Manuscript XX-B@1 · XX-B.tex · section · 56d708a5
The complete second-order classical field equations
The complete second-order classical field equations · lines 577–672
XX-B@1#eq:J, XX-B@1#eq:C, XX-B@1#eq:R2, XX-B@1#eq:Rscalar2, XX-B@1#eq:G2, XX-B@1#eq:U, XX-B@1#eq:T2, XX-B@1#eq:A, XX-B@1#eq:scalar2
This section supplies a finite coefficient algorithm for the quadratic Einstein–scalar terms. It also fixes what “through quadratic order” means. No nonlinear differential operator is being assigned a linear Green inverse.
Define
For the jet (eq:jet), the inverse metric coefficients are
The connection difference coefficients are
Thus
Put , . For ,
Write , , and . Then
For the scalar equation, define
Its complete second coefficient is
Displayed formulas in this passage
XX-B@1#eq:J · line 593
XX-B@1#eq:C · line 600
XX-B@1#eq:R2 · line 610
XX-B@1#eq:Rscalar2 · line 610
XX-B@1#eq:G2 · line 610
XX-B@1#eq:U · line 633
XX-B@1#eq:T2 · line 645
XX-B@1#eq:A · line 655
XX-B@1#eq:scalar2 · line 664
unlabeled · line 586