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Axes in outer space

About this Title

Michael Handel, Lehman College, CUNY and Lee Mosher, Rutgers University, Newark

Publication: Memoirs of the American Mathematical Society
Publication Year: 2011; Volume 213, Number 1004
ISBNs: 978-0-8218-6927-7 (print); 978-1-4704-0621-9 (online)
DOI: https://doi.org/10.1090/S0065-9266-2011-00620-9
Published electronically: March 10, 2011
MSC: Primary 20F65, 57M07

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Table of Contents

Chapters

  • 1. Introduction
  • 2. Preliminaries
  • 3. The ideal Whitehead graph
  • 4. Cutting and pasting local stable Whitehead graphs
  • 5. Weak train tracks
  • 6. Topology of the axis bundle
  • 7. Fold lines

Abstract

We develop a notion of axis in the Culler–Vogtmann outer space $\mathcal {X}_r$ of a finite rank free group $F_r$, 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 Teichmüller space, $\mathcal {X}_r$ 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” $\mathcal {A}_\phi$ with nice topological properties: $\mathcal {A}_\phi$ is a closed subset of $\mathcal {X}_r$ proper homotopy equivalent to a line, it is invariant under $\phi$, the two ends of $\mathcal {A}_\phi$ limit on the repeller and attractor of the source–sink action of $\phi$ on compactified outer space, and $\mathcal {A}_\phi$ depends naturally on the repeller and attractor. We propose various definitions for $\mathcal {A}_\phi$, each motivated in different ways by train track theory or by properties of axes in Teichmüller space, and we prove their equivalence.

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