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energy in GR |
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| Jun11-12, 05:43 PM | #18 |
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energy in GRBut many non-conserved quantities are nonetheless physically meaningful. |
| Jun11-12, 05:50 PM | #19 |
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| Jun11-12, 05:57 PM | #20 |
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| Jun11-12, 06:09 PM | #21 |
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| Jun11-12, 06:26 PM | #22 |
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| Jun11-12, 07:07 PM | #23 |
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I think you may be confusing events in the spacetime manifold with their coordinates. |
| Jun11-12, 08:00 PM | #24 |
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"The principle of relativity" by Einstein and others,
"That this requirement of general covariance, which takes away from space and time the last remnant of physical objectivity, is a natural one, will be seen from the following reflexion". See Rovelli "Quanyum Gravity" p.74 "The disapearence of spacetime". |
| Jun11-12, 08:41 PM | #25 |
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Note this refers to "space and time", not "spacetime". My interpretation of this is therefore "the objectivity of space" and "the objectivity of time", certainly not "the objectivity of spacetime". |
| Jun11-12, 08:54 PM | #26 |
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| Jun11-12, 10:17 PM | #27 |
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One is a local statement, and one is a large-scale statement. The local statement of conservation of energy can be expressed as a differential equation, the continuity equation: ∂/∂t ρ = - ∇.j where ρ is the energy density, and j is the energy flux (transfer of energy per unit cross-sectional area per unit time). Now, in flat spacetime, we can define Etotal = ∫ρ dV where the integral is over some closed surface S. Then energy conservation can be expressed as: The rate of change of Etotal is equal to the energy flux into surface S, which can be written as the integral equation: d/dt ∫ρ dV = ∫j.dS The left-side is a volume integral over the volume enclosed by the surface, and the right-side is a surface integral over the surface. In flat spacetime, the differential form of the law of conservation of energy is equivalent to the integral form. In curved spacetime, the local form continues to hold, but the integral form doesn't necessarily hold except in special circumstances. I don't know what the best way to describe why not, but here's a hand-wavy explanation: One problem with the integral form, which you can see immediately, is that it involves on the left-hand side, a derivative with respect to t. So there must be a notion of time t common to the entire region enclosed by the surface S in order to make sense of the integral form. In contrast, the local form only requires a local notion of t,which always exists by considering a local inertial frame. Anyway, energy density is always defined in GR, but total energy in a region may not be well-defined. |
| Jun11-12, 10:40 PM | #28 |
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A quote: |
| Jun12-12, 05:04 PM | #29 |
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I think you can give definite meaning to the matter SET if you use material reference systems. Gravity on the other hand is a bit more tricky...you can always go to a system in free fall and get rid of the grav field... that is not an active diff transformation...so yeah I agree what was said before about defining energy-momentum density for the grav field. |
| Jun12-12, 05:18 PM | #30 |
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| Jun12-12, 05:47 PM | #31 |
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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 |
| Jun12-12, 05:52 PM | #32 |
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The stress-energy tensor is well defined at every point in spacetime. |
| Jun12-12, 06:07 PM | #33 |
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Sam |
| Jun12-12, 06:17 PM | #34 |
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Commutators of vector fields are preserved by push-forwards of diffeomporphisms, so push-forwards preserve Lie derivatives and thus Killing's equation. |
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