Coarse-graining support: #
Support.Deterministic.ConstantCoefficientDirichletBesov.StandardProjectionIncrementEnergy
Imported from the Apache-2.0 CoarseGraining development at commit
c7ddd76c08ade64fed1b8d2ca51be14dfee8deb4.
Energy bounds for standard martingale increments #
This file records the local Jensen step needed for the boundary-budget
construction: a child-minus-parent average is controlled by the L² energy of
the field measured relative to the parent average on that child.
A child-average jump is controlled coordinatewise by the child L²
energy relative to the parent average.
Pointwise form for a martingale increment on a child cube: the squared increment value is paid by the child energy relative to the parent average.
The child-energy sum relative to a parent average is controlled by the
ordinary vector L² fluctuation on the parent. The factor 3^d comes from
summing normalized child averages rather than averaging over the children, and
the factor d comes from comparing the Euclidean coordinate sum to the ambient
Pi norm used by cubeLpNorm.
Summed over all depth-m parents, the parent child-energy budgets are
controlled by the ordinary standard positive depth average.
If the point lies in a depth-m parent, the pointwise martingale
increment at scale m + 1 is controlled by the finite sum of the child
energies of that parent.
Local overlap version of the child-energy budget. When the overlap cube
does not leave a depth-m parent, the fluctuation of the m + 1 martingale
increment is paid by the finite child-energy sum of that parent.
Depth-m parents whose standard cubes meet a fixed overlap cube. This
is the local-neighbor family needed for the true finite-overlap summation.
Equations
Instances For
Pointwise local-neighbor version: on an overlap cube contained in Q, a
martingale increment is paid by child energies of only those depth-m parents
which meet that overlap cube.
Overlap-fluctuation local-neighbor budget for one martingale increment.