Source-scale reduction for the remainder index. The corrected
indexing fixes the remainder at Jcut β; the estimates below retain that exact exponent.
The actual tensor remainder at the corrected index Jcut.
Equations
- AVenhance.Infra.Section4.dmFrozenTailTerm I hΦ m κ T n z i = ∑ j : Fin 2, ∑ k : Fin 2, I.Amnr hΦ m κ n T (AVenhance.Jcut β) z.1 z.2 i j k * I.qMNR κ m n (AVenhance.Jcut β) z.1 j k
Instances For
d_m source split with its first vector term left explicit. The
first term is (Jhat_m - J_m) Σ_l xihat_l (∇X_l∘X_l⁻¹)∇T; the second is
the literal A_{m,n,Jcut} q_{m,n,Jcut} remainder.
Equations
- AVenhance.Infra.Section4.dmFrozenSource I hΦ m κ T first z = first z + ∑ n ∈ Finset.range (AVenhance.Nstar β), AVenhance.Infra.Section4.dmFrozenTailTerm I hΦ m κ T n z
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The Jhat_m - J_m first term of d_m:
Σ_l ξ̂_l F_lᵀ (JHat - 𝒥) F_l ∇T, with the flow Jacobian F_l on both sides of
the flux gap (§9.4).
Equations
- One or more equations did not get rendered due to their size.
Instances For
Convexity of the cutoff average for vector-valued summands.
Pointwise bound on the first summand from an active-window flow bound and a uniform flux-gap bound.
The first term has the Piola-conjugated flux gap as multiplier. Its
analytic inputs are a pointwise bound L on the active flow Jacobians and the
source L² bound for the temperature gradient; the flux gap is supplied by the
corrected Section 3 Jhat estimate.
Specialization of the preceding first-term estimate to the actual Section 3 coefficients. The
paper's J_m is the flux, so the corrected
flux_sub_Jhat_norm_le estimate bounds the matrix multiplier directly.
One coordinate summand in the A_{m,n,Jcut} q_{m,n,Jcut}
vector tail.
Equations
- AVenhance.Infra.Section4.dmFrozenTailCoordinateTerm I hΦ m κ T n i j k z p = if i = p then I.Amnr hΦ m κ n T (AVenhance.Jcut β) z.1 z.2 i j k * I.qMNR κ m n (AVenhance.Jcut β) z.1 j k else 0
Instances For
L² multiplication by a scalar bounded in absolute value.
Decomposition of the vector tail into its eight single-coordinate products.
Actual tail estimate from the (k,ell)=(0,0) instance of the
source p.Amnr.bounds and the corrected geometric qMNR bound. The
AMNR input is the tensor-valued source estimate; only its finite coordinate
projections are used here.
L² triangle estimate for the d_m split.
Complete d_m source estimate after inserting the actual J_m
flux first term, the corrected Section 3 flux gap, and the (0,0) p.Amnr
source bound for every tail mode. The ratio hypothesis is the Section 3
smallness input used to discard the remaining mode factor R^n ≤ 1.
Transfer of the first d_m term from the corrected 4δ exprat scale
to the Jcut exponent. The proof uses N ≤ 3J and J ≤ 4N, which hold
for the large cutoff once Jcut ≥ 2.
Assembly of the corrected first-term transfer and the Jcut remainder
sum. This is the scalar source split used before the spacetime L² triangle
inequality for the vector-valued d_m.
p.dm.bounds after the source parameter inequalities are supplied.
The first scalar premise is the four-delta flux transfer; the second is
the p.Amnr/qMNR scale for the Jcut tail. The actual L² estimate
and its J_m = flux identification are proved by
dm_frozenSource_eLpNorm_le_of_section3_pAmnr above.