词条 | Stress–energy–momentum pseudotensor |
释义 |
In the theory of general relativity, a stress–energy–momentum pseudotensor, such as the Landau–Lifshitz pseudotensor, is an extension of the non-gravitational stress–energy tensor which incorporates the energy–momentum of gravity. It allows the energy–momentum of a system of gravitating matter to be defined. In particular it allows the total of matter plus the gravitating energy–momentum to form a conserved current within the framework of general relativity, so that the total energy–momentum crossing the hypersurface (3-dimensional boundary) of any compact space–time hypervolume (4-dimensional submanifold) vanishes. Some people (such as Erwin Schrödinger{{citation needed|date=October 2015}}) have objected to this derivation on the grounds that pseudotensors are inappropriate objects in general relativity, but the conservation law only requires the use of the 4-divergence of a pseudotensor which is, in this case, a tensor (which also vanishes). Also, most pseudotensors are sections of jet bundles, which are now recognized as perfectly valid objects in GR. Landau–Lifshitz pseudotensorThe use of the Landau–Lifshitz pseudotensor, a stress–energy–momentum pseudotensor for combined matter (including photons and neutrinos) plus gravity,[1] allows the energy–momentum conservation laws to be extended into general relativity. Subtraction of the matter stress–energy–momentum tensor from the combined pseudotensor results in the gravitational stress–energy–momentum pseudotensor. RequirementsLandau and Lifshitz were led by four requirements in their search for a gravitational energy momentum pseudotensor, :[1]
DefinitionLandau & Lifshitz showed that there is a unique construction that satisfies these requirements, namely where:
VerificationExamining the 4 requirement conditions we can see that the first 3 are relatively easy to demonstrate:
Cosmological constantWhen the Landau–Lifshitz pseudotensor was formulated it was commonly assumed that the cosmological constant, , was zero. Nowadays we don't make that assumption, and the expression needs the addition of a term, giving: This is necessary for consistency with the Einstein field equations. Metric and affine connection versionsLandau & Lifshitz also provide two equivalent but longer expressions for the Landau–Lifshitz pseudotensor:
[2]
[3] This definition of energy–momentum is covariantly applicable not just under Lorentz transformations, but also under general coordinate transformations. Einstein pseudotensorThis pseudotensor was originally developed by Albert Einstein.[4][5] Paul Dirac showed[6] that the mixed Einstein pseudotensor satisfies a conservation law Clearly this pseudotensor for gravitational stress–energy is constructed exclusively from the metric tensor and its first derivatives. Consequently, it vanishes at any event when the coordinate system is chosen to make the first derivatives of the metric vanish because each term in the pseudotensor is quadratic in the first derivatives of the metric. However it is not symmetric, and is therefore not suitable as a basis for defining the angular momentum. See also
Notes1. ^1 2 Lev Davidovich Landau and Evgeny Mikhailovich Lifshitz, The Classical Theory of Fields, (1951), Pergamon Press, {{ISBN|7-5062-4256-7}} chapter 11, section #96 2. ^Landau–Lifshitz equation 96.9 3. ^Landau–Lifshitz equation 96.8 4. ^Albert Einstein Das hamiltonisches Prinzip und allgemeine Relativitätstheorie (The Hamiltonian principle and general relativity). Sitzungsber. preuss. Acad. Wiss. 1916, 2, 1111–1116. 5. ^Albert Einstein Der Energiesatz in der allgemeinen Relativitätstheorie. (An energy conservation law in general relativity). Sitzungsber. preuss. Acad. Wiss. 1918, 1, 448–459 6. ^P.A.M.Dirac, General Theory of Relativity (1975), Princeton University Press, quick presentation of the bare essentials of GTR. {{ISBN|0-691-01146-X}} pages 61—63 References
2 : Tensors|Tensors in general relativity |
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