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Relative energy of a black hole.

 
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Mar1-12, 10:44 AM   #86
 
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Relative energy of a black hole.


Quote by TrickyDicky View Post
They define (page 176 of the first reference) the source as the SET on the RHS of the EFE, and then they explicitly state that the gravitational field (energy) itself acts as a source.
Hmm. Do they give any actual examples of SETs? Or worked problems where they explicitly say what the SET is? I'm particularly curious if they give, for example, something like the solution for a static spherically symmetric star, which is one of the paradigmatic cases we've been discussing. In this case, the SET does *not* include any "gravitational field energy" (it's just the standard perfect fluid SET), but nevertheless it's commonly said that "gravitational field energy" needs to be taken into account in determining the externally measured mass M of the star.

(I've explained several times how the standard picture actually deals with this--the mass M is ultimately derived from the standard SET by solving the standard EFE, with no extra "source" terms for "gravitational field energy"--the latter just happens to be one way of describing the relationship between the mass M that appears in the metric and the standard SET that appears on the RHS of the EFE.)
Mar1-12, 12:04 PM   #87
 
Quote by PeterDonis View Post
Hmm. Do they give any actual examples of SETs? Or worked problems where they explicitly say what the SET is? I'm particularly curious if they give, for example, something like the solution for a static spherically symmetric star, which is one of the paradigmatic cases we've been discussing. In this case, the SET does *not* include any "gravitational field energy" (it's just the standard perfect fluid SET), but nevertheless it's commonly said that "gravitational field energy" needs to be taken into account in determining the externally measured mass M of the star.
Well in the static case highly unrealistic conditions are imposed: staticity, asymptotic flatness, vacuum... and still a very good approximation in solar system scale is reached.
The problem is nobody thinks our universe has those properties listed above, and it is in these cases (basically all GR physics other than the static solution) where the problem with gravitational fields as sources comes up. You cannot negate it because it doesn't appear in static solutions unless you believe our universe is static.
It is something that has been troubling relativists from 1915 when Hilbert referred to it saying that GR generates improper energy theorems. And it hasn't been solved, as I said is at the root of many difficulties with quantum gravity.
Mar1-12, 12:46 PM   #88
 
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So glad you guys are homing in on the discrepancy between Tricky's sources and the discucssion here!! .....
I have seen references like Tricky posted but could not locate any again....and yet everything Peter posts is also consistent with what I have seen.

This seems closely related to the issue...I sure don't get it:

..In general relativity, the partial derivatives used in special relativity are replaced by covariant derivatives. What this means is that the continuity equation no longer implies that the non-gravitational energy and momentum expressed by the tensor are absolutely conserved, i.e. the gravitational field can do work on matter and vice versa. In the classical limit of Newtonian gravity, this has a simple interpretation:
energy is being exchanged with gravitational potential energy, which is not included in the tensor
, and momentum is being transferred through the field to other bodies.
http://en.wikipedia.org/wiki/Stress-energy_tensor

Maybe this "classical limit" issue is the one Peter described:

".... it is intuitively appealing (because) we are used to looking at stationary, or nearly stationary, systems, for which two things are true: (1) a meaningful definition of "energy stored in the field" can be given that corresponds, intuitively, to "gravitational potential energy", which is familiar from Newtonian physics; (2) because the system is stationary, there is a very simple relationship between what's there on a spacelike slice and what's there in the past light cone of any particular event. The conceptual issues you are having are basically due to trying to extend the simple viewpoint that works reasonably well for stationary systems to a more general domain, non-stationary systems (systems that collapse, and systems that radiate energy) where items (1) and (2) no longer hold."
Mar1-12, 01:37 PM   #89
 
