Orbit portrait

In mathematics, an orbit portrait is a combinatorial tool used in complex dynamics for understanding the behavior of one-complex dimensional quadratic maps.

In simple words one can say that it is :

• a list of external angles for which rays land on points of that orbit
• graph showing above list

Definition

Given a quadratic map

${\displaystyle f_{c}:z\mapsto z^{2}+c.}$

from the complex plane to itself

${\displaystyle f_{c}:\mathbb {\mathbb {C} } \to \mathbb {\mathbb {C} } }$

and a repelling or parabolic periodic orbit ${\displaystyle {\mathcal {O}}=\{z_{1},\ldots z_{n}\}}$ of ${\displaystyle f}$, so that ${\displaystyle f(z_{j})=z_{j+1}}$ (where subscripts are taken 1 + modulo ${\displaystyle n}$), let ${\displaystyle A_{j}}$ be the set of angles whose corresponding external rays land at ${\displaystyle z_{j}}$.

Then the set ${\displaystyle {\mathcal {P}}={\mathcal {P}}({\mathcal {O}})=\{A_{1},\ldots A_{n}\}}$ is called the orbit portrait of the periodic orbit${\displaystyle {\mathcal {O}}}$.

All of the sets ${\displaystyle A_{j}}$ must have the same number of elements, which is called the valence of the portrait.

Examples

Julia set with external rays landing on period-3 orbit

Julia set with period-two parabolic orbit. The associated orbit portrait has characteristic arc I = (22/63, 25/63) and valence v = 3 rays per orbit point.

Parabolic or repelling orbit portrait

valence 2

${\displaystyle {\mathcal {P}}=\left\{\left({\frac {1}{3}},{\frac {2}{3}}\right)\right\rbrace }$

${\displaystyle {\mathcal {P}}=\left\{\left({\frac {3}{7}},{\frac {4}{7}}\right),\left({\frac {6}{7}},{\frac {1}{7}}\right),\left({\frac {5}{7}},{\frac {2}{7}}\right)\right\rbrace }$

${\displaystyle {\mathcal {P}}=\left\{\left({\frac {4}{9}},{\frac {5}{9}}\right),\left({\frac {8}{9}},{\frac {1}{9}}\right),\left({\frac {7}{9}},{\frac {2}{9}}\right)\right\rbrace }$

${\displaystyle {\mathcal {P}}=\left\{\left({\frac {11}{31}},{\frac {12}{31}}\right),\left({\frac {22}{31}},{\frac {24}{31}}\right),\left({\frac {13}{31}},{\frac {17}{31}}\right),\left({\frac {26}{31}},{\frac {3}{31}}\right),\left({\frac {21}{31}},{\frac {6}{31}}\right)\right\rbrace }$

valence 3

Valence is 3 so rays land on each orbit point.

3 external rays of period 3 cycle : ${\displaystyle {\mathcal {R}}_{\frac {1}{7}},{\mathcal {R}}_{\frac {2}{7}},{\mathcal {R}}_{\frac {4}{7}}\,}$, which land on fixed point ${\displaystyle z=\alpha _{c}\,}$

${\displaystyle {\mathcal {P}}=\left\{\left({\frac {1}{7}},{\frac {2}{7}},{\frac {4}{7}}\right)\right\rbrace }$

For complex quadratic polynomial with c= -0.03111+0.79111*i portrait of parabolic period 3 orbit is : ^[1]

${\displaystyle {\mathcal {P}}=\left\{\left({\frac {74}{511}},{\frac {81}{511}},{\frac {137}{511}}\right),\left({\frac {148}{511}},{\frac {162}{511}},{\frac {274}{511}}\right),\left({\frac {296}{511}},{\frac {324}{511}},{\frac {37}{511}}\right)\right\rbrace }$

Rays for above angles land on points of that orbit . Parameter c is a center of period 9 hyperbolic component of Mandelbrot set.

