Caleb Martin

Properties of Julia Sets

Let be a polynomial of degree at least 2, and let be the k-fold composition of, so denotes the iterate of w under. Then we define the filled-in Julia setfor

The Julia set for is then defined to be the boundary of this set, .For example, if, then and , where represents absolute value, since clearly iff and iff .

Lemma 1: Given with , there exists some constant r such that if then .

Proof: Choose r large enough that if, then and . Then if ,

.

Further, if for some p, then we can apply Lemma 1 inductively to show that , so we must have .

Some fundamental properties of Julia sets follow quickly from this:

  1. and are nonempty and compact, e.g. closed and bounded
  2. for all
  3. is forward and backward invariant, e.g.

Proof:

  1. With r given by Lemma 1, clearly and are contained in the neighborhood of the origin and thus are bounded. Suppose . Then , so for some p, and since polynomials are everywhere continuous, for all w in some small neighborhood . So by the lemma, for all such w and therefore . So is open and is closed. is also closed, and thus both sets are compact.
  2. By the lemma, iff . So and have the same filled-in Julia sets and thus the same Julia sets.
  3. Let , so , and we can find a sequence such that for each n. Thus the points , but , and by continuity, can be chosen arbitrarily close to , and thus . It follows that and . For the reverse inclusion, take z and as before and find a sequence and for all n. By similar arguments we get , so it follows that and the equalities we want hold.

We say w is an attracting fixed point of if and. We say w is repelling if or, and similarly for periodic points. (w is periodic with period k if for some k) Note we allow to be considered as a normal point. Define the basin of an attracting fixed point w to be the set

.

The following three statements are given without proof, as they rely on some fairly technical results from complex variable theory, specifically Montel’s Theorem about normal families of complex analytic functions, which implies that iff the family is not normal at z.However, they give useful characterizations of general Julia sets, so are worth mentioning.

In particularly, they rely on the result that for any , if is a small neighborhood of z, then is the entirely of except for no more than one exceptional point for each .

Theorem 1: Let w be any attracting fixed point of. Then.

Theorem 2: is the closure of the repelling periodic points of.

Theorem 3: If , then is exactly the closure of .

As a simple example of the first two statements, consider our previous example, . Attracting fixed points clearly exist at 0 and , and is the unit circle, which is exactly and equivalently, . Moreover, for on the unit circle,iterating f corresponds to rotating by , so we have repelling periodic points at all rational values of . Sinceis dense in, the closure of is exactly the unit circle.

The Mandelbrot Set

We now focus our attention on the specific class on functions, where c is some complex constant. For simplicity, we write to mean . By Theorem 3, if we can reliably locate at least one point of we get a convenient way to plot the entire Julia set. Since, its inverse is given by. We can use a deterministic game to plot iterations of, where the correspond to the positive and negative branches of each chosen with probability ½. However, it takes many iterations to fill the entire Julia set, as points tend to cluster around certain regions.

Note that our choice of functions to examine is not as restrictive as it seems. Consider the transformation. Then , so by carefully choosingand we can produce a conjugate map for any degree 2 polynomialwe like. Since is a linear map, this means that the Julia sets and are geometrically similar to each other.

Now we are able to define the Mandelbrot set,

Note Mis aset in the parameter plane, not the normal complex plane where the Jc’s reside. We are ready to prove our main result of this section, using the following lemma.

Lemma 2: Let be a loop (simple closed curve) in the complex plane.

  1. If c is interior to , then is also a loop, with the inverse image of the interior of equal to the interior of .
  2. If c lies on , then is a figure-8 with self-intersection point at the origin, such that the inverse image of the interior of is equal to the interior of each leaf.

Proof: Since and , these are finite and non-zero when , and thus each branch of is locally smooth provided .

  1. Suppose . Take any initial value w on and choose one of the two values of . If we let vary as z traverses , then traces out a smooth curve. When z returns to the initial value w, takes on its other value, and as z traverses again, continues along a smooth path and returns to the first value of when z returns to w a second time. Since , , so along . This implies that cannot be a point of self-intersection, since then would be a self-intersection point of . So is also a loop. Note as z traverses once, the rays from 0 to fill half the interior of , and as z traverses again, the rays from 0 to the other value fill the other half, so the correspondence from to is one-to-one.
  2. Proof is similar to (1). Let , so if is a piece of curve through c, consists of two smooth pieces of curve through 0 which are perpendicular. As in (1), if we take an initial value w on , choose a value of , and let z traverse , then traces out a closed loop, hitting 0 at , then taking on the other value of and tracing out another, disjoint, closed loop before closing when again. For z on the first loop, rays from zero fill the interior, and similarly for on the second loop, so we have the desired correspondence between and each leaf of .

