Rotation number should not be confused with Rotation (quantity).
In mathematics, the rotation number is an invariant of homeomorphisms of the circle.
It was first defined by Henri Poincaré in 1885, in relation to the precession of the perihelion of a planetary orbit. Poincaré later proved a theorem characterizing the existence of periodic orbits in terms of rationality of the rotation number.
Suppose that
f:S1\toS1
S1=\R/\Z.
F:\R\to\R
F(x+m)=F(x)+m
for every real number and every integer .
The rotation number of is defined in terms of the iterates of :
\omega(f)=\limn\toinfty
Fn(x)-x | |
n |
.
Henri Poincaré proved that the limit exists and is independent of the choice of the starting point . The lift is unique modulo integers, therefore the rotation number is a well-defined element of Intuitively, it measures the average rotation angle along the orbits of .
If
f
2\piN
0<N<1
F(x)=x+N,
and its rotation number is
N
The rotation number is invariant under topological conjugacy, and even monotone topological semiconjugacy: if and are two homeomorphisms of the circle and
h\circf=g\circh
for a monotone continuous map of the circle into itself (not necessarily homeomorphic) then and have the same rotation numbers. It was used by Poincaré and Arnaud Denjoy for topological classification of homeomorphisms of the circle. There are two distinct possibilities.
The rotation number is continuous when viewed as a map from the group of homeomorphisms (with topology) of the circle into the circle.