Geometric Properties of Partial Sums of Univalent Functions
Key words and phrases:
univalent function, starlike function, convex function, sections, partial sums2010 Mathematics Subject Classification:
30C45, 30C80The th partial sum of an analytic function is the polynomial . A survey of the univalence and other geometric properties of the th partial sum of univalent functions as well as other related functions including those of starlike, convex and close-to-convex functions are presented.
1. Introduction
For , let be the open disk of radius centered at and be the open unit disk. An analytic function is univalent in the unit disk if it maps different points to different points. Denote the class of all (normalized) univalent functions of the form
(1.1) |
by . Denote by , the class of all analytic functions of the form (1.1). The Koebe function defined by
is univalent and it is also extremal for many problems in geometric function theory of univalent functions. A domain is starlike with respect to a point if every line segment joining the point to any other point in lies completely inside . A domain starlike with respect to the origin is simply called starlike. A domain is convex if every line segment joining any two points in lies completely inside ; in other words, the domain is convex if and only if it is starlike with respect to every point in . A function is starlike if is starlike (with respect to the origin) while it is convex if is convex. The classes of all starlike and convex functions are respectively denoted by and . Analytically, these classes are characterized by the equivalence
and
More generally, for , let and be the subclasses of consisting of respectively starlike functions of order , and convex functions of order . These classes are defined analytically by the equivalence
and
Another related class is the class of close-to-convex functions. A function satisfying the condition
for some (not necessarily normalized) convex univalent function , is called close-to-convex of order . The class of all such functions is denoted by . Close-to-convex functions of order are simply called close-to-convex functions. Using the fact that a function with
is in , close-to-convex functions can be shown to be univalent.
The th partial sum (or th section) of the function , denoted by , is the polynomial defined by
The second partial sum of the Koebe function is given by
It is easy to check directly (or by using the fact that for ) that this function is univalent in the disk but, as , not in any larger disk. This simple example shows that the partial sums of univalent functions need not be univalent in .
The second partial sum of the function is the function . If , then and its properties are clear. Assume that . Then the function satisfies, for , the inequality
provided . Thus the radius of starlikeness of is . Since is convex in if and only if is starlike in , it follows that the radius of convexity of is . If is univalent or starlike univalent, then and therefore the radius of univalence of is 1/4 and the radius of convexity of is 1/8. (See Fig. 1 for the image of and under the function .) For a convex function as well as for functions whose derivative has positive real part in , and so the radius of univalence for the second partial sum of these functions is 1/2 and the radius of convexity is 1/4. In [25], the starlikeness and convexity of the initial partial sums of the Koebe function and the function are investigated.

It is therefore of interest to determine the largest disk in which the partial sums of the univalent functions are univalent. Szegö also wrote a survey [50] on partial sums in 1936. In the present survey, the various results on the partial sums of functions belonging to the subclasses of univalent functions are given. However, Cesàro means and other polynomials approximation of univalent functions are not considered in this survey.
2. Partial sums of univalent functions
The second partial sum of the Koebe function indicates that the partial sums of univalent functions cannot be univalent in a disk of radius larger than 1/4. Indeed, by making use of Koebe’s distortion theorem and Löwner’s theory of univalent functions, Szegö [49] in 1928 proved the following theorem.
Theorem 2.1 (Szegö Theorem).
The partial sums of univalent functions are univalent in the disk and the number cannot be replaced by a larger one.
Using an inequality of Goluzin, Jenkins [14] (as well as Ilieff [12], see Duren [4, §8.2, pp. 241–246]) found a simple proof of this result and also shown that the partial sums of odd univalent functions are univalent in . The number is shown to be the radius of starlikeness of the partial sums of the odd univalent functions by He and Pan [10]. Iliev [13] investigated the radius of univalence for the partial sums , , of univalent function of the form . For example, it is shown that is univalent in , and is univalent in , for all . He has also shown that is univalent in for . Radii of univalence are also determined for and , as functions of , and for as a function of .