Theorem 4: Let M be the Mandelbrot set. Then the following are equivalent definitions:

Proof: If we let , then we can apply Lemma 1 to show that these two definitions are equivalent to each other. We show that if is bounded, then is connected, and for the reverse inclusion, we show that if, then is disconnected. We write for , and for .

Assume is bounded, and let be a circle large enough to completely enclose , with the additional properties that all points outside are in and that lies in the interior of . Since , we must have c inside . By Lemma 2.1, maps to , so since, we must also have c inside . We proceed inductively, applying the lemma at each stage. For , , and at each k, since , so, so, and so on. Thus we construct an infinite series of nested loops, each contained in the interior of the last.

Let , and let . By our choice of , any point outside for some n must iterate to infinity, so it follows that . But then the filled-in Julia set is exactly K.

So . From a basic result in topology, a nested sequence of compact connected sets has connected intersection and boundary, so we see that is connected, as desired.

Assume is unbounded, i.e. . Then let be a circle large enough that all points outside are in, lies in the interior of , and that for some value of p, we have with , and . We begin just as in (1), constructing a series of nested loops, but when we get to, where c lies on the curve instead of interior to it and Lemma 2.1 no longer applies. From now on we apply Lemma 2.2, so we get that is a figure-8, with contained in its interior. Since we have the one-to-one correspondence between inverse images given by the lemma, each leaf of the figure-8 contains points of , and thus is disconnected.

Note we can actually do better than this and make our original definition of M more robust. If is disconnected, we can inductively apply Lemma 2.2 to show that after some , there is an infinite series of figure-8’s contained in each leaf of the previous curve , all containing nonempty subsets of . Thus consists of infinitely many disconnected sets, and is actually a Cantor dust (each of these sets consists only of a single point), but that requires some extra analysis to prove explicitly.

See Appendix A for an illustration of the general idea behind this proof.

Periodic Orbits and the Structure of M

The large cardioid that comprises the bulk of the Mandelbrot set corresponds to those values of c where has an attracting fixed point. Julia sets in this region are deformed circles, with the point giving a the unit circle as we saw before, and becoming increasingly complex as c approaches the boundary of the cardioid. We use this characterization to solve for its boundary explicitly.

If has an attracting fixed point at , and . Clearly z on the boundary of such points satisfies , or . Substituting back into , we get , which indeed traces out the cardioid as traverses . Reparametrizing, we can model the equation as .

Similarly, we can solve explicitly for the circular bulb to the left of the main cardioid by noting that it corresponds to values of c where has a period-2 orbit.

If has a period-2 orbit, then has an attracting fixed point. Then for z in the circular region, . Factoring, we get

Roots of the second term on the right are just the fixed points of , which makes sense because fixed points of are also fixed under . Let , be the roots of the first term on the right. The product of the two roots is the constant term, so we get . Since they are period-2, and . Differentiating gives us . Since they are attracting, we know that , and equating these gives the condition , the boundary of which is indeed a circle of radius ¼ centered at .

Note the correspondence shown below between points in the parameter plane where the bulbs of the Mandelbrot set are attached to the largest adjacent bulb and the bifurcation points of the logistic map. In the large cardioid, we correspond to stable orbits of , in the period-2 bulb, we correspond to period-2 orbits, and similarly all the way down the period-double cascade in the logistic map until it dissolves into chaos and the Mandelbrot set is a segment of the axis. The cardioid of the smaller copy of M centered around corresponds to the stable period-3 region that arises in the bifurcation plot, and similarly for the period-doubling cascade following it, and so on. It is theoretically possible to solve for the bounds of any bulb on the Mandelbrot set using similarly descriptive conditions on periodic orbits of , but the complexity of the relevant equations scale up inordinately quickly for efficient computation. As we move along the negative axis, the next largest copy of M will a period-4 region in its cardioid, and so on. Note the periods of the bulbs on all these smaller copies are exactly the same as that of the correspondingbulb on the whole of M, except multiplied by the period of main cardioid in the copy.

M, plotted in black on the parameter plane :

Bifurcation diagram of the map:

Extending this, all of the bulbs on the Mandelbrot set can be put in a correspondence with the existence of periodic orbits for a given period, but this correspondence turns out to be extraordinarily detailed. For example, in the equation previously given for the boundary of the main cardioid, , we observe that , the point given by is exactly where a period-k bulb is connected to the main cardioid. (We just demonstrated this for the bulb) Thus we see that as we travel towards the origin along the boundary of the main cardioid starting at , the next largest bulb (the topmost one) is the period-3 bulb, the next largest the period-4, and so on. Immediately we know we can find values of c which give stable periodic orbits of any given period, a hallmark of chaos, though we are in parameter space and thus ranging over a family of related functions instead of ranging over initial values for a single function. Moreover, given any two bulbs of period p and q, the period of the largest bulb between them is always given by.