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Quote by PeterDonis View Post
Hmm. Do they give any actual examples of SETs? Or worked problems where they explicitly say what the SET is? I'm particularly curious if they give, for example, something like the solution for a static spherically symmetric star, which is one of the paradigmatic cases we've been discussing. In this case, the SET does *not* include any "gravitational field energy")
This is always the case. From 19.8 Gravitational Field Energy of Penrose's Road to Reality
Let us return to the question of mass/energy in the gravitational field itself. Although there is no room for such a thing in the energy-momentum tensor T, its is clear that there are situations where a 'disembodied' gravitational energy is actually playing a physical role.
Disembodied, because, from Ryder,
We cannot, then, identify a place or places, where where the gravitational field exists and carries energy, since whether the field carries energy also depends on the frame of reference. Gravitational energy is not localisable.
This means that gravitation energy cannot be included in the stress-energy-tensor field, as this is a mapping from spacetime into the space of tensors.

From page 131 of MTW's Gravitation
At each point in spacetime, there exists a stress-energy tensor. It is a machine that contains a knowledge of the energy density, momentum density, and stress as measured by any and all observers at that event. Included are energy, momentum, and stress associated with all forms of matter and all nongravitational fields.
These quotes do not contradict the other quotes in this thread taken from standard references.
Mar1-12, 02:01 PM   #90
 
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Quote by George Jones View Post
This is always the case.
Agreed, I should have made that clear (thought it ought to be clear from my other posts in this thread).

Quote by George Jones View Post
From 19.8 Gravitational Field Energy of Penrose's Road to Reality...
I don't have my copy handy to check: by "a physical role" for "disembodied" energy in the field, is he referring to gravitational waves carrying energy (for example, the binary pulsar emitting them, as has been discussed in this thread)?
Mar1-12, 02:11 PM   #91
 
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Quote by TrickyDicky View Post
You cannot negate it because it doesn't appear in static solutions unless you believe our universe is static.
I wasn't intending to say that my statements about the SET only applied to the static case; they always apply (see George Jones' post and my response). I was only using the static case as a simple example that most textbooks say something about, so it might be a way to get more information about what the authors of this one were thinking.

Quote by TrickyDicky View Post
It is something that has been troubling relativists from 1915 when Hilbert referred to it saying that GR generates improper energy theorems. And it hasn't been solved, as I said is at the root of many difficulties with quantum gravity.
The "improper energy theorems" bother some relativists because, as I've said in previous posts, they don't fit our intuitions about how "energy" ought to behave. Since standard GR with the standard SET the way it is accounts for all the evidence we currently have, the question of whether the improper energy theorems are a "real problem" or just a sign that our intuitions aren't a good match for this area of physics is, IMO, more a question of philosophy than physics. If we get further evidence that doesn't match the standard GR predictions, then of course that will change, as I've already said.

With regard to quantum gravity, AFAIK the reason this issue creates a problem there is that we don't know how do to quantum theory period with systems that have improper energy theorems. It's quite possible that that is a problem with the way we are doing quantum theory rather than with gravity; we may simply be using the wrong set of tools. Again, unless and until we get further evidence, IMO this is more a question of philosophy than physics.
Mar1-12, 02:24 PM   #92
 
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Quote by PeterDonis View Post
Agreed, I should have made that clear (thought it ought to be clear from my other posts in this thread).
I thought that this is your position. I just wanted to agree, and to give quotes that back this up.
Quote by PeterDonis View Post
I don't have my copy handy to check: by "a physical role" for "disembodied" energy in the field, is he referring to gravitational waves carrying energy (for example, the binary pulsar emitting them, as has been discussed in this thread)?
Yes.
Mar1-12, 02:30 PM   #93
 
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Quote by Naty1 View Post
Maybe this "classical limit" issue is the one Peter described:
Yes, that's more or less right. Slightly further down the same Wiki page is this comment:

"In curved spacetime, the spacelike integral now depends on the spacelike slice, in general. There is in fact no way to define a global energy-momentum vector in a general curved spacetime."

