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Volumn 52, Issue 1, 2011, Pages

Noether symmetries, energy-momentum tensors, and conformal invariance in classical field theory

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EID: 79551519980     PISSN: 00222488     EISSN: None     Source Type: Journal    
DOI: 10.1063/1.3532941     Document Type: Article
Times cited : (30)

References (52)
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    • An improvement is the addition to the energy-momentum tensor of a functional of the fields with identically vanishing divergence.
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    • To our knowledge, these identities were obtained in the language of mechanics by Kiyoshi Kamimura, in the early 1980s, by direct computation, and never published. A particular case of, for variations satisfying the Noether condition-see below-was written in Ref. 15, Eq.. We thank for pointing this out to us.
    • Salisbury D. To our knowledge, these identities were obtained in the language of mechanics by Kiyoshi Kamimura, in the early 1980s, by direct computation, and never published. A particular case of, for variations satisfying the Noether condition-see below-was written in Ref. 15, Eq.. We thank for pointing this out to us.
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    • As stated in Introduction, we only consider active variations on the fields. Any transformation of the coordinates-passive transformation-is rewritten as an active one.
    • As stated in Introduction, we only consider active variations on the fields. Any transformation of the coordinates-passive transformation-is rewritten as an active one.
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    • This sufficient condition may be further restricted in some cases if some boundary conditions are imposed on the acceptable solutions. See also Ref. 18 for a geometric characterization of on shell symmetries.
    • This sufficient condition may be further restricted in some cases if some boundary conditions are imposed on the acceptable solutions. See also Ref. 18 for a geometric characterization of on shell symmetries.
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    • Rosenfeld's contribution, which has been overlooked for a long time, has recently resurfaced thanks to the work of D. Salisbury and it is discussed in Ref. 26.
    • Rosenfeld's contribution, which has been overlooked for a long time, has recently resurfaced thanks to the work of D. Salisbury and it is discussed in Ref. 26.
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    • σ. This restriction will be lifted in Sec. IVC.
    • Note, however, that we restrict here the covariant behavior of the fields (scalars, vectors, tensors) for we do not allow them to be densities. For instance, our scalars here transform as. This restriction will be lifted in Sec. IVC.
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    • dg→η = 0, the quantities need not vanish.
    • dg→η = 0, the quantities need not vanish.
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    • Notice that here we only analyze spacetime conformal transformations, always within the active view. Sometimes the same language is used for Weyl transformations, which are not spacetime transformations. Weyl symmetries, which can be rigid or gauge, are dealt with in Ref. 10.
    • Notice that here we only analyze spacetime conformal transformations, always within the active view. Sometimes the same language is used for Weyl transformations, which are not spacetime transformations. Weyl symmetries, which can be rigid or gauge, are dealt with in Ref. 10.
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    • μν must be taken antisymmetric in such indices. This is the reason of the factor 1/2.
    • μν must be taken antisymmetric in such indices. This is the reason of the factor 1/2.
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    • μ)2 is considered
    • μ)2 is considered
  • 48
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    • Note
    • The assumptions made in Ref. 44 exclude our example.
  • 49
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    • Note
    • It is a tensor density of weight 1 because the Lagrangian is a scalar density.
  • 50
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    • Note
    • Since the background is fixed, there is no longer the gauge symmetry of diffeomorphism invariance. A residual, nongauge, subgroup of diffeomorphisms can still realize Noether symmetries, as we shall see.
  • 51
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    • Note
    • Conserved or covariantly conserved is the same for a vector density, with the standard Riemmanian connection.
  • 52
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    • f depending on the derivatives of the fields, since these derivatives become covariant derivatives upon covariantization.
    • f depending on the derivatives of the fields, since these derivatives become covariant derivatives upon covariantization.


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