Szegö’s theorem that the partial sums of univalent functions are univalent in was strengthened to starlikeness by Hu and Pan [11]. Ye [53] has shown that the partial sums of univalent functions are convex in and that the number 1/8 is sharp. Ye [53] has proved the following result.
Theorem 2.2.
Let and
Then are convex in . The radii of convexity are sharp.
Ruscheweyh gave an extension of Szegö’s theorem that the th partial sums are starlike in for functions belonging not only to but also to the closed convex hull of .
Let where stands for the closed convex hull. Convolution of two analytic functions and is the function defined by
Ruscheweyh [33] proved the following theorem.
Theorem 2.3.
If and , then is starlike in . The constant 1/4 is best possible.
In particular, for , Theorem 2.3 reduces to the following result.
Corollary 2.1.
If belongs to or, in particular, to the class of the normalized typically real functions, then the th partial sum is starlike in . The constant 1/4 is best possible.
The class contains the following two subsets:
and
Since the class of convex functions is a subset of , it is clear that . For , Theorem 2.3 reduces to the following:
Corollary 2.2.
If belongs to , then the function and, in particular, the th partial sum , is convex in . The constant 1/4 is best possible.
We remark that Suffridge [48] has shown that the partial sums of the function are all convex. More generally, Ruscheweyh and Salinas [35] have shown that the functions of the form , are either constant or convex univalent in the unit disk . Let be analytic . Reade [27] obtained the radius of univalence for the partial sums when is univalent or when in .
3. Partial sums of starlike functions
Szegö [49] showed that the partial sums of starlike (respectively convex) functions are starlike (respectively convex) in the disk and the number cannot be replaced by a larger one. If is fixed, then the radius of starlikeness of can be shown to depend on . Motivated by a result of Von Victor Levin that the th partial sum of univalent functions is univalent in where for , Robertson [28] determined such that the th partial sum to have certain property in when the function has the property in . He considered the function has one of the following properties: is starlike, has positive real part, is convex, is typically-real or is convex in the direction of the imaginary axis and is real on the real axis. An error in the expression for was later corrected in his paper [29] where he has extended his results to multivalent starlike functions.
The radius of starlikeness of the th partial sum of starlike function is given in the following theorem.
Theorem 3.1.
An analytic function is -valently starlike [29, p. 830] if assumes no value more than times, at least one value times and
For -valently starlike functions, Robertson [29, Theorem A, p. 830] proved that the radius of -valently starlikeness of the th partial sum is at least . Ruscheweyh [32] has given a simple proof that the partial sums of -valently starlike (or close-to-convex) function is -valently starlike (or respectively close-to-convex) in .
Theorem 3.2.
If is a starlike function, then every partial sum of is convex in and the number 1/8 cannot be increased.
In view of the above theorem, the th partial sum of Koebe function is convex in . A verification of this fact directly can be used to give another proof of this theorem by using the fact [34] that the convolution of two convex function is again convex. It is also known [34] that for a function starlike of order 1/2. This result was extended by Singh and Paul [45] in the following theorem.
Theorem 3.3.
If , then
provided that and are both nonnegative with at least one of them nonzero or provided that is a complex number with . The result is sharp in the sense that the ranges of and cannot be increased.
4. Partial sums of convex functions
For a convex function , it is well-known that . Extending this result, Sheil-Small [36] proved the following theorem.
Theorem 4.1.
If , then the th partial sum of satisfies
and hence
(4.1) |
As a consequence of this theorem, he has shown that the function given by is a close-to-convex univalent function. In fact, the inequality (4.1) holds for as shown in [34]. The inequality (4.1) also holds for odd starlike functions as well as for functions whose derivative has real part greater than 1/2 [46].
Recall once again that [49] the partial sums of convex functions are convex in the disk and the number cannot be replaced by a larger one. A different proof of this result can be given by using results about convolutions of convex functions. In 1973, Ruscheweyh and Shiel-Small proved the Polya-Schoenberg conjecture (of 1958) that the convolution of two convex univalent functions is again convex univalent. Using this result, Goodman and Schoenberg gave another proof of the following result of Szegö [49].
