Geometric limits of Julia sets for sums of power maps and polynomials
Micah Brame, Scott Kaschner

TL;DR
This paper characterizes the geometric limits of Julia sets for maps combining power maps and polynomials as the degree of the power map tends to infinity, identifying conditions for convergence to the unit disk or circle.
Contribution
It establishes necessary and sufficient conditions for the limits of Julia sets in these maps and describes their structure in many cases.
Findings
Limits are the closed unit disk or circle under certain conditions.
Provides a comprehensive description of the limiting sets.
Identifies key parameters influencing the geometric limits.
Abstract
For maps of one complex variable, , given as the sum of a degree power map and a degree polynomial, we provide necessary and sufficient conditions that the geometric limit as approaches infinity of the set of points that remain bounded under iteration by is the closed unit disk or the unit circle. We also provide a general description, for many cases, of the limiting set.
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Geometric limits of Julia sets for sums of power maps and polynomials
Micah Brame
Butler University, 4600 Sunset Ave., Indianapolis, IN 46208, USA
and
Scott Kaschner
Butler University, 4600 Sunset Ave., Indianapolis, IN 46208, USA
Abstract.
For maps of one complex variable, , given as the sum of a degree power map and a degree polynomial, we provide necessary and sufficient conditions that the geometric limit as approaches infinity of the set of points that remain bounded under iteration by is the closed unit disk or the unit circle. We also provide a general description, for many cases, of the limiting set.
1. Introduction
Let be a degree polynomial; define by
[TABLE]
and note that is the sum of a power map (whose power we increase in the limit) and a fixed degree polynomial, . For a map , the filled Julia set for , , is the set of points that remain bounded under iteration by . We use the notation for the unit circle and for the closed unit disk. The purpose of this study is to describe the limit of in the Hausdorff topology as .
This work was inspired the 2012 study by Boyd and Schulz [4] that included a result for the family with ; that is, . Among many other things, they proved
Theorem 1.1** (Boyd-Shulz, 2012).**
If , then under the Hausdorff metric,
[TABLE]
It comes as little surprise that this phenomena is easily disrupted. It was shown in [13] that when with , the limiting behavior of depends on number-theoretic properties of and the limit almost always fails to exist. Another study by Alves [1], has shown that for maps of the form for a fixed positive integer , if , then the limit of as is .
Returning to the more general case in which is any polynomial, the limiting behavior of is substantially more interesting. See Figure 1 for examples of filled Julia sets for , where and , that very clearly fail to limit to either the closed unit disk or the unit circle. The color gradation in the pictures indicates the number of iterates required to exceed a fixed bound for modulus.
Some results from the cases still hold. If , we can still expect the image of under to have large modulus for large enough . Guided by this intuition, we find the following generalization of a lemma from [4]. We omit the proof, as it is similar to [4], and adopt the notation
[TABLE]
Lemma 1.2**.**
For any polynomial and any , there is an such that for all ,
[TABLE]
Some of the dependence of the limiting behavior of on is obvious; by Lemma 1.2, one should expect any point whose orbit by leaves the unit disk to not be in for all sufficiently large. Thus, one might expect to be contained in the closure of the set
[TABLE]
However, this is not quite the case. One can prove, as in the cases, that is always a subset of the .
Evidence for this fact (proved in Section 3) comes by noting that when is much larger than the degree of , the fixed points of are roughly equidistributed around the unit circle. This result is connected to the work of Erdös, Turan, et al. [7, 11, 12] on distribution of zeros for sequences of complex polynomials.
By invariance properties of the filled Julia set, one should then expect the preimages of by (that still have modulus less than or equal to one) to be contained in . The basins of the fixed points accumulating on and their preimages (appearing as small black spots) can be seen in Figure 1. These ideas and the preceding lemmas lead to the next definition and theorem.
Definition 1.3**.**
Let
[TABLE]
where , is the unit circle , and for any integer ,
[TABLE]
is the set of points in whose orbits by remain in (the set ), the unit circle (), and the parts of the iterated preimages of that remain in at each step (the sets for ). See Figure 2 for an example of with and several different values of compared to a sketch of for this polynomial .
By the construction of , any point bounded a definite distance away from will eventually be mapped a definite distance outside the unit disk. Then Lemma 1.2 implies such a point must be in the basin of infinity for all with large enough , so we have the following theorem.
Theorem 1.4**.**
For any polynomial ,
[TABLE]
What is happening here heuristically is that as long as the orbit of remains in , the polynomial dominates the dynamics; if the orbit of leaves , then the power map dominates. When the orbit hits , it is not clear whether or should win, so you get a point in the Julia set. Now simple conditions that describe precisely when we can expect the closed unit disk, , or the unit circle, , as a limit follow from Theorem 1.4:
Corollary 1.5**.**
Suppose and has no fixed points in . Under the Hausdorff metric,
- (1)
* if and only if , and* 2. (2)
* if and only if .*
With a couple additional assumptions on , we also have the following stronger result.
Theorem 1.6**.**
If and is hyperbolic with no attracting periodic points on , then under the Hausdorff metric
[TABLE]
We are left with the following open question.
