Coarse-graining support: Support.HighContrast.EntryScale.BadMaximal.P1 #
Imported from the Apache-2.0 CoarseGraining development at commit
c7ddd76c08ade64fed1b8d2ca51be14dfee8deb4.
Bad maximal observable #
This file isolates the manuscript bad-event maximal slot from the scalar post-split bound used in the no-drop response estimate.
Nonnegativity of the bad-event truncation for a nonnegative observable.
The bad-event truncation is bounded by the original nonnegative observable.
Sharp good/bad split of a nonnegative maximal observable: on the good event
{M <= 1} the observable equals min M 1, and on the bad event {1 < M} it
is paid by the bad-event truncation at first power (with the harmless extra
min M 1 = 1). This is the first-power replacement for the crude split
M <= 1 + badEventTruncation M.
First-power good/bad split of a nonnegative maximal factor against a
nonnegative response: M * J is paid by min M 1 * J on the good event and
by badEventTruncation M * J on the bad event. No squaring and no
deterministic cap on J is introduced.
The bad-event truncation of an a.e. strongly measurable observable is a.e. strongly measurable.
The deterministic weighted drift supremum in the manuscript split of
\mathcal M_m.
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Instances For
The stochastic/subthreshold/deterministic random envelope that appears after the manuscript positive-part split. This is not the source observable itself; it is the pointwise upper envelope whose square is later integrated.
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Instances For
Any scale term in the deterministic drift split is selected by the drift supremum over the high-scale window.
The operator norm of the C-star positive part is bounded by the operator norm of the original full-block matrix.
This is the local analytic bridge behind the manuscript step
|(X)_+| ≤ |X|. It is proved by diagonalizing self-adjoint matrices and
using unitary invariance of the C-star norm; non-self-adjoint matrices have
zero positive part by the Mathlib definition.
The literal terminally-normalized spectral positive part on one block.
This uses the library's normalized full-block fluctuation matrix for
Ahom_m^{-1/2} (bfA(Q) - Ahom_m) Ahom_m^{-1/2} and mathlib's C-star
positive part M⁺.
Equations
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