Abstract
In this paper, we consider some relations related to the representations of starlike and convex functions, and obtain some sufficient conditions for starlike and convex functions by using the theory of differential subordination. Actually, we generalize a result by Suffridge for analytic functions with missing coefficients and then we apply that generalization for obtaining the different methods to the implications of starlike or convex functions. Our results generalize and improve the previous results in the literature.
Keywords:
analytic functions; differential subordination; fixed initial coefficient; starlike functions; convex functions MSC:
30C45; 30C80
1. Introduction
We let denote the class of analytic functions in the open unit disk and define
where and n is a positive integer number. Furthermore, we introduce the subclass of as follows:
In particular, we set . As usual, let the subclass of be the class of all univalent functions in the open unit disk . A function is said to be starlike of order , written , if it satisfies
Specifically, we put . Every element in is called a starlike function. Furthermore, a function is said to be convex of order written , if it satisfies
In particular, we put . Every element in is called a convex function. Now for analytic functions in with the fixed initial coefficient, we define the class as follows:
where n is a positive integer number, and are fixed numbers. Moreover we assume
where n is a positive integer number and is a fixed number. In addition, we set . Assume f and g be in . We say that the function f is subordinate to g, denoted by , if there exists an analytic function in , with and , such that . Moreover, if g is an univalent function in , then if and only if and .
By considering the function , we can generalize the class of starlike functions as follows:
Let and . Then it is said that if and only if
Through (1), it can be easily observed that with maps the open unit disc onto the open disc with the center and the radius . Thus, for all , the relation holds and hence . Moreover for the different values of A and B, other types of the class such as the class , which is equivalent to the class , also for , the class which is equivalent to and are obtained.
The theory of differential subordination has a key role in the study of geometric function theory. In 1935 Goluzin [1] considered the subordination and proved that if h is convex then . Furthermore, in 1970 Suffridge [2] showed that Goluzin’s result is true if h is starlike. Moreover, Miller and Mocanu by writing many research papers in this direction extended the concept of differential subordination (see for example [3] and references therein). Further, many authors have recently using different combinations of the representations of starlike and convex functions have obtained the simple conditions for starlikeness and convexity of analytic functions. In [4], Silverman gained the results for analytic functions including the terms as the quotient of the analytic representations of convex and starlike functions. For instance, Silverman proved that , where and
Next, Obradovic and Tuneski [5], in view of , improved the work of Silverman. Indeed, they established for . Nunokawa et al. [6], by applying the Silverman’s quotient function [4], proved that f could be strongly starlike, strongly convex or starlike in . In [7,8,9,10], the authors have studied some conditions for the analytic functions to belong to the class . In [11], some results related to the above discussion, with respect to n-symmetric points of functions, have been given. Inspired by [9,10], in this paper, we will extend and improve some results obtained in [9,10] and then we will determine some conditions which by means of them, a function belongs to the class .
The contents of this article are regulated as follows: In Section 3, initially, we will prove a theorem that is the extension of a little change to the Suffridge theorem [3]. Next, we bring some applications of this theorem as the main results, making the functions be in the class . These results extend and improve some results in [10]. In Section 4, we intend to bring some sufficient conditions for starlikeness of analytic functions. We also produce the functions belonging to the class by considering other conditions, and so we include some corollaries from the result acquired. Furthermore, these results extend and improve some results in [9]. Moreover, Suffridge’s result is used in recent investigations like [12,13,14,15]. Note that some results related to this article for analytic functions with fixed initial coefficients are also mentioned.
In the continuation of the argument, in order to prove the main results, we require to remind a definition and two basic lemmas:
Definition 1.
(see [3]) Let Q denote the set of functions q that are analytic and injective on , where
and are such that for .
Lemma 1.
(see [3] ) Let with , and let be analytic in with and . If p is not subordinate to q, then there exist points and , and an for which ,
- (i)
- ,
- (ii)
- , and
- (iii)
- .
Lemma 2.
(see [16]) Let with and with . If there exist a point such that and , then
and
where and
2. Main Results
First, we mention a lemma which is slightly different from the original one, ([3], Th 3.4 h).
Lemma 3.
Let q be univalent in and functions θ and ϕ be analytic in a domain containing and for . Moreover, let
- (i)
- be starlike and
- (ii)
If , with , and
then and is the best dominant.
Proof.
Let us define . It easy to verify that the conditions (i) and (ii) imply that h is close-to-convex and hence univalent in . Now using the same argument as the proof of ([3], Th 3.4h), we get our result and we omit the details of the proof. □
By considering in Lemma 3, we extend a little change of the Suffridge theorem [3] as follows:
Corollary 1.
Let q be univalent in and . Moreover, let ϕ be analytic in a domain D containing and let . If is starlike in , then
and q is the best -dominant.
Using the same argument of Lemma 3 and applying Lemma 1, we obtain the following theorem, and we omit its proof:
Theorem 1.
Let q be univalent in and . Furthermore, let ϕ be analytic in a domain D containing and let with . If is starlike in , then
By putting in Lemma 3 and Theorem 1, we reach to the following corollaries:
Corollary 2.
Let q be convex univalent in with . If and
then .
Corollary 3.
