Manuscript V@1 · V.tex · section · e7ddf37d

Option A inverse and its constraints

Contrast: the Newton–wave cubic form › Option A inverse and its constraints · lines 3080–3141

V@1#eq:RA

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For , use the stress from Section sec:external and its polarization

Differentiation gives

Thus it is conserved for free scalar solutions. Take these solutions to have Schwartz Cauchy data. On bounded time intervals the polarized sources are smooth Schwartz functions in space.

Fix the Newton inverse

with its locally integrable multiplier and no added zero-supported Fourier distribution.

For a conserved source , let

Specify trace-reversed metric data by

Let denote trace reversal. Define

Then .

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