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The conservation laws that we consider here are called dynamical because they explicitly involve the equations of motion. There exists also specific topological conservation laws, see e.g..
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This correspondence is one-to-one for gauge parameters that may depend on the linearized fields φi and that satisfy δξ(x,φi),Λ(x, φi) i≈lin0, i.e. zero for solutions φi of the linearized equations of motion. However, it has been proven in that this φ-dependence is not relevant in the case of Einstein gravity. Such a dependence will not be considered here.
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This correspondence is one-to-one for gauge parameters that may depend on the linearized fields φi and that satisfy δξ(x,φi),Λ(x, φi) i≈lin0, i.e. zero for solutions φi of the linearized equations of motion. However, it has been proven in that this φ-dependence is not relevant in the case of Einstein gravity. Such a dependence will not be considered here.
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