Let q be convex univalent in with . If with and
then .
Corollary 4.
Let . Suppose that A and B are real numbers with . If
then .
Proof.
Let us define and . A simple computation and yield
On the other hand, q is convex in with , consequently by applying Corollary 2, we deduce that and hence . □
By applying the same argument as Corollary 4, and using Corollary 3 we have:
Corollary 5.
Let , and A and B be real numbers with and . If
then .
Setting in Corollary 4, we obtain:
Corollary 6.
Let . Moreover, let A and B be real numbers with . If
then .
Setting in Corollary 5, we obtain:
Corollary 7.
Let , and A and B be real numbers with and . If
then .
Putting in Corollary 6, we get to the following corollary:
Corollary 8.
Let . Moreover, let B be a real number with . If
for all , we have
Putting in Corollary 7, we come to the following corollary:
Corollary 9.
Let . Moreover, let B be a real number with and . If
for all , then
Remark 1.
Corollary 4, Corollary 6 and Corollary 8, respectively, extend and improve Lemma , Theorem and Corollary in [10].
3. Further Results about Analytic Functions to Settle in the Class
It is well known that for , the condition is sufficient for starlikeness of f. In this section, we will extend this result and will also try to bring other sufficient conditions for starlikeness.
Theorem 2.
Let A and B be real numbers with . Suppose that and in . If
then
Proof.
Let us define , and . For proving this theorem, it is sufficient to show that the conditions of Lemma 3 hold. However, we note that the condition (i) is equivalent to
where . Since
we attain the assertion of condition (i). On the other hand, from
we observe (ii). Moreover, the condition is correct and consequently the proof is completed. □
By putting and in Theorem 2 we obtain:
Corollary 10.
Let and with in . If
then f is starlike.
Proof.
Let us define . By some calculations, one can observe that . However, the function takes the the minimum value at the point and so . Hence, h maps unit disk onto the complement of and the proof is completed. □
By using Corollary 10, we have:
Corollary 11.
Let with in . If
- (i)
- (ii)
then f is starlike and the result is sharp for the function .
By putting , and in Theorem 2, we obtain:
Corollary 12.
Let with in . If
then f is starlike of order and the result is sharp for the function .
We remark that Corollary 12 is the generalization of Marx-Strohhcker Theorem (see [17]). By putting , and in Theorem 2 we gain:
Corollary 13.
Let with in . If
then
and the result is sharp for the function .
Theorem 3.
Let with in . Moreover, let A and B be real numbers with . If
where
then
In particular, if
then f is convex in .
Proof.
Let us define and . It can be readily observed that and q is convex univalent in . We claim that , otherwise there exist points and , and an such that
With some calculations and so utilizing , one can obtain
By letting , where and using (8), we have
Letting and defining
we have
In view of we deduce that g is an increasing function and takes its minimum at the point . Hence
for all . Therefore
which contradicts , and so this give the result. Since , we have
Now combining , and , we have
and so f is convex. □
With the same approach as the previous theorem and by applying Lemma 1, we attain the following theorem which we omit the proof of.
Theorem 4.
Let with in . Moreover, let A and B be real numbers with and . If
where
then
In particular, if and
then f is convex in .
By putting and letting , we obtain , where is given in Theorem 4. Now let . Since , we have . Hence we gain:
Corollary 14.
Let with in and . If
then
and . In particular, if , then , and f is convex in .
Remark 2.
Theorem 4 and Corollary 14 extend and improve Theorem 1 and Corollary 1 in [9], respectively.
By setting , and letting , we obtain , where is given in Theorem 4. Now let . Since , we have . So we obtain:
Corollary 15.
Let with in and . If
then
and . In particular, if , then , and f is convex in .
Corollary 16.
Let be an odd function with in . If and
then . In particular, if , then and f is convex in .
Proof.
Since f is odd function, we have . Putting in Corollary 15, the desired result is obtained. □
Example 1.
Let with . We know that f is an odd analytic function. On the other hand, one can see that
Therefore making use of Corollary 16, if and , then . In addition, if and , then f is convex.
Finally we prove the following result:
Theorem 5.
Let and with in . If
then f is a starlike function.
Proof.
Let us define and . We will show that . Suppose that p is not subordinate to q. Then from Lemma 1 there exist two points and such that and , where . Thus, with and . Furthermore with some calculations we find that
and so
If we denote
where , then it is easy to check that , then h is a decreasing function, Hence and
However, this contradicts . Hence the proof is completed. □
4. Conclusions
In this paper, we have proved a result similar to Suffridge’s theorem and given some applications related to this result. Moreover, we have investigated some sufficient conditions for starlikeness of analytic functions and functions that are in the class .
Author Contributions
Conceptualization: S.S., R.A. (Rasoul Aghalary) and A.E., original draft preparation: R.A. (Rasoul Aghalary), writing—review and editing: A.E. and N.E.C. investigation: R.A. (R. Alavi). All authors have read and agreed to the published version of the manuscript.
Funding
This research received no external funding.
Data Availability Statement
Not applicable.
Acknowledgments
The authors thank the anonymous referees for their invaluable comments in improving the first draft of this paper.
Conflicts of Interest
The authors declare no conflict of interest.
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