that any local theory (e.g., a single free scalar field) can be written in diffeomorphism-invariant form through a process known as parametrization"
I think diff invariance implies exactly the same thing as what you're saying about Newtonian mechanics.atyy said:In Newtonian mechanics, time reversal symmetry means if you reverse time and momenta, the different physical situation obtained is also a solution of the equations of motion. I think Demystifier was giving a comment along these lines, which seems to be different from the diff invariance perspective.
bcrowell said:This paper might be relevant: http://arxiv.org/abs/gr-qc/0603087
Take a look at p. 7. They show an example of a heat diffusion equation, which isn't diff-invariant, and definitely not time-reversal invariant. They turn it into a diff-invariant equation, but in order to do that they have to introduce a background field that points in the preferred direction of time. I think the key is that this background field is written as if it were a tensor, but it doesn't transform like a tensor; it's postulated to be constant in its upper-index form.
The field equations of GR aren't like this. They're written in terms of things that really transform like tensors -- no fixed background.
bcrowell said:I think diff invariance implies exactly the same thing as what you're saying about Newtonian mechanics.
In the standard formulation of Newtonian mechanics, the laws of physics are form-invariant under time reversal. Therefore any solution can be time-reversed, and it's still a solution.
In the standard formulation of GR, the laws of physics are form-invariant under diffeomorphisms, which include time reversal. Therefore any solution can be time-reversed, and it's still a solution.
I don't think there's anything mysterious or deep going on here. If you write down the tensor transformation law as applied to the rank-2 tensors in the Einstein field equations, they operate in the same way on both sides of the equation, and the only requirement is that the transformation be a diffeomorphism (so that the derivatives appearing in the transformation law don't blow up or fail to exist). The transformation can be any diffeomorphism you like. Time reversal is simply one special case.
This argument only depends on the assumption that everything in the field equations is a tensor that really transforms like a tensor -- not something that's written so as to look like a tensor, but doesn't transform like one.
This ISN'T enough.bcrowell said:I don't think there's anything mysterious or deep going on here. If you write down the tensor transformation law as applied to the rank-2 tensors in the Einstein field equations, they operate in the same way on both sides of the equation
I believe the standard model can be written in terms of tensors. Using your limited requirement for "time reversal symmetry", we can apply any coordinate transformation to both sides of a tensor equation, so yes, in that sense (which I feel lacks meaning) it has time reversal symmetry. But the "form" of the equations changed. The weak force instead of dealing only with left handed neutrinos, now only deals with right handed neutrinos.bcrowell said:I think what you've proved is that the standard model can't be written in terms of tensors.
Gauge symmetries certainly are real symmetries. They are the most fundamental symmetries of the standard model or any field theory. Also, per Noether's theorem they lead to conservation laws, e.g. the U(1) gauge symmetry leads to the conservation of charge.atyy said:But diff invariance is a gauge symmetry, which isn't a real symmetry, is it?
DaleSpam said:Gauge symmetries certainly are real symmetries. They are the most fundamental symmetries of the standard model or any field theory. Also, per Noether's theorem they lead to conservation laws, e.g. the U(1) gauge symmetry leads to the conservation of charge.
EDIT: I just realize that I have violated my usual policy of not getting involved in discussions about whether or not something is "real". So I would like to revise my above statement and simply say that a gauge symmetry is a differential symmetry that leads to a conservation law as per Noether's theorem. As to whether or not that qualifies it for status of a "real" symmetry depends on the definition of "real".
If you look at that example in the paper, the only way they were able to recast the heat diffusion equation into a diff-invariant form was by writing the field equations with a background "tensor" that doesn't really transform like a tensor. This background points in the forward time direction, and it's the only thing in the field equations that defines a direction in time.atyy said:I agree GR has no fixed background, which is different from diff invariance (or in the language of that paper, diff covariance). But what has no fixed background got to do with time reversal?
Hmm...you lost me here. It seems to me that the gauge symmetry of GR is symmetry under diffeomorphisms. We don't want time to be invariant under diffeomorphisms, because then it would be absolute...?atyy said:Time is absolute in Newtonian mechanics. The time you are referring to seems to be coordinate time, which is not gauge invariant. Is there any formulation using the absolute notion of timelike?
DaleSpam said:I don't know the distinction. I thought U(1) was the gauge symmetry.
bcrowell said:If you look at that example in the paper, the only way they were able to recast the heat diffusion equation into a diff-invariant form was by writing the field equations with a background "tensor" that doesn't really transform like a tensor. This background points in the forward time direction, and it's the only thing in the field equations that defines a direction in time.
bcrowell said:Hmm...you lost me here. It seems to me that the gauge symmetry of GR is symmetry under diffeomorphisms. We don't want time to be invariant under diffeomorphisms, because then it would be absolute...?