It doesn't say exactly which "spacelike integral" is being talked about, but I assume they mean the continuity equation integral above. In certain special cases, a particular set of spacelike slices is picked out by the symmetry of the spacetime, and the continuity integral using that set of slices defines a "total energy" that behaves the way our "Newtonian" intuitions say energy ought to behave in the presence of gravity--it includes "gravitational energy", *and* energy is "exchanged" between ordinary matter-energy and gravitational energy in such a way that the total is conserved.

But that only holds for spacetimes where the symmetry picks out a particular set of spacelike slices: two examples are a single isolated gravitating body (the "Newtonian" case is a subcase of this), where the time translation symmetry picks out a particular set of slices, and a case like FRW spacetime, where the spherical symmetry defines a set of "comoving" observers that pick out a particular set of slices. (That's why the Usenet Physics FAQ page I linked to earlier includes this case in their discussion.)

Also, note carefully that the way "gravitational energy" enters into the continuity integral is *not* by any change in the SET's definition; it is purely due to the fact that, in curved spacetime, we use covariant derivatives instead of ordinary derivatives. That means extra terms come in due to the connection coefficients, and in certain special cases the extra terms have a simple interpretation in terms of "gravitational energy" being exchanged with ordinary matter-energy.
Mar1-12, 02:31 PM   #94
 
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Quote by George Jones View Post
I thought that this is your position. I just wanted to agree, and to give quotes that back this up.

Yes.
George, thanks for the support and clarification!
Mar1-12, 04:08 PM   #95
 
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For what little it's worth, I understood George's comment as supportive...

I could not find it again, but Wikipedia has a statement to the effect that the gravitational field CANNOT be associated with any particular component of the Einstein formulation...not the metric, not the Riemann curvature, not Christoffel symbol, etc,etc
and goes to say one entity cannot take precedence over all the others in defining/representing the gravitational field. In addition, Ben Crowell has previously posted in another discussion how the gravitational field representations, and the energy therein, can be subject to varying interpretations....lost that somewhere in my notes, still looking.

These are the kind of tidbits that add clarity:

That means extra terms come in due to the connection coefficients, and in certain special cases the extra terms have a simple interpretation in terms of "gravitational energy" being exchanged with ordinary matter-energy.
Again, PeterDonis, thanks for your time and effort....I picked up a lot of good information from your posts....
Mar1-12, 04:51 PM   #96
 
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To supplement George's comment from THE ROAD TO REALITY:

Peter explained that quote, I think, in earlier posts here. At least I 'got it'.

Penrose has a bit more detail immediately following George's excerpt [above]which I believe directly complements Peter's previous posts:

[for two massive bodies close together and at rest].....

.... there will be [negative] gravitational potential energy contribution that makes the total energy and therefore the total mass smaller than it would be if they are far apart. Ignoring much tinier energy effects, such a distortions of each body's shape due to the gravitational field of the other, we see that the total contributions from the actual energy momentum tensor T will be the same whether the two bodies are close together or far apart. Yet the total mass/energy will differ in the two cases and this difference would be attributed to the energy in the gravitational field itself [in fact a negative contribution, that is more sizeable when the bodies are close than when they are far apart.]
...Now let us consider that the bodies are in motion.....[he describes the Taylor-Hulse binary thingy]....The energy-momentum tensor in empty space is zero, so the gravitational wave energy has to be measured in some other way that is not locally attributable to an energy 'density'. Gravitational energy is a genuinely non-local entity. This does not imply there is no mathematical description of gravitational energy, however. Although I believe it is fair to say we do yet yet have a complete understanding of gravitational mass/energy, there is an important class of situations in which a very complete answer can be given. These situations are those referred to as asymptotically flat and they refer to gravitating systems that may be regarded as being isolated from the rest of the universe, essentially because of there very large distance from everything else. ....The work of Biondi...generalized by Sachs provided a clear cut mathematical accounting of the mass energy carried away from such a system in the form of gravitational waves and a conservation law for energy-momentum was accordingly achieved. This conservation law does not have a local character of that for non gravitational fields.....
Extending the above concepts, Penrose closes the chapter:

