Axes in Outer Space
Abstract
We develop a notion of axis in the Culler--Vogtmann outer space Xr of a finite rank free group Fr, with respect to the action of a nongeometric, fully irreducible outer automorphism phi. Unlike the situation of a loxodromic isometry acting on hyperbolic space, or a pseudo-Anosov mapping class acting on Teichmuller space, Xr has no natural metric, and phi seems not to have a single natural axis. Instead our axes for phi, while not unique, fit into an ``axis bundle'' Aphi with nice topological properties: Aphi is a closed subset of Xr proper homotopy equivalent to a line, it is invariant under phi, the two ends of Aphi limit on the repeller and attractor of the source--sink action of phi on compactified outer space, and Aphi depends naturally on the repeller and attractor. We propose various definitions for Aphi, each motivated in different ways by train track theory or by properties of axes in Teichmuller space, and we prove their equivalence.
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