The coordinate-independent way of singling out the role of time, as opposed to some other coordinate, is that the signature of the metric is +---, as opposed to, say, ++++ or something. The signature is diff-invariant, by Sylvester's law of inertia. There is nothing in the field equations of GR that prevents us from constructing solutions with signatures like ++++ or ++--. When we look for solutions that have the +--- signature, we are externally imposing a requirement that is not present in the field equations, and that in some sense artificially breaks the symmetry between time and space.
If time reversal means taking some coordinate and subjecting it to a transformation [itex]t\rightarrow -t[/itex], then it's a diffeomorphism, and therefore a diff-invariant theory can't distinguish between a solution and its time-reversal. You don't have to say anything about "without prior geometry." If the equations of the theory are written solely in terms of tensors (meaning things that transform like tensors), then it's diff-invariant.atyy said:But how do we know that there is no theory without prior geometry that isn't time reversal invariant?
You seem to be saying that Lorentzian signature doesn't imply time-reversal invariance. That's true, but I never said anything to the contrary.atyy said:But what has the signature got to do with diffeomorphisms or no prior geometry? Special relativity also has Lorentzian signature, but the standard model of particle physics is a specail relativistic theory which isn't time reversal invariant.
bcrowell said:If time reversal means taking some coordinate and subjecting it to a transformation [itex]t\rightarrow -t[/itex], then it's a diffeomorphism, and therefore a diff-invariant theory can't distinguish between a solution and its time-reversal. You don't have to say anything about "without prior geometry." If the equations of the theory are written solely in terms of tensors (meaning things that transform like tensors), then it's diff-invariant.
bcrowell said:You seem to be saying that Lorentzian signature doesn't imply time-reversal invariance. That's true, but I never said anything to the contrary.
The reason I brought up Lorentz signature was in reply to your post where you asked this: "Time is absolute in Newtonian mechanics. The time you are referring to seems to be coordinate time, which is not gauge invariant. Is there any formulation using the absolute notion of timelike?"
bcrowell said:One thing to keep in mind is that GR itself has an extremely high level of symmetry, but that doesn't mean that the matter fields you plug into the stress-energy tensor have that same level of symmetry.
So if the OP asked the question "Is GR time-reversal-symmetric?" (paraphrased), possibly the reason we're all confusing each other is that some of us may be talking about GR itself, whereas others may be talking about GR coupled to some matter fields.
Again, I have to object here, because then by that reasoning electrodynamics has Galilean symmetry.bcrowell said:If time reversal means taking some coordinate and subjecting it to a transformation [itex]t\rightarrow -t[/itex], then it's a diffeomorphism, and therefore a diff-invariant theory can't distinguish between a solution and its time-reversal. You don't have to say anything about "without prior geometry." If the equations of the theory are written solely in terms of tensors (meaning things that transform like tensors), then it's diff-invariant.
I see. Yeah, that's a very good point that I hadn't thought about carefully enough before.atyy said:Well, basically I'm trying to understand if Demystifier's and your answers mean the same thing. It didn't seem obvious to me that "time reversal means taking some coordinate and subjecting it to a transformation [itex]t\rightarrow -t[/itex]" , because it's not clear in GR which coordinate is the "time" coordinate. So the definition of time reversal should involve a a diff-invariant quantity in GR, and I thought you were bringing in the signature as the meaning of time in GR.
I don't think swapping the signature from -+++ to +--- has anything to do with time reversal.atyy said:Is Demystifier's answer the same as saying that both every [-+++] GR spacetime has a [+---] counterpart which is its time reverse and also a GR spacetime?
I don't think the standard model can be written completely in tensor notation. There are all kinds of issues there. For instance, time is treated differently than position in quantum mechanics (time is not an operator), and that distinction can't be expressed in tensor language. Raising and lowering indices is done in the SM by using a fixed background metric, which doesn't transform like a tensor.JustinLevy said:Would you claim the standard model has Galilean symmetry?
