HolderGagliardoRadial #
Ported from scottnarmstrong/Superdiffusion at 7f20476385d4af418f110303085ad0740c9eba46. Module imports, support namespace and local option directives adapted for Lean Pool.
The radial kernel integral ∫_{B(x,R)} |x-y|^{-β} dy #
Nothing here imports that file, nothing here claims the anchor, and nothing here is a frozen statement.
The target #
This file proves the sharp-in-R bound, with the explicit constant, in the
ambient supremum metric of Vec d:
∫_{B(x,R)} |x-y|^{-β} dy ≤ ( 2^d 3^β / (1 - 3^{β-d}) ) · R^{d-β}
for 0 < β < d .
Everything is ℝ≥0∞-valued, so no integrability side condition is needed.
The mechanism #
The ball is covered by the point x (where the integrand is the junk value
0^{-β} = 0) together with the triadic annuli A_i = { R·3^{-i-1} ≤ |x-y| < R·3^{-i} }. On A_i the integrand is at most (R·3^{-i-1})^{-β} and |A_i| ≤ (2·R·3^{-i})^d, so the i-th contribution is T_i = (^{-i-1})^{-β} (2^{-i})^d, a geometric sequence of ratio 3^{β}/3^{d} < 1.
References #
- ABK26,
t.regularityStep 4, (the two seminorm comparisons stated without proof). - ABK26, (the fractional Sobolev seminorm) (the Hölder seminorm and the
p = ∞convention).
1. The triadic annuli around a point #
The radius R · 3^{-i} of the i-th triadic shell.
Equations
- Algsuperdiff.Section4.Provider.Regularity.annulusRadius R i = R * 3 ^ (-↑i)
Instances For
The i-th triadic annulus { R·3^{-i-1} ≤ |x-y| < R·3^{-i} } around x.
Equations
- One or more equations did not get rendered due to their size.
Instances For
The annuli cover the punctured ball. The centre is separated out
because the integrand takes the junk value 0^{-β} = 0 there.
2. The geometric sequence of shell contributions #
The common ratio 3^β / 3^d of the shell contributions.
Equations
- Algsuperdiff.Section4.Provider.Regularity.annulusRatio d beta = 3 ^ beta / 3 ^ d
Instances For
3. The shell estimate #
4. The ball estimate #
C_rad(d,β) = 2^d · 3^β · (1 - 3^{β-d})^{-1}, in the closed form the shell
sum produces: (R/3)^{-β}(2R)^d divided by 1 - 3^β/3^d, at R = 1.
Equations
- Algsuperdiff.Section4.Provider.Regularity.radialKernelConst d beta = (1 / 3) ^ (-beta) * 2 ^ d / (1 - Algsuperdiff.Section4.Provider.Regularity.annulusRatio d beta)
Instances For
The radial kernel integral on a ball.
For 0 < β < d, in the ambient supremum metric,
∫_{B(x,R)} |x-y|^{-β} dy ≤ C_rad(d,β) · R^{d} · R^{-β}.
5. The ℝ≥0∞-native form #
Points are null in Vec d once d ≥ 1 ({x} is the closed ball of radius
0, of volume (2·0)^d).
The radial kernel integral, with the ℝ≥0∞-native kernel ‖x-y‖ₑ^{-β}.
The two kernels differ only on the diagonal — where the real junk value is
0^{-β} = 0 and the ℝ≥0∞ value is ⊤ — which is null because 0 < β < d
forces 1 ≤ d.