For a measurable weight ω:Rd→R\omega:\mathbb R^d\to\mathbb R, define

G(x)=∫1/22∣ω(sx)∣ ds,G∗(r)=sup⁡∣x∣=rG(x).G(x)=\int_{1/2}^{2}|\omega(sx)|\,ds, \qquad G^*(r)=\sup_{|x|=r}G(x).

The radial-line growth condition is

∫0∞G∗(r)1+r2 dr<∞.\int_0^\infty\frac{G^*(r)}{1+r^2}\,dr<\infty.
Geometric meaning

The first average smooths the weight along a short radial segment; the spherical supremum then records the worst direction at radius rr. The final integral measures whether these worst directional masses can be summed over scales.

One-dimensional comparison

For d=1d=1, the growth integral is comparable, up to absolute constants, to ∫R∣ω(t)∣/(1+t2) dt\int_{\mathbb R}|\omega(t)|/(1+t^2)\,dt, the condition in the classical .

Role of line porosity

When ω\omega is assembled from cubes meeting a , the controls G∗G^* on every .

References
  1. Alex Cohen, “Fractal uncertainty in higher dimensions,” 2024. arXiv record. Relevant: equations (1.9)–(1.13).