Well, basically I think electrodynamics does have symmetry under Galilean transformations, but I don't necessarily mean what you think I mean by that. First off, there is the kind of difficulty that atyy was talking about above. Atyy pointed out that the meaning of a global time reversal is not even necessarily well defined in GR, on an arbitrary spacetime. This is even more of a problem when it comes to trying to define something like Galilean symmetry. You don't have global coordinate systems, so you don't necessarily have any clearcut way to define what you even mean by a global Galilean transformation. But in any case, I think it's certainly true that, for example, any electrovac solution of GR is still a solution under an arbitrary diffeomorphism. The electrovac field equations basically make statements about purely topological facts, e.g., that magnetic field lines never terminate at a point, or that electric field lines don't pass through one another. They also relate the fields to the metric, but again only in ways that are diff-invariant. If you give me an electrovac solution that has the global topology of [itex]\mathbb{R}^4[/itex] and is time-orientable, then I can label it with a single coordinate chart consisting of four coordinates (p,q,r,s), where, say, p is everywhere timelike. Then it is certainly true that this electrovac solution is still a solution after I apply a diffeomorphism that takes q to q'=q+kp, where k is some constant. This diffeomorphism does sort of look like a Galilean transformation, if you think of p as time, q as position along some axis, and k as a velocity -- but there is no guarantee that this is really their physical interpretation in any meaningful way.JustinLevy said:Again, I have to object here, because then by that reasoning electrodynamics has Galilean symmetry.
bcrowell said:The fact that the signature is Lorentzian means that locally, you can always define a distinction between two light cones; locally, time reversal means swapping those two light cones. But to talk about global time-reversal, I think you have to assume that the spacetime is time-orientable, meaning that the distinction between timelike vectors in the two light cones can be made in a way that is continuous. Not all spacetimes are time-orientable.
So if your spacetime is not time-orientable, then I guess you definitely can't define anything like a global time-reversal.
Let's look at the lagrangian. There are no uncontracted spacetime or spinor indices. This means the action is, at a minimum, a psuedo-scalar. It cannot change under a coordinate transformation like a Galilean transformation ... the Lagrangian stays the same.bcrowell said:I don't think the standard model can be written completely in tensor notation.Would you claim the standard model has Galilean symmetry?
First responding to your comments on the standard model and time. In non-relativistic quantum "particle" theory, position is an operator, and time is merely a parameterizing label. But the standard model is a field theory. In relativistic quantum field theory, time and space must be treated equally, so either time must be promoted to an operator or position demoted to a label. The standard approach is coordinates are just labels in quantum field theory (and the field itself promoted to an operator). The Lagrangian / Path integral formulation helps really make this lorentz symmetry clear.bcrowell said:There are all kinds of issues there. For instance, time is treated differently than position in quantum mechanics (time is not an operator), and that distinction can't be expressed in tensor language. Raising and lowering indices is done in the SM by using a fixed background metric, which doesn't transform like a tensor.
You're turning this into a "global" vs "local" issue, which I feel is missing the point.bcrowell said:Well, basically I think electrodynamics does have symmetry under Galilean transformations, but I don't necessarily mean what you think I mean by that. First off, there is the kind of difficulty that atyy was talking about above. Atyy pointed out that the meaning of a global time reversal is not even necessarily well defined in GR, on an arbitrary spacetime. This is even more of a problem when it comes to trying to define something like Galilean symmetry. You don't have global coordinate systems, so you don't necessarily have any clearcut way to define what you even mean by a global Galilean transformation.
I think this is starting to hit on why coordinate independence itself is not sufficient to tell us whether theories have Lorentz symmetry, etc. Because they are coordinate independent, the coordinates lose physical meaning. They are merely labels. We can choose all kinds of bizarre coordinate systems. So merely doing the coordinate transformation which inverts the sign on the 0th component of the coordinate labels everywhere, may not even mean time inversion locally.bcrowell said:A secondary issue is that when you refer to Galilean symmetry, you're referring to something that carries a lot more baggage than a simple coordinate transformation. It's a coordinate transformation that is part of a continuous group, with each member of the group labeled by a velocity vector v. Transformations corresponding to v and -v are inverses. There is also the notion that v is related in some specific way to tangent vectors of observers' world-lines. All of these additional notions are separate things that do not follow from diff-invariance.
atyy said:Charge conservation via Noether's theorem comes from U(1) as a global symmetry, not a gauge symmetry.
I think the issue here is what the contractions mean. The contractions involve raising and lowering indices. In QFT the raising and lowering of the indices is done using a fixed metric, which doesn't transform like a tensor. Therefore the Lagrangian is written to look like a tensor, but it isn't actually a tensor.JustinLevy said:Let's look at the lagrangian. There are no uncontracted spacetime or spinor indices. This means the action is, at a minimum, a psuedo-scalar. It cannot change under a coordinate transformation like a Galilean transformation ... the Lagrangian stays the same.
