English

Catastrophe conditions for vector fields in $\mathbb R^n$

Mathematical Physics 2023-10-24 v1 Dynamical Systems math.MP

Abstract

Practical conditions are given here for finding and classifying high codimension intersection points of nn hypersurfaces in nn dimensions. By interpreting those hypersurfaces as the nullclines of a vector field in Rn\mathbb R^n, we broaden the concept of Thom's catastrophes to find bifurcation points of (non-gradient) vector fields of any dimension. We introduce a family of determinants Bj{B}_j, such that a codimension rr bifurcation point is found by solving the system B1=...=Br=0{B}_1=...={B}_r=0, subject to certain non-degeneracy conditions. The determinants Bj{B}_j generalize the derivatives j  xjF(x)\frac{\partial^j\;}{\partial x^j}F(x) that vanish at a catastrophe of a scalar function F(x)F(x). We do not extend catastrophe theory or singularity theory themselves, but provide a means to apply them more readily to the multi-dimensional dynamical models that appear, for example, in the study of various engineered or living systems. For illustration we apply our conditions to locate butterfly and star catastrophes in a second order PDE.

Cite

@article{arxiv.2310.14813,
  title  = {Catastrophe conditions for vector fields in $\mathbb R^n$},
  author = {Mike R. Jeffrey},
  journal= {arXiv preprint arXiv:2310.14813},
  year   = {2023}
}
R2 v1 2026-06-28T12:58:47.594Z