Manuscript XX-B@1 · XX-B.tex · section · 56d708a5

Perturbations, clock, and lapse

The complete background and classical prescription › Perturbations, clock, and lapse · lines 298–347

XX-B@1#eq:jet, XX-B@1#eq:clock, XX-B@1#eq:raw-lapse, XX-B@1#eq:clock-jet, XX-B@1#eq:theta

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Retain the factorial convention

The classical coefficient fields are smooth and have a common compact spatial support on each compact time interval used in the observable calculation. They need not solve the perturbed Euler equations.

The field-dependent cosmic label is

The raw matter-scalar lapse, on the positive branch, is

It is not silently replaced by the lapse calibrated to . The two normalizations satisfy

Let invert the clock at fixed spatial coordinate. Then

All inverse coefficients are evaluated at .

Displayed formulas in this passage

  • XX-B@1#eq:jet · line 301

  • XX-B@1#eq:clock · line 313

  • XX-B@1#eq:raw-lapse · line 318

  • XX-B@1#eq:clock-jet · line 332

  • XX-B@1#eq:theta · line 332

  • unlabeled · line 326