High-contrast homogenization: Entry.Multiscale.OneGrid.ExponentAndLossArithmetic #
Imported from the Apache-2.0 HighContrastHomogenization development at commit
7a13dbcd8d6609264a713373f5c69ceeac870472.
Exponent And Loss Arithmetic #
This module proves the exponent arithmetic of the one-grid propagation and the algebra of the
log-determinant loss it is applied to. It establishes the numeric facts about Q = π¬(d,Ξ³)
and the contraction, span and averaging coefficients, the elementary exponential inequalities
and the geometric profile weights; and it proves additivity of the log-determinant loss, its
comparison with the synchronized loss, and the synchronized multiplicity bound. It serves
p.fixed.geometry.one.grid.propagation.
Printed exponent and coefficient arithmetic #
Group A of the printed proof (p.fixed.geometry.one.grid.propagation): the numeric facts about
Q = π¬(d,Ξ³), the contraction, span and averaging coefficients, the elementary
exponential inequalities and the geometric profile weights.
Part of the proof of the statement in
HCPoly/Entry/Statements/OneGridPropagation.lean. Conventions of the group:
q = π¬(πͺ) is Geometry.explicitRoundedGrid jStar metric at every loss, history, profile and drift;
metric (not m) names the positive matrix, because m, n, mβ are generations; the
source lower scale e.source.lower.scale is carried exactly by the
module HCPoly/Entry/OneGridPropagation.lean; this group's stronger internal
algebraic and history lemmas omit an unused threshold, and this group's generic
integration helpers take finiteness, integrability or measurability inputs that are proved
at their actual use sites, not extra premises of the printed proposition.
Group A. The printed exponent and coefficient arithmetic #
(p.fixed.geometry.one.grid.propagation)
3^{-β
(1-Ξ³)h} β€ 3^{-3} < 1/8 for every natural h β₯ 2Q
(p.fixed.geometry.one.grid.propagation). This is the
drift half of the contraction.
The printed contraction coefficient
3^{-ΒΌ(1-Ξ³)h} + 2^{Q-1}(3^dQ)^Q 3^{-Qdh/2} β€ 3^{-6} + Β½Β·3^{-12} < 1/8, for every natural
h β₯ 2Q (p.fixed.geometry.one.grid.propagation).
The span-2Q coefficient 2^{Q-1}(3^dQ)^Q 3^{-dQΒ²} β€ 1/8 used in Step 4, where the
recurrence is applied with the fixed span 2Q so that the constants do not depend on the
possibly larger h (p.fixed.geometry.one.grid.propagation).
QΒ·3^{d/2}(1 + (2d)^{1/Q}) β€ 3^d Q for d β₯ 2, Q β₯ 2
(p.fixed.geometry.one.grid.propagation): the step that
turns the recurrence's printed prefactor into the contraction's.
The geometric tail of the profile weights is bounded by a constant depending only on Ξ³
(p.fixed.geometry.one.grid.propagation, "the geometric sum is bounded by C").
Log-determinant loss algebra and the multiplicity bound #
Group B of the printed proof (p.fixed.geometry.one.grid.propagation): additivity of the
log-determinant loss, its comparison with the synchronized loss, and conjunct 7,
e.fixed.geometry.synchronized.multiplicity.
Part of the proof of HCPoly/Entry/Statements/OneGridPropagation.lean. Conventions of this group:
q = π¬(πͺ) is Geometry.explicitRoundedGrid jStar metric at every loss, history, profile and drift;
metric (not m) names the positive matrix, because m, n, mβ are generations; the
source lower scale e.source.lower.scale is carried exactly by the
HCPoly/Entry/OneGridPropagation.lean; this group's stronger internal
algebraic and history lemmas omit an unused threshold, and this group's generic
integration helpers take finiteness, integrability or measurability inputs that are proved
at their actual use sites, not extra premises of the printed proposition.
Group B. Log-determinant loss algebra and the multiplicity bound #
(p.fixed.geometry.one.grid.propagation)
Ξ^q_{j-h,m+h} β€ ΞΜ^q_h(m) for m < j β€ m+h (p.fixed.geometry.one.grid.propagation).
Taking j = m+h gives
the Ξ^q_{m,m+h} β€ ΞΜ^q_h(m) used in Step 3.
Conjunct 7, e.fixed.geometry.synchronized.multiplicity
(p.fixed.geometry.one.grid.propagation): expand the synchronized losses into adjacent
increments, observe that the smallest
index is at least j_* and that each increment occurs at most h times.