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

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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

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