Shuichi Nos\'e opened up a new world of atomistic simulation in 1984. He
formulated a Hamiltonian tailored to generate Gibbs' canonical distribution
dynamically. This clever idea bridged the gap between microcanonical molecular
dynamics and canonical statistical mechanics. Until then the canonical
distribution was explored with Monte Carlo sampling. Nos\'e's dynamical
Hamiltonian bridge requires the "ergodic" support of a space-filling structure
in order to reproduce the entire distribution. For sufficiently small systems,
such as the harmonic oscillator, Nos\'e's dynamical approach failed to agree
with Gibbs' sampling and instead showed a complex structure, partitioned into a
chaotic sea, islands, and chains of islands, that is familiar textbook fare
from investigations of Hamiltonian chaos. In trying to enhance small-system
ergodicity several more complicated "thermostated" equations of motion were
developed. All were consistent with the canonical Gaussian distribution for the
oscillator coordinate and momentum. The ergodicity of the various approaches
has undergone several investigations, with somewhat inconclusive (
contradictory ) results. Here we illustrate several ways to test ergodicity and
challenge the reader to find even more convincing algorithms or an entirely new
approach to this problem.Comment: 12 pages and five figure