Theorem 4.2.
If is convex function, then every partial sum of is convex in .
Proof.
The convex function is extremal for many problems associated with the class of convex functions. By Szegö’s result the partial sum of is convex in and therefore is a convex univalent function. If is also convex, then its convolution with the convex function is convex and so is convex. Therefore, the partial sum of the convex function , as , is convex in . In view of this discussion, another proof of Szegö result comes if we can directly show that is convex in . This will be done below.
A calculation shows that
where , and . The bilinear transformation maps onto the disk and hence
It is therefore enough to show that
as this inequality together with yield
Now, for , we have
and so
Therefore, it follows that
holds if
or equivalently
The last inequality becomes an equality for and the right hand side expression is an increasing function of . ∎
Let denote the class of functions analytic and satisfying the condition for . Bernardi [3] proved that the sharp inequality
holds for , , and . He has also shown that, for any complex , ,
For a convex function , he deduced the sharp inequality
Making use of this inequality, he proved the following theorem.
Theorem 4.3.
[3, Theorem 4, p. 117] If is convex, then the th partial sum is starlike in where is the positive root of the equation . The result is sharp for each even for .
The above theorem with a weaker conclusion that is univalent was obtained earlier by Ruscheweyh [31]. Singh [44] proved that the th partial sum of a starlike function of order 1/2 is starlike in where is given in Theorem 4.3. He has also shown that the conclusion of Theorem 4.3 can be strengthened to convexity if one assumes that is a convex function of order 1/2. In addition, for a convex function of order 1/2, he has shown that and 1/2 is sharp. It is also known that all the partial sums of a convex function of order 1/2 are close-to-convex with respect to itself and that there are convex functions of order whose partial sums are not univalent [30]. Singh and Puri [46] have however shown that each of the partial sums of an odd convex function is close-to-convex with respect to .
Silverman [38] also proved Theorem 4.3 by finding the radius of starlikeness (of order ) of the th partial sums of the function . The result then follows from the fact that the classes of convex and starlike functions are closed under convolution with convex functions.
Lemma 4.1.
The function is starlike of order in where is the smallest positive root of the equation
The result is sharp for even .
Proof.
The bilinear transformations maps the circular region onto the circle
Similarly
Since
it follows that, for ,
The above inequality shows that
provided
The sharpness follows easily. ∎
Theorem 4.4.
[38, Theorem 1, p. 1192] If is convex, then the th partial sum is starlike in for all . In particular, is starlike in and the radius 1/2 is sharp.
Proof.
In view of the previous lemma, it is enough to show that
for . For , the above inequality is equivalent to
which holds for .
The second result follows as is an increasing function of and from the fact that, for , . ∎
Silverman [38, Corollary 2, pp. 1192] also proved that the th partial sum of a convex function is starlike in for and the radius is sharp. For a convex function , its th partial sum is shown to be starlike of order in , convex of order in and the radii are sharp.
A function is uniformly convex, written , if maps every circular arc contained in with center onto a convex arc. The class of parabolic starlike functions consists of functions satisfying
In other words, the class consists of functions where . A survey of these classes can be found in [1].
Lemma 4.2.
The function is in for where is the smallest positive root of the equation
The result is sharp for even .
Proof.
Theorem 4.5.
If is convex of order 1/2, then the partial sums are uniformly convex for where is the smallest positive root of
Proof.
For the function convex of order 1/2, the function is starlike of order 1/2. Since is uniformly convex in ,
is uniformly convex in . ∎
5. Functions whose derivative is bounded or has positive real part
Theorem 5.1.
Proof.