For parabolic julia set c = -1.125 + 0.21650635094611*i. It is a root point between period 2 and period 6 components of Mandelbrot set. Orbit portrait of period 2 orbit with valence 3 is : ^[2]

${\displaystyle {\mathcal {P}}=\left\{\left({\frac {22}{63}},{\frac {25}{63}},{\frac {37}{63}}\right),\left({\frac {11}{63}},{\frac {44}{63}},{\frac {50}{63}}\right)\right\rbrace }$

valence 4

${\displaystyle {\mathcal {P}}=\left\{\left({\frac {1}{15}},{\frac {2}{15}},{\frac {4}{15}},{\frac {8}{15}}\right)\right\rbrace }$

Formal orbit portraits

Every orbit portrait ${\displaystyle {\mathcal {P}}}$ has the following properties:

• Each ${\displaystyle A_{j}}$ is a finite subset of ${\displaystyle {\mathbb {R} }/{\mathbb {Z} }}$
• The doubling map on the circle gives a bijection from ${\displaystyle A_{j}}$ to ${\displaystyle A_{j+1}}$ and preserves cyclic order of the angles. ^[3]
• All of the angles in all of the sets ${\displaystyle A_{1},\ldots ,A_{n}}$ are periodic under the doubling map of the circle, and all of the angles have the same exact period. This period must be a multiple of ${\displaystyle n}$, so the period is of the form ${\displaystyle rn}$, where ${\displaystyle r}$ is called the recurrent ray period.
• The sets ${\displaystyle A_{j}}$ are pairwise unlinked, which is to say that given any pair of them, there are two disjoint intervals of ${\displaystyle {\mathbb {R} }/{\mathbb {Z} }}$ where each interval contains one of the sets.

Any collection ${\displaystyle \{A_{1},\ldots ,A_{n}\}}$ of subsets of the circle which satisfy these four properties above is called a formal orbit portrait. It is a theorem of John Milnor that every formal orbit portrait is realized by the actual orbit portrait of a periodic orbit of some quadratic one-complex-dimensional map. Orbit portraits contain dynamical information about how external rays and their landing points map in the plane, but formal orbit portraits are no more than combinatorial objects. Milnor's theorem states that, in truth, there is no distinction between the two.

Trivial orbit portraits

Orbit portrait where all of the sets ${\displaystyle A_{j}}$ have only a single element are called trivial, except for orbit portrait ${\displaystyle {0}}$. An alternative definition is that an orbit portrait is nontrivial if it is maximal, which in this case means that there is no orbit portrait that strictly contains it (i.e. there does not exist an orbit portrait ${\displaystyle \{A_{1}^{\prime },\ldots ,A_{n}^{\prime }\}}$ such that ${\displaystyle A_{j}\subsetneq A_{j}^{\prime }}$). It is easy to see that every trivial formal orbit portrait is realized as the orbit portrait of some orbit of the map ${\displaystyle f_{0}(z)=z^{2}}$, since every external ray of this map lands, and they all land at distinct points of the Julia set. Trivial orbit portraits are pathological in some respects, and in the sequel we will refer only to nontrivial orbit portraits.

Arcs

In an orbit portrait ${\displaystyle \{A_{1},\ldots ,A_{n}\}}$, each ${\displaystyle A_{j}}$ is a finite subset of the circle ${\displaystyle \mathbb {R} /\mathbb {Z} }$, so each ${\displaystyle A_{j}}$ divides the circle into a number of disjoint intervals, called complementary arcs based at the point ${\displaystyle z_{j}}$. The length of each interval is referred to as its angular width. Each ${\displaystyle z_{j}}$ has a unique largest arc based at it, which is called its critical arc. The critical arc always has length greater than ${\displaystyle {\frac {1}{2}}}$

These arcs have the property that every arc based at ${\displaystyle z_{j}}$, except for the critical arc, maps diffeomorphically to an arc based ${\displaystyle z_{j+1}}$, and the critical arc covers every arc based at ${\displaystyle z_{j+1}}$ once, except for a single arc, which it covers twice. The arc that it covers twice is called the critical value arc for ${\displaystyle z_{j+1}}$. This is not necessarily distinct from the critical arc.

When ${\displaystyle c}$ escapes to infinity under iteration of ${\displaystyle f_{c}}$, or when ${\displaystyle c}$ is in the Julia set, then ${\displaystyle c}$ has a well-defined external angle. Call this angle ${\displaystyle \theta _{c}}$. ${\displaystyle \theta _{c}}$ is in every critical value arc. Also, the two inverse images of ${\displaystyle c}$ under the doubling map (${\displaystyle {\frac {\theta _{c}}{2}}}$ and ${\displaystyle {\frac {\theta _{c}+1}{2}}}$) are both in every critical arc.

Among all of the critical value arcs for all of the ${\displaystyle A_{j}}$'s, there is a unique smallest critical value arc ${\displaystyle {\mathcal {I}}_{\mathcal {P}}}$, called the characteristic arc which is strictly contained within every other critical value arc. The characteristic arc is a complete invariant of an orbit portrait, in the sense that two orbit portraits are identical if and only if they have the same characteristic arc.