If the spacetime is a fixed background that doesn't obey the Einstein field equations, then we're no longer discussing the symmetry properties of GR; we're discussing the symmetry properties of some theory that violates the Einstein field equations.JustinLevy said:Heck we can look at quantum field theory in curved spacetimes if you wish. (my understanding from others responding to this on this forum is that we can do this, but insurmountable issues arise if we try to take the next step and allow spacetime itself to be dynamicly interacting using the current quantum field theory framework)
To answer this question, you would have to define what was meant by a global Lorentz transformation. Since there is in general no way to define such a thing, there is no way to define whether GR has global Lorentz symmetry.JustinLevy said:You're turning this into a "global" vs "local" issue, which I feel is missing the point.
Would you agree with the following:
GR doesn't have global Lorentz symmetry.
GR has local Lorentz symmetry.
The theory has a certain symmetry if the laws of physics retain the same form under that transformation. It doesn't matter if you write the laws of physics as the Einstein field equations, a Lagrangian, or a Hamiltonian; they all have the same properties under the same transformations.JustinLevy said:A possible definition of symmetry is: If the operator generating some symmetry commutes with the Hamiltonian, then the theory is said to have that symmetry.
Wait, you're claiming terms like the free field in QED:bcrowell said:I think the issue here is what the contractions mean. The contractions involve raising and lowering indices. In QFT the raising and lowering of the indices is done using a fixed metric, which doesn't transform like a tensor. Therefore the Lagrangian is written to look like a tensor, but it isn't actually a tensor.
You were using the ability to write the lagrangian in coordinate free notation (and thus be valid under any coordinate system, or coordinate transformation), to make claims about physical symmetries. I brought up non GR examples to simplify the situation and point out what I hoped would be obvious counter-examples.bcrowell said:If the spacetime is a fixed background that doesn't obey the Einstein field equations, then we're no longer discussing the symmetry properties of GR; we're discussing the symmetry properties of some theory that violates the Einstein field equations.
By "meant by" you seem to want to inject some kind of physical / coordinate independent meaning, to what the coordinate transformation is doing. So you seem to have some sense of the lorentz symmetry, not being just a coordinate symmetry of the equations ... which is exactly what I'm trying to get at. You can't just take the Lagrangian, which is a scalar and coordinate indepedent, and claim because it is coordinate independent that automatically means it has any coordinate symmetry.bcrowell said:To answer this question, you would have to define what was meant by a global Lorentz transformation. Since there is in general no way to define such a thing, there is no way to define whether GR has global Lorentz symmetry.
No. I would maintain that classical electrodynamics, written in tensor notation, retains that "form" regardless of the coordinate system you use. But if you look at how the evolution equations look in terms of E and B fields, they will NOT look the same after applying a galilean transformation. So if you use "same form" to define symmetry, then the resulting symmetries do depend on how you write it. I don't think this "same form" definition is precise enough, or useful, when we have tensor equations which are coordinate system independent.bcrowell said:The theory has a certain symmetry if the laws of physics retain the same form under that transformation. It doesn't matter if you write the laws of physics as the Einstein field equations, a Lagrangian, or a Hamiltonian; they all have the same properties under the same transformations.
Again, by this argument, GR has local Galilean symmetry.bcrowell said:I think the long and the short of it is this. Almost all spacetimes that are of any physical interest are time-orientable. Time-orientability is an extremely weak condition. Even a spacetime that has closed, timelike curves is typically still time-orientable. For any time-orientable spacetime, there is a unique and physically reasonable way to define a time-reversal operator. In particular, this operator acts in the same way locally (in the tangent space) as the time-reversal from the Poincare group. This operator is a diffeomorphism, so by diff-invariance, a spacetime that has been subjected to this operation remains a valid solution to the Einstein field equations. In this sense, GR has time-reversal symmetry.
You were right about this point and I was wrong. I wasn't appropriately distinguishing between a fixed geometry and a fixed form for the metric.JustinLevy said:The geometry is fixed, not the components of the metric. That term is indeed a scalar.
Yes, if you don't take that to imply any of the "baggage" referred to in #29. Otherwise no.JustinLevy said:Would you claim GR has local Galilean symmetry, just because the lagrangian is a scalar?
The field equations of classical electrodynamics as expressed in GR, on a dynamical background, are certainly form-invariant under a local Galilean transformation. But again, that doesn't imply any of the "baggage," and there is also no sensible way to define a global Galilean transformation, because we don't have global coordinates that have the right interpretation.JustinLevy said:No. I would maintain that classical electrodynamics, written in tensor notation, retains that "form" regardless of the coordinate system you use. But if you look at how the evolution equations look in terms of E and B fields, they will NOT look the same after applying a galilean transformation. So if you use "same form" to define symmetry, then the resulting symmetries do depend on how you write it. I don't think this "same form" definition is precise enough, or useful, when we have tensor equations which are coordinate system independent.