Question**.**
In what ways can the hypotheses from Theorem 1.6 on polynomial be relaxed and still have ?
Following a brief tour of background information and examples in Section 2, we present the proof of Theorem 1.4 in Section 3. Lastly, Section 4 is devoted to the proofs of theorems that require specific hypotheses on .
The authors are grateful to Roland Roeder at Indiana University Purdue University Indianapolis for his very helpful advice and the Butler University Mathematics Research Camp, where this project began. We are also very grateful to the referee for their insightful and helpful suggestions. All images we created with the Dynamics Explorer [3] program.
2. Background and Examples
2.1. Notation and Terminology
The main results in this note rely on the convergence of sets in the Riemann sphere, , where the convergence is with respect to the Hausdorff metric. Given two sets in a metric space , the Hausdorff distance between the sets is defined as
[TABLE]
The distance from each point in to has a least upper bound, and the same it true for each point from to . The Hausdorff distance is the supremum over all of these distances. As an example, consider a regular hexagon with sides of length inscribed in a circle of radius . In this case, , the shortest distance from the circle to the midpoint of any of the sides of the hexagon.
Filled Julia sets are compact [2], bounded, and contained in the compact space . Moreover, with the Hausdorff metric , the space of all subsets of is complete [9]. Suppose and are compact subsets of . We say converges to and write if for all , there is such that for all , we have .
We’ve also made use of Painlevé-Kuratowski set convergence [15]. For a sequence of sets, , we have
[TABLE]
It follows immediately that . We say converges to a set in the sense of Painlevé-Kuratowski if , or equivalently, . It is shown in [6] that for sequences of bounded sets, the notion of Painlevé-Kuratowski set convergence agrees with the notion of convergence with Hausdorff distance.
2.2. Complex Dynamics
We provide here only the fine details relevant to this paper. Thorough explorations of this subject and proof of all the facts below can be found in [14, 2, 5]. The Fatou set of rational map , denoted , is the set of points for which the iterates of form a normal family; the Julia set of , denoted , is the complement of in . When is a polynomial map, the Julia set of is the boundary of the filled Julia set; that is, .
We say a point is periodic for with period if and the points are all distinct. The multiplier of a periodic point of period is defined as
[TABLE]
If , then is attracting; if , is repelling; if , is indifferent. Repelling periodic points are contained in ; in fact, repelling periodic points are dense in . Attracting periodic points, on the other hand, are contained in . Moreover, for every attracting periodic point of period , there is an open neighborhood such that and the orbit by of any point in converges to . The set of all points whose orbits by converge to is called the basin of attraction for . Finally, a rational map is called hyperbolic if every point in converges to an attracting periodic cycle.
2.3. Examples
Example 1*.*
Let with , , and . For , we have , so in this case, . For , we have , so in this case, . Both of these cases follow from Corollary 1.5. The more interesting case is in which . See Figure 3. The limit, should it exist, of is the set , which is now significantly more complicated, neither the closed unit disk nor the unit circle.
3. Proof of Main Results
Proof of Lemma 1.2.
Let . We prove for all using induction. Let be the coefficients of , and pick . Then for any , we have . Choose and large enough that . Let . Observe that
[TABLE]
Now suppose for some , we know . Let , and note that . Then for any ,
[TABLE]
It follows that for all . Since , the orbit of under escapes to infinity. Thus, . ∎
Before proving Theorems 1.6, we need a couple more lemmas.
Lemma 3.1**.**
If and , then for any positive integer , there is an such that for all ,
[TABLE]
Moreover, for all and any positive integer , there is an such that for all ,
[TABLE]
Proof.
This proof follows by continuity and is left to the reader. ∎
Lemma 3.2**.**
[TABLE]
There is a body of work on the distribution of polynomial roots begun by Erdös and Turán in [7]. Specific results in [11, 12] dealing with the accumulation of polynomial roots around the unit circle could be applied to the polynomials to find fixed points. However, the case here is simpler because of the coefficients of are all zero. Thus, we have a concise argument using the following potential theory lemma.
Lemma 3.3**.**
For any fixed degree nonzero polynomial, , the zeros of the polynomial cluster uniformly around the unit circle as . More specifically, for each , let
[TABLE]
where is a point mass at , and the roots of are counted with multiplicity. Then weakly as , where is normalized Lebesgue measure on .
Proof of Lemma 3.3.
Note that
[TABLE]
Let be the zero set of , let be a compact subset of , and let be the maximum of on . Then there is an such that for any , we have and either or .
If , then
[TABLE]
Using this and defining , we have
[TABLE]
If , then there is an such that for all , we have . Then
[TABLE]
Noting that when , we have for all that
[TABLE]
Using Equations (1) and (2), we have uniformly on as ; by the compactness theorem for families of subharmonic functions [10, Theorem 4.1.9], it follows that in . Note that , and we have from the Poincarè-Lelong formula [8] that . Thus, we have
[TABLE]
weakly as . ∎
Proof of Lemma 3.2.
