Manuscript XI-A-ST@1 · XI-A-ST.tex · section · c3f0929d

The quadratic normalization

The signed action and its Euler derivatives › The quadratic normalization · lines 793–881

XI-A-ST@1#rest:euler, XI-A-ST@1#eq:eexact, XI-A-ST@1#eq:eexp, XI-A-ST@1#eq:Ephiexact, XI-A-ST@1#eq:scalar-switch, XI-A-ST@1#eq:sourcedivergence, XI-A-ST@1#sec:noether

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The invariant metric Euler density is

It contains no derivatives of .

By contrast, the scalar Euler density is

Equivalently,

where

Finally,

Proof. The formulas are XI-A :euler and :scalar-switch CheungXIA. Combining (eq:stressvariation) with gives (eq:eexact); no metric integration by parts in the matter action is involved. Scalar integration by parts instead gives (eq:Ephiexact), and hence (eq:scalar-switch). The identity gives (eq:sourcedivergence). All operations are completion-chart operations and transport by Lemma lem:transfer.

The action is fixed before its derivative is projected. The classical cubic and quartic Einstein coefficients supply and . Because (eq:eexact) contains , a covariance check through order must retain the required order-three metric curvature data. A premature order-two truncation of the pulled-back metric is not sufficient.

identities and tensor-density covariance

correct adjoint operator

Displayed formulas in this passage

  • XI-A-ST@1#eq:eexact · line 798

  • XI-A-ST@1#eq:eexp · line 798

  • XI-A-ST@1#eq:Ephiexact · line 815

  • XI-A-ST@1#eq:scalar-switch · line 830

  • XI-A-ST@1#eq:sourcedivergence · line 839

  • unlabeled · line 824

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