...There are general prescriptions for obtaining conservation laws for systems of interacting fields. These come from the Langrangian approach....very powerful,,,,despite the fact that it does not...directly SEEM to give us everything we need in the case of gravitation.....
[I even had some of the above highlighted from a few years ago....too bad I did not remember this source!]
Mar1-12, 05:56 PM   #97
 
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Quote by Naty1 View Post
Again, PeterDonis, thanks for your time and effort....I picked up a lot of good information from your posts....
You're welcome! Glad I was able to help.

Quote by Naty1 View Post
Extending the above concepts, Penrose closes the chapter:
Just to expand on this a bit, I believe Penrose is referring here to Noether's theorem: if the Lagrangian of a system has a symmetry, Noether's theorem shows how to construct a conserved current from that symmetry. "Energy" in this interpretation is the conserved current associated with time translation symmetry. Most of the spacetimes discussed in this thread where a useful definition of "total energy" can be made have time translation symmetry; but there are important spacetimes that don't (for example, the FRW spacetimes), which is why this method of defining energy "does not...directly SEEM to give us everything we need in the case of gravitation", as Penrose says.
Mar2-12, 04:36 AM   #98
 
Quote by PeterDonis View Post
Q-reeus: "I will assume when you write GW above it is not the wave but gravitational energy in a static field."
Then you assume wrongly; by "GW" I meant specifically "gravitational waves". I thought that was clear from context, but I suppose I should have spelled it out. Please re-read interpreting "GW" specifically as "gravitational waves".
But then it makes no sense. You say I should have known from context GW in #77 meant gravitational waves, not gravitational energy. If you take the trouble to trace back that discussion it was referencing to comparing possible pressure vs static field gravitational energy contributions - all in the context of that given in #45 & elaborated in #52. GW's were not involved (there were of course other discussions considering GW's role, but clearly distinct from this matter). So who's to blame for thinking you must logically have meant energy in a static field, not GW's? Maybe you had another entry in mind when writing that.
Q-reeus: "That position is 'my version of the EFE/SET in GR is Absolute Truth, if you find differently by any counterexample/counterargument whatsoever, you must be in error - end of story.'"
My position is that the *standard GR* version of the EFE/SET accounts for all the physics. So far you have given no counterexample to that claim...
Last bit is patently untrue, but I guess you forgot to insert 'that I acknowledge'.
I am not saying that your way of describing certain aspects of the physics is "wrong"; I'm only saying that it's limited to certain aspects of the physics.
Which just amounts to what I say above quoted. Any counterexample, e.g. in #45, cannot be true by definition, so why bother taking it seriously? The way you express that is a little less blatant: 'just apply the standard EFE/SET formula and all must be right. Counterexample X suggesting otherwise must thus be wrong'. This is your procedure to 'defeat' any counterargument, by referring back to the rote formula I complain about! No-win situation gauranteed. i will have another shot at breaking that cyclic dilemma in a later posting.
(1) The GR solutions for static or nearly static stars require pressure to contribute to the SET in the standard way--in other words, it's not enough just to put pressure into an equation of hydrostatic equilibrium, you also need to include pressure as a "source" on the RHS of the EFE. These solutions do a good job of predicting the observed masses and other properties of stars.
Is there actually observational evidence here? Would have thought pressure a negligible SET source in stars. Maybe neutron stars, but even there do we have convincing evidence it is needed to account presumably for maximum NS mass (less if pressure is SET source, than if not)? Have come across articles where it is admitted the eqn's of state within NS's are still not fully understood.
Mar2-12, 04:38 AM   #99
 
Quote by George Jones View Post
...Disembodied, because, from Ryder,

We cannot, then, identify a place or places, where where the gravitational field exists and carries energy, since whether the field carries energy also depends on the frame of reference. Gravitational energy is not localisable.

