2002
DOI: 10.1088/0264-9381/19/2/304
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Symmetry properties under arbitrary field redefinitions of the metric energy–momentum tensor in classical field theories and gravity

Abstract: We derive a generic identity which holds for the metric (i.e. variational) energy–momentum tensor under any field transformation in any generally covariant classical Lagrangian field theory. The identity determines the conditions under which a symmetry of the Lagrangian is also a symmetry of the energy–momentum tensor. It turns out that the stress tensor acquires the symmetry if the Lagrangian has the symmetry in a generic curved spacetime. In this sense, a field theory in flat spacetime is not self-contained.… Show more

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Cited by 14 publications
(49 citation statements)
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“…The trivial gauge invariant Lagrangian L = 0, is the only gauge invariant expression. This is the expected result because spin-2 is well known to have an action which is gauge invariant only up to a surface term [9,6]. We can find this surface term by using integration by parts, leaving us with a total divergence and some remaining terms,…”
Section: A Procedures For Gauge Invariant Lagrangian Formulationsupporting
confidence: 52%
“…The trivial gauge invariant Lagrangian L = 0, is the only gauge invariant expression. This is the expected result because spin-2 is well known to have an action which is gauge invariant only up to a surface term [9,6]. We can find this surface term by using integration by parts, leaving us with a total divergence and some remaining terms,…”
Section: A Procedures For Gauge Invariant Lagrangian Formulationsupporting
confidence: 52%
“…(65) (10) is not gauge invariant. In fact, one can prove a general theorem [12] that the energy momentum tensor for the spin-2 field cannot be made gauge invariant for any choice of ψ cpq . This raises serious questions about whether the resulting theory after infinite iteration will possess any trace of the original gauge symmetry.…”
Section: Action and Energy Momentum Tensor For The Spin-2 Fieldmentioning
confidence: 99%
“…A possible source of a further constraint is divergence of eq. (40). It may be shown by a direct calculation that if the equations (39) and (40) hold throughout the spacetime and if the five constraints are satisfied everywhere, then divergence of eq.…”
Section: The Four-dimensional Casementioning
confidence: 99%
“…(55) do not generate further constraints since their divergence vanishes identically providedR µν = 0 and π µν ;ν = 0. Secondly, one takes the limit m → 0 in the equations of motion (39) and (40). Since the scalar χ has already been eliminated, the resulting field equations,R µν = 0 and (55), represent the full set of solutions rather than a special class; the five constraints hold.…”
Section: Massless Spin-two Field In Hjfmentioning
confidence: 99%
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