Eventual compact covering and backward-orbit density #
Section 5: real-axis expansion and two logarithms give eventual covering of compact sets.
Part of Lasse Rempe's formalisation of Shen and Rempe-Gillen's exponential-map paper,
with generative AI assistance including Copilot, Claude, and particularly ChatGPT.
The initial proof architecture uses John Harrison's HOL Light formalisation.
See LeanPool.ExpChaotic for attribution and the upstream source.
Section 5: eventual covering of compact sets #
We use radius-eight disks instead of radius-2π disks to keep the estimates simple.
Since Lemma 6 already supplies an orbit reaching the real axis in every open disk,
we only need expansion along real orbits, rather than general escaping orbits.
A small disk centred on the real axis is expanded by a prescribed factor.
Iterated images of a disk on a sufficiently far right real orbit contain unit disks.
Two exponentials of a radius-eight disk sufficiently far along the real axis cover any prescribed annulus. Integer translates of a logarithm supply the preimages.
Compactness makes the preceding elementary covering estimate uniform.
Every sufficiently late image of a disk centred on a far right real point covers a given compact subset of the punctured plane.
Corollary 5.5 (open sets spread everywhere). Every sufficiently late iterated image of a nonempty open set contains any given compact set omitting zero. Only real-axis Lemma 6 and the quantitative open-mapping Lemma 3 are needed.
The compact covering theorem specialised to an open ball of positive radius.
Lemma 6, negative-axis form. This now follows from the Section 5 theorem
by taking the nonzero target to be -1. The connectedness hypothesis is retained
for compatibility with the original statement.
The backward orbit of the real axis is dense.