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
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