PeterDonis
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Q-reeus said:I just had this sixth-sense feeling we would meet up again about here.
Q-reeus said:As I further recall you cited ADM definition as evidence gravity (but only as GW's) sort of contributed. But that begs the question - what is fundamentally different about static vs propagating field curvature that one can sort of contribute but absolutely not the other?
I think you're either misremembering or misinterpreting--and to be fair, these issues are not easy to disentangle given all that has been said about them by various experts in the field. To briefly restate the key points from earlier discussions:
(1) Neither "static" nor "propagating" curvature contributes to the SET; *no* aspect of gravity contributes to the SET. (I've always been consistent about this. Also, I should note that I am assuming a zero cosmological constant; including that would just get us into a further argument about whether the cosmological constant should be viewed as an "aspect of gravity" or not, depending on which side of the EFE we choose to put it on. I don't think we need to go there.)
(2) If one really, really wants to salvage some kind of "contribution of gravity to total energy", one can define various pseudo-tensors that allow one to do that. However, they are all pseudo-tensors, meaning they are dependent on how you slice up spacetime into space and time, and they can only be consistently defined in certain kinds of spacetimes. None of this changes #1 above.
(3) One can also, in certain kinds of spacetimes, define "total energy at a given time" in different ways, which can sometimes give different results. In the case of a spacetime containing gravitational waves, such as a binary pulsar spacetime, one can show that the ADM energy and the Bondi energy are different, and the difference between them is standardly viewed as "energy carried away by gravitational waves". But this energy cannot be localized; it can only be "seen" when you look at the global properties of the spacetime. None of this changes #1 above either.
Q-reeus said:Gravitational waves for one!
Then in GR, curvature is "curvature of an actual physical medium" by your definition, and *not* just "curvature of spatial and temporal relationships", since GR predicts that gravitational waves can exist. What's the problem? (Also see further comments at the end of this post on spacetime as a "physically stressed medium".)
Q-reeus said:I understand that source - binary pulsars - as gravitating objects necessarily generates a static/quasi-static curvature through which GW's must propagate, but that's in geometric interpretation. You are well aware there exist other formulations of gravity where everything is owing to fields existing in an unobservable flat background spacetime. That's what I meant there.
This is a valid interpretation, but note that if you adopt it, the quasi-static part of the field does not "propagate". It's just there.
Q-reeus said:I'm no expert, but there are alternate descriptions/formulations using field concept - Yuri Baryshev comes to mind but there are others.
AFAIK there isn't any such alternate formulation that works for cosmology. But there is a lot of literature out there that I have not read, so I may be missing something. Any relevant links would be welcome.
Q-reeus said:In any case, sticking to geometric concept, how do you explain energy-momentum transport in GW's without it directly implying a physically 'stressed' medium of some sort?
To me, curved spacetime *is* a "physically stressed medium" that can transport energy. But looking at it that way dives below the level that GR addresses; it involves trying to come up with a more fundamental theory that underlies GR, such as string theory or loop quantum gravity. AFAIK it is generally accepted that GR is not a "fundamental" theory in this sense; it is a low-energy approximation to some other more fundamental theory. So I don't expect GR to tell me *how* curved spacetime can be a physically stressed medium; I need the more fundamental theory to do that. Unfortunately we don't have any way to probe the structure of spacetime at a small enough distance scale to investigate this sort of thing experimentally.
