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
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 .
Displayed formulas in this passage
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