The function is starlike in if
This sufficient condition is now well-known (Alexandar II) and it was also proved by Noshiro [21]. The Parseval- Gutzmer formula for a function analytic in is
Using this formula for and noting that , it follows that
Now, by using the Cauchy- Schwarz inequality, it readily follows that, for ,
The sharpness follows from the function given by
its derivative vanishes at . ∎
Nabetani [20] noted that Theorem 5.1 holds even if the inequality is replaced by the inequality
He has shown that the radii of starlikeness and convexity of functions satisfying the inequality
are respectively the positive root of the equations
and
For functions whose derivative has positive real part, MacGregor [18] proved the following result.
Theorem 5.2.
If the analytic function given by (1.1) satisfies the inequality , then is univalent in .
Proof.
Theorem 5.3.
[28] If is analytic and has positive real part in , then, for , has positive real part in where is the root in (0,1) of the equation
Singh [43] investigated the radius of convexity for functions whose derivative has positive real part and proved the following result.
Theorem 5.4.
If the analytic function given by (1.1) satisfies the inequality , then is convex in . The number 1/4 cannot be replaced by a greater one.
Extending Theorem 5.2 of MacGregor, Silverman [42] has shown that, whenever , is univalent in , where is the smallest positive root of the equation , and the result is sharp for even. He also shown that and for . Also he proved that the sharp radius of univalence of is . Yamaguchi [51] has shown that is univalent in if the analytic function given by (1.1) satisfies the inequality .
Let and denote by the class of functions that are regular and univalent in the unit disc and satisfy . Let . Kudelski [17] proved the following results. The corresponding results for were proved by Aksentév [2].
Theorem 5.5.
Let . Then in the disc , where is the least positive root of the equation . Also is univalent for , where is the least positive root of .
6. Close-to-convex functions
Recall that a function satisfying the condition
for some (not necessarily normalized) convex univalent function , is called close-to-convex. In this section, some results related to close-to-convex functions are presented.
Theorem 6.1.
The function satisfying the hypothesis of the above theorem is clearly close-to-convex. This theorem implies that is also close-to-convex for and therefore it is a generalization of Szegö result. The result applies only to a subclass of the class of close-to-convex functions as is assumed to be normalized. Ogawa [24] proved the following two theorems.
Theorem 6.2.
If is analytic and satisfy
where is starlike univalent, then, for each ,
and the constant cannot be replaced by any greater one.
Theorem 6.3.
Let , be analytic and satisfy
where is schlicht and convex in . Then, for each ,
The constant cannot be replaced by any greater one.
Theorem 6.4.
[9] Let , be analytic and satisfy
where is starlike in . Then, for each ,
The constant cannot be replaced by any greater one.
A domain is said to be linearly accessible if the complement of can be written as the union of half-lines. Such a domain is simply connected and therefore, if it is not the whole plane, the domain is the image of the unit disk under a conformal mapping. Such conformal mappings are called linearly accessible. For linearly accessible functions, Sheil-Small [37] proved the following theorem.
Theorem 6.5.
If be linearly accessible in , then
7. Partial sums of functions satisfying some coefficient inequalities
Silverman [41] considered functions of the form satisfying one of the inequalities
where . These coefficient conditions are sufficient for to be starlike of order and convex of order , respectively. If satisfies either of the inequalities above, the partial sums also satisfy the same inequality.
Silverman [41] obtained the sharp lower bounds on , , , and for functions satisfying either one of the inequalities above. In fact, he proved the following theorem.
Theorem 7.1.
If the analytic function satisfies
for some , then
The inequalities are sharp for the function
Silverman [41] also proved a similar result for function satisfying the inequality . These results were extended in [7] for classes of functions satisfying an inequality of the form .
