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The graph of a nondecreasing function,
, is called a devil's staircase if
there exists a family of disjoint open intervals, such that their union is
dense in
,
the function
is constant on each interval and such that
takes
different values on different intervals (see, e.g., [6, 8]).
A rational number,
is called exceptional,
if the homeomorphism
such that
is conjugate to
.
For any non-exceptional p/q, the set
is an interval,
with nonempty interior.
Using the terminology of circle maps, we call
a phase locking interval.
If p/q is exceptional, the interval
degenerates to a single point
.
In this case, every point on the invariant
curve
is periodic. From the formula in Lemma 2.2
of
we get:
This leads to the following Corollary:
By differentiating this relation along a deformation, we get
necessary conditions which have to hold in an exceptional case.
Let
be a q-periodic orbit, and let
be a deformation of O. We assume that I is an interval
with a nonempty interior,
that
. Let
be the
polygon corresponding to O(t).
We will assume that the deformation O(t) is differentiable for
and nontrivial.
By this we mean that
are
-functions, that
for
, and that at least one
for
.
We say a periodic orbit
admits a deformation
if O is contained in an interval of periodic orbits.
Proof. Assume a deformation O(t) exists. Let
be parameterized
by arc lengths
.
We have
and
. Use this and
the mirror equation of geometrical optics to get
Differentiating
obtained from Equation (1) gives
This is not possible since
for at least one j
and
for all
.
End of the proof.
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Fig. 9. Proof of Lemma 3.3. |
This is a special case of a more general theorem, which we have proven in
[3].
There is first of all a geometrical argument which shows that for a generic
convex curve
, the rotation function is a devil's staircase. We also
showed that if
has a flat point of if
is a polygon, then the rotation function is a devil's staircase.
Figure 10 shows a numerically computed graph of the rotation function
in our case, when the
is an equilateral triangle.
The graph shows the rotation number in dependence on
.
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Fig. 10. Numerical computation of the rotation number in dependence of |
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