We first deal only with the unit circle by showing that . Let and . Define
[TABLE]
so the zeros of are fixed points of . By Lemma 3.3, the fixed points of cluster uniformly near the unit circle. If any of the fixed points are repelling, then they are contained in [14]. Otherwise, they are attracting or indifferent, in which case they must be close to because . It follows that .
Since filled Julia sets are backward invariant, the preimages by of the fixed points clustering on will also be in . We now show that these preimages cluster on the sets (which are contained in the preimages of ). Specifically, we must show that for large enough , any point in for any is close to a preimage of one of the fixed points on . This task is made easier by the fact that by construction, the nonempty accumulate (when there are an infinite number of them) on the boundary of . To see this, define
[TABLE]
and note that for any , we have from construction that and . For any , the set has compact closure, so for any , there is a and points such that
[TABLE]
That is, we have a finite open cover of the set of all the sets: for all , there is an integer such that .
With this finite open cover, it is now straightforward to use Lemmas 3.1 and 3.3 to show that for all sufficiently large, each (a center of one of the balls in the open cover) is close to some , a preimage of a fixed point of on . Since each , we can choose large enough so that for all we have . Thus, for any for any , we have . ∎
It is intuitive by the construction of that points bound a definite distance away from will not be in for all sufficiently large . We nevertheless provide the formal statement and proof of this fact in the following lemma.
Lemma 3.4**.**
For any , there is an such that for any
[TABLE]
Proof.
First we consider the case in which . By Lemma 1.2 there is a large enough such that for all , we have . To attend to the remaining points, suppose and . However, since , we only need to consider with . Note that is a compact set, so there is some such that for all , we have . By Lemma 3.1, for all sufficiently large . Again, by Lemma 1.2, we have in this case as well. ∎
Lemma 3.5**.**
For any periodic orbit of contained in and any , there is an such that for all , has a periodic orbit also contained such that
[TABLE]
Moreover, if is attracting (repelling) for , then each cycle is attracting (repelling) for each corresponding .
While zeros of non-contant polynomials depend continuously on the coefficients of the polynomial, the set of polynomials is discrete. Nevertheless, Lemma 3.5 still follows quickly from Rouche’s theorem and the fact that on any compact subset of , we have uniformly and uniformly, so we omit the proof.
Proof of Theorem 1.4.
From Lemma 3.4, it follows that for all , . From this and Lemma 3.2, we have
[TABLE]
so it remains only to show that . A point must be an accumulation point of or in . In the former case, we have , so suppose the latter: , and let . Since repelling periodic points are dense in [14], there is a repelling periodic point such that . By Lemma 3.5, there is an such that for all , there is a repelling periodic point such that . Thus, . ∎
4. Hyperbolic and Other More Specific Maps
We turn our attention now to the more specific cases in which is hyperbolic and has no periodic points on .
Proof of Theorem 1.6.
By Theorem 1.4, it remains only to show that , the interior of , is a subset of . That is, we need only now show that any point of is close to for all sufficiently large . If is empty, we are done, so we proceed with the assumption that is nonempty.
Since is hyperbolic, we know that the orbit of every point in converges to an attracting periodic cycle for . Suppose is such an attracting cycle. We will show that for large enough , every has an attracting periodic near . Then every point in will have some forward image near an attracting cycle of , ensuring these points are in .
For each in the attracting cycle for , there is a neighborhood such that . Let . By Lemma 3.5, there is an such that for all , has an attracting periodic orbit where . By Lemma 3.1, there is an such that for all we also have . Thus, we have constructed a neighborhood that is forward invariant for all with , so this neighborhood must be contained in each .
We now show that compact subsets of are eventually mapped by into the forward invariant neighborhood we just constructed. Let and be a compact subset of such that for all , there is some such that . Then there is an such that
[TABLE]
Again by Lemma 3.1, there is an such that for all we also have
[TABLE]
Let . For all , it follows that the orbit by of any point converges to an attracting periodic cycle of contained in ; that is, . Then for any point , there is a such that . ∎
Proof of Corollary 1.5.
We prove the first part of the corollary. Suppose first that the image of under is contained in and let . By the open mapping theorem, we know is an open set in , so . Since , we have from the Denjoy-Wolff Theorem [14] that has a fixed point in to which orbits of all points in any compact subset of converge. We have assumed has no fixed points in , so , and in this case, we also have from the Denjoy-Wolff Theorem that is the unique fixed point in . From Lemma 3.5, we have that for all , there is an such that for all , has an attracting fixed point with and no other fixed points in . Thus, we have . Combining this with Lemma 1.2, for any , we may choose large enough such that
[TABLE]
Now suppose the image of under is not contained in , so is nonempty. Since is compact, is also compact, and since is open and is nonempty, there is some and such that and for any , we have . Then one can pick large enough that for any and any , we have . Then for all , .
For the second part of the theorem, assume under does not intersect , so . That is, for all , we have . Let
[TABLE]
so . Then . Since is compact, we may choose this so that for any , we have . Then for any , we also have
[TABLE]
By Lemma 1.2, it follows that is in the basin of infinity of for all . The result then follows from this fact and Lemma 3.2.
Lastly, suppose the image under does intersect . Then by Theorem 1.6, if the limit exists, is nonempty, so the limit cannot be . ∎
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