For functions belonging to the subclass , it is well-known that for . A function whose coefficients satisfy the inequality for are analytic in (by the usual comparison test) and hence they are members of . However, they need not be univalent. For example, the function
satisfies the inequality but its derivative vanishes inside and therefore the function is not univalent in . For the function satisfying the inequality , Gavrilov [8] showed that the radius of univalence of and its partial sums is the real root of the equation while, for the functions whose coefficients satisfy , the radius of univalence is . Later, in 1982, Yamashita [52] showed that the radius of univalence obtained by Gavrilov is also the same as the radius of starlikeness of the corresponding functions. He also found lower bounds for the radii of convexity for these functions. Kalaj, Ponnusamy, and Vuorinen [15] have investigated related problems for harmonic functions. For functions of the form whose Taylor coefficients satisfy the conditions , , and , or () for , the sharp radii of starlikeness and convexity of order , , are obtained in [26]. Several other related results can also be found.
Theorem 7.2.
Let , , and for . Then satisfies the inequality
where is the real root in of the equation
The number is also the radius of starlikeness of order . The number is the radius of parabolic starlikeness of the given functions. The results are all sharp.
8. Partial sums of rational functions
Define to be the class of all analytic functions satisfying the condition
It is well-known that consists of only univalent functions. In this section, we consider the partial sums of functions belonging to . All the results in this section are proved by Obradović and Ponnusamy [22].
Theorem 8.1.
If has the form
(8.1) |
such that is real and non-negative for each , then for each
In particular,
in the disk , where is the unique positive root of the equation:
(8.2) |
and, for , we also have .
The values of corresponding to from (8.2) are , , , respectively.
Theorem 8.2.
Theorem 8.3.
Suppose that and is its partial sum. Then for each
Proof.
Let so that
is its -th partial sum. Also, let
Then
where and
for By de Branges theorem, for all , and therefore, we obtain that
and that for (by the Cauchy-Schwarz inequality)
From Theorem 8.2, we deduce that , while for we have
in view of the inequalities
it follows easily that
which, in particular, implies that
This inequality, together with the fact that , gives that
for . The proof is complete. ∎
As a corollary, the following result holds.
Corollary 8.1.
Suppose that . Then for one has
or equivalently
When the second Taylor coefficient of the function vanish, the following results hold.
Theorem 8.4.
If i.e. belongs to the class , then the -th partial sum is in the class in the disk , where is the unique positive root of the equation
In particular, for , we have
For , one has
respectively.
Theorem 8.5.
Let i.e. belong to the class . Then for each integer , we have
in the disk
9. Generalized Partial Sum
By making use of the fact that the convolution of starlike with a convex function is again a starlike function, Silverman [38] has proved the following result.
Theorem 9.1.
If is convex, then , , is starlike in . The bound is sharp for every .
The proof follows from the following inequality satisfied by :
Since attains its minimum when , it follows that, for a convex function , the is starlike in . Since the radius of convexity of is , it follows that is convex in whenever is convex.
To an arbitrary increasing sequence (finite or not) of integers with and a function , the function is called the generalized partial sum of the function . For the generalized partial sum of convex mappings, Fournier and Silverman [5] proved the following results.
Theorem 9.2.
If is convex, then the generalized partial sum of the function is
-
(1)
convex univalent in where is the unique root in of the equation
-
(2)
starlike univalent in where is the unique root in of the equation
The function associated with the convex function is extremal for the radii of convexity and starlikeness.
These results are proved by using the information about neighborhoods of convex functions. They [5] also proved that, for a starlike function , the generalized partial sum is starlike in where is as above or in other words,
(9.1) |
where is the class of starlike univalent functions. The above implication in (9.1) is also valid for the classes of convex univalent functions and close-to-convex functions and the class consisting of functions for which for all starlike univalent functions . They [6] later showed that the implication in (9.1) is also valid for the class of univalent functions by proving the following theorem.
Theorem 9.3.
If , then the generalized partial sum of the function satisfies for all , where is as in Theorem 9.2. The function and show that the result is sharp.
For the class of functions in for which , , Silverman [39] proved the following result and some related results can be found in [40].
Theorem 9.4.
Let denote the positive root of the equation . If , then for . The result is sharp, with extremal function .
For functions , it is also known [47] that the th partial sum of satisfies and hence is univalent. Also .
Acknowledgement
The author is thankful to Sumit Nagpal for carefully reading this manuscript.
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