Manuscript XIX-A@1 · XIX-A.tex · section · e30d8062

Clock, lapse, and relational pullback

The scalar-clock lapse and the original spatial rods › Clock, lapse, and relational pullback · lines 472–522

XIX-A@1#eq:timelike, XIX-A@1#eq:clock-normal, XIX-A@1#eq:original-rods, XIX-A@1#eq:relmap, XIX-A@1#eq:rel-lapse

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Let have signature , and let be a smooth scalar with

The clock orientation is chosen so that increases to the future. Its future unit normal and raw lapse are

Thus and .

The lapse is neither the scalar value nor its normal derivative. It is a functional of the metric and the first derivatives of .

Let be the Laplace–Beltrami operator of the Riemannian metric induced on a -level set. The original rods satisfy

These are slice-elliptic equations, not spacetime wave equations. The original and modified choices in BFHPR (arXiv equations (28)–(35)) must be distinguished. The supplied Em02-E record explicitly selects the original rods CheungEm02E.

For a fixed background clock with , let

The relational lapse is

The fixed clock calibration in (eq:relmap) is part of this definition.

Displayed formulas in this passage

  • XIX-A@1#eq:timelike · line 476

  • XIX-A@1#eq:clock-normal · line 482

  • XIX-A@1#eq:original-rods · line 496

  • XIX-A@1#eq:relmap · line 509

  • XIX-A@1#eq:rel-lapse · line 516