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
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