English

Triangular Constellations in Fractal Measures

Fluid Dynamics 2015-06-19 v1 Statistical Mechanics

Abstract

The local structure of a fractal set is described by its dimension DD, which is the exponent of a power-law relating the mass N{\cal N} in a ball to its radius ϵ\epsilon: NϵD{\cal N}\sim \epsilon^D. It is desirable to characterise the {\em shapes} of constellations of points sampling a fractal measure, as well as their masses. The simplest example is the distribution of shapes of triangles formed by triplets of points, which we investigate for fractals generated by chaotic dynamical systems. The most significant parameter describing the triangle shape is the ratio zz of its area to the radius of gyration squared. We show that the probability density of zz has a phase transition: P(z)P(z) is independent of ϵ\epsilon and approximately uniform below a critical flow compressibility βc\beta_{\rm c}, but for β>βc\beta>\beta_{\rm c} it is described by two power laws: P(z)zα1P(z)\sim z^{\alpha_1} when 1zzc(ϵ)1\gg z\gg z_{\rm c}(\epsilon), and P(z)zα2P(z)\sim z^{\alpha_2} when zzc(ϵ)z\ll z_{\rm c}(\epsilon).

Keywords

Cite

@article{arxiv.1405.0572,
  title  = {Triangular Constellations in Fractal Measures},
  author = {Michael Wilkinson and John Grant},
  journal= {arXiv preprint arXiv:1405.0572},
  year   = {2015}
}

Comments

4 pages, 1 figure

R2 v1 2026-06-22T04:05:13.206Z