This means that gravitation energy cannot be included in the stress-energy-tensor field, as this is a mapping from spacetime into the space of tensors.
Precisely confirming my suspicions given in #59.
Mar2-12, 04:41 AM   #100
 
Quote by PeterDonis View Post
...In this case, the SET does *not* include any "gravitational field energy" (it's just the standard perfect fluid SET), but nevertheless it's commonly said that "gravitational field energy" needs to be taken into account in determining the externally measured mass M of the star.
(I've explained several times how the standard picture actually deals with this--the mass M is ultimately derived from the standard SET by solving the standard EFE, with no extra "source" terms for "gravitational field energy"--the latter just happens to be one way of describing the relationship between the mass M that appears in the metric and the standard SET that appears on the RHS of the EFE.)
Hope you can appreciate that from my pov the above is frustratingly empty. On the one hand, a clear statement that gravitational field energy Eg is specifically absent from the SET. But then go on to say it is one way of describing the relationship between measured M and the SET. But nowhere have I seen you attempt to pin down what is then gravitational "energy's" role in a 'way of describing'. What exactly is it that means anything given Eg is utterly absent from the SET? Curvature non-linearity? If so, how about just plainly say so and why, or if something else, say exactly what it is.
Mar2-12, 04:44 AM   #101
 
Quote by PeterDonis View Post
Q-reeus: "And you go on to say GW's are included somehow in the balance despite possessing zero SET contribution themselves."

What "balance" are you talking about? I said GWs carry away energy in the sense that they can later do work on a detector; and I said that the externally observed mass of the system that emits GWs decreases. But neither of those things affect the "balance" expressed in the energy conservation equation I gave, that the covariant divergence of the SET is zero.
Not energy balance per se - I have consistently acknowledged there is at least nominally a system "energy" balance. Try the 'balance' of total system *gravitating* mass (inclusive of all energy flows including GW's) discussed particularly in #50 and #54. You here in #83 (which in turn references back to #73) have imo clearly set a trap for yourself. Gravitationally collapsed system mass M - the externally observed Keplerian *gravitating* mass, declines by your admission above. Further, by your admission, the decline is owing to GW "energy" emission - which you state clearly is not a part of SET and contributes nothing to M. So please, no appeal to a rote formula here. Admit the inescapable, basic logic - *total* system *observed* mass M thus declines. If your 'answer' is to ignore this request, understand I will feel free to draw obvious conclusions. And recall in past postings you have specifically claimed M cannot decline if all matter+energy is included. Deny that and I will gladly furnish quotes to the contrary. This is relevant to the monopole GW issue btw.
Mar2-12, 08:46 AM   #102
 
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Q-reeus posts:

...But nowhere have I seen you attempt to pin down what is then gravitational "energy's" role in a 'way of describing'.

If you READ from posts 88 on....Tricky, my posted quotes, George Jones comments and quotes and Peter's comments explain it to the extent it can be....'non localizable', covarient derivative effects, non localizable,etc,etc ......

these are all complementary, not in conflict.

including these:

There is in fact no way to define a global energy-momentum vector in a general curved spacetime."
from Ryder
We cannot, then, identify a place or places, where where the gravitational field exists and carries energy, since whether the field carries energy also depends on the frame of reference. Gravitational energy is not localisable.
and from Penrose:
.... Although I believe it is fair to say we do yet yet have a complete understanding of gravitational mass/energy, there is an important class of situations in which a very complete answer can be given. These situations are those referred to as asymptotically flat......
I could quibble with Peter's comment about problems with energy theorems (in #91) being more 'philosophy' than physics.....but that's waaaaaaaaay too nit picky....

Q-Reeus...While I see why pervect opted out early, I am on the other hand happy to see your persistence:

" It is better to debate a question without settling it than to settle a question without debating it."
.......Joseph Joubert, the 18th century philosopher


I, for one, am 'outta' here....finally!!
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