Sectors

Much as the rays landing on the orbit divide up the circle, they divide up the complex plane. For every point ${\displaystyle z_{j}}$ of the orbit, the external rays landing at ${\displaystyle z_{j}}$ divide the plane into ${\displaystyle v}$ open sets called sectors based at ${\displaystyle z_{j}}$. Sectors are naturally identified the complementary arcs based at the same point. The angular width of a sector is defined as the length of its corresponding complementary arc. Sectors are called critical sectors or critical value sectors when the corresponding arcs are, respectively, critical arcs and critical value arcs. ^[4]

Sectors also have the interesting property that ${\displaystyle 0}$ is in the critical sector of every point, and ${\displaystyle c}$, the critical value of ${\displaystyle f_{c}}$, is in the critical value sector.

Parameter wakes

Two parameter rays with angles ${\displaystyle t_{-}}$ and ${\displaystyle t_{+}}$ land at the same point of the Mandelbrot set in parameter space if and only if there exists an orbit portrait ${\displaystyle {\mathcal {P}}}$ with the interval ${\displaystyle [t_{-},t_{+}]}$ as its characteristic arc. For any orbit portrait ${\displaystyle {\mathcal {P}}}$ let ${\displaystyle r_{\mathcal {P}}}$ be the common landing point of the two external angles in parameter space corresponding to the characteristic arc of ${\displaystyle {\mathcal {P}}}$. These two parameter rays, along with their common landing point, split the parameter space into two open components. Let the component that does not contain the point ${\displaystyle 0}$ be called the ${\displaystyle {\mathcal {P}}}$-wake and denoted as ${\displaystyle {\mathcal {W}}_{\mathcal {P}}}$. A quadratic polynomial ${\displaystyle f_{c}(z)=z^{2}+c}$ realizes the orbit portrait ${\displaystyle {\mathcal {P}}}$ with a repelling orbit exactly when ${\displaystyle c\in {\mathcal {W}}_{\mathcal {P}}}$. ${\displaystyle {\mathcal {P}}}$ is realized with a parabolic orbit only for the single value ${\displaystyle c=r_{\mathcal {P}}}$ for about

Primitive and satellite orbit portraits

Other than the zero portrait, there are two types of orbit portraits: primitive and satellite. If ${\displaystyle v}$ is the valence of an orbit portrait ${\displaystyle {\mathcal {P}}}$ and ${\displaystyle r}$ is the recurrent ray period, then these two types may be characterized as follows:

• Primitive orbit portraits have ${\displaystyle r=1}$ and ${\displaystyle v=2}$. Every ray in the portrait is mapped to itself by ${\displaystyle f^{n}}$. Each ${\displaystyle A_{j}}$ is a pair of angles, each in a distinct orbit of the doubling map. In this case, ${\displaystyle r_{\mathcal {P}}}$ is the base point of a baby Mandelbrot set in parameter space.
• Satellite orbit portraits have ${\displaystyle r=v\geq 2}$. In this case, all of the angles make up a single orbit under the doubling map. Additionally, ${\displaystyle r_{\mathcal {P}}}$ is the base point of a parabolic bifurcation in parameter space.

Generalizations

Orbit portraits turn out to be useful combinatorial objects in studying the connection between the dynamics and the parameter spaces of other families of maps as well. In particular, they have been used to study the patterns of all periodic dynamical rays landing on a periodic cycle of a unicritical anti-holomorphic polynomial. ^[5]

See also

• Lamination

References

1. Flek, Ross; Keen, Linda (2010). "Boundaries of Bounded Fatou Components of Quadratic Maps" (PDF). Journal of Difference Equations and Applications. 16 (5–6): 555–572. doi:10.1080/10236190903205080. S2CID   54997658.
2. Milnor, John W. (1999). "Periodic Orbits, Externals Rays and the Mandelbrot Set: An Expository Account". Preprint. arXiv: math/9905169 . Bibcode:1999math......5169M.
3. Chaotic 1D maps by Evgeny Demidov
4. Periodic orbits and external rays by Evgeny Demidov
5. Mukherjee, Sabyasachi (2015). "Orbit portraits of unicritical antiholomorphic polynomials". Conformal Geometry and Dynamics. 19 (3): 35–50. arXiv: 1404.7193 . doi: 10.1090/S1088-4173-2015-00276-3 .