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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.(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 |
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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: 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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From page 131 of MTW's Gravitation |
| Mar1-12, 02:01 PM | #90 |
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| Mar1-12, 02:11 PM | #91 |
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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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| Mar1-12, 02:30 PM | #93 |
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"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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| 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: |
| 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]..... |
| Mar1-12, 05:56 PM | #97 |
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| Mar2-12, 04:36 AM | #98 |
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| Mar2-12, 04:38 AM | #99 |
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| Mar2-12, 04:41 AM | #100 |
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| Mar2-12, 04:44 AM | #101 |
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| Mar2-12, 08:46 AM | #102 |
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Q-reeus posts:
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: 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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