Finite source-Q weighted derivatives and telescoping #
This module closes the finite, source-level calculus behind Suzuki Proposition
9.3(iii) and Proposition 9.4(vi), specialized to κ = 1, β = 2.
The base layer is kept separate. On 2 < s < 3, its weighted derivative is
-1; this is the term which combines with the even-layer derivatives to recover
the prescribed history Q(s-1) = A_m/(s-1). Above 3, the ordinary layer
recurrences telescope, leaving only the last even layer.
The exceptional f₁ derivative on the first source strip. This is the
base term used in the 2 < s < 3 finite-Q equation.
Above the support endpoint of f₁, its weighted derivative is zero.
The ordinary recursive weighted derivative, stated separately from the exceptional base layer.
The even predecessors of the first m odd layers are exactly the first
m even layers with the terminal even layer removed. This is the finite
index telescope in Proposition 9.3(iii).
The predecessors of the first m even layers are exactly the first m
odd layers.
On the missing window 2 < s < 3, the finite source prefix satisfies the
exact weighted delay equation with no residual. The -1 from f₁ is essential:
it turns 1 + T_{2m-1}(s-1) into the prescribed history A_m/(s-1).
Above the common differentiability threshold 3, all recursive layers
differentiate and telescope; only the last even layer remains.
Unified finite telescoping equation away from the genuine source kink
s = 3. The residual is exactly suzukiProposition118SourceQTerminal.