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Caleb Martin

Right: The primary bulbs of M, labeled according to their period. Note the behavior as described above.

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Caleb Martin

We can also determine the period of a bulb just by looking at it, either in the parameter plane or by looking at a Julia set for some c value in the bulb. In a period-k bulb, there will always be a large spindly arm extending away from the bulb that separates into several smaller arms. The number of arms that meet at this intersection is always exactly the period, k. Moreover, the filled-in Julia set at cwill have a large central region symmetric about the origin, pinching down on either side to a single point where several smaller buds meet. Since Julia sets are fractals, self-similarity assures that this happens on all of these secondary buds as well, but the largest ones are sufficient to determine the period. As expected, there are exactly k buds meeting at each of these points (so removing any one of them disconnects into k disjoint pieces.

We illustrate this below for several bulbs on the Mandelbrot set:

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Caleb Martin

Period 3

Period 5

Period 4

Period 7

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Caleb Martin

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Caleb Martin

The same behavior, this time using Julia sets to determine period:

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Caleb Martin

Period 2,

Period 5,

Period 4,

Period 7,

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Caleb Martin

This correspondence between location and periodic orbits goes considerably deeper. Instead of assigning each bulb an integer kthat corresponds to the existence of a stable period-k orbit of for values of c in the bulb, we assign each bulb a rotation number . For the bulbs we first described (i.e. the large primary bulbs attached to the main cardioid at for integer values of k), we say . For rotation numbers, the denominator n corresponds to the period, and if we let be the stable orbit, we let the numerator m be the number such that for .

We can still determine rotation numbers by looking at the bulb in the Mandelbrot set or the Julia set of and appropriate value of c. In the Mandelbrot set, consider the spike complex that we used to determine period. The shortest spike counterclockwise from the main one connected to the bulb is the one. Analogously, in the Julia sets, the smallest of the n buds counterclockwise from the main one is the one.

Thus referring back to our previous examples and reading left-right, top-bottom, the rotation numbers of the Mandelbrot set bulbs are given by 1/3, 1/4, 2/5, and 3/7. In the Julia set examples, rotation numbers are given by 1/2, 1/4, 1/5, and 1/7. Note for Julia sets, it is difficult to tell if a bulb is primary or not, and in general one must check where the c value actually lies in the parameter plane to check this.

It is easy to see that points where bulbs attach to the main cardioid of the Mandelbrot set are dense on its boundary. Amazingly, the set of points where the bulb of rotation number attaches to the cardioid are ordered precisely by the natural order of the rationals. Since M is symmetrical with respect to the axis, we can imagine traversing the around boundary of the main cardioid starting and ending at the origin, and at every rational point we will hit a bulb of rotation number .

Also, note that we can generalize rotation numbers of primary bulbs to bulbs of arbitrary order by analogous definitions, where a k-ary bulb defined recursively as a bulb attached by a point to a (k-1)-ary bulb and primary bulbs the ones touching the main cardioid by assigning k-ary bulbs a k-tuple of rotation numbers in .

To expand on this, we can still calculate rotation numbers from the rotation numbers of nearby bulbs in a similar fashion as we had for periods. Given bulbs with rotation numbers and , the rotation number of the largest bulb between them is not given by , but rather by , the naïve definition of addition in the rational numbers. There is an explanation for this occurrence, however. This type of addition is relevant in number theory, where it is termed Farey addition, and it describes the relationship that given two (proper) fractions and , the resulting sum is the (proper) fraction strictly between and with lowest denominator. This makes sense with our description of how the rotation numbers ordered the bulbs along the boundary of the main cardioid in the same manner that is ordered as a field.

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Right: an illustration of Farey addition for rotation numbers of bulbs in the Mandelbrot set, (e.g. )

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Finally, because of this structure of how rotation numbers and periods are located around the boundary of the cardioid, we can provide geometric trajectories around the parameter plane that represent nearly any algebraic sequence we wish:

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Caleb Martin

Right: For example, we can represent the familiar Fibonacci sequence , by starting with the period-2 bulb, and then taking to be the period of the next largest bulb clockwise around the boundary, the period of the next bulb counterclockwise, and so on, so we always consider the largest bulb between the previous two.