Abstract
The main objective of this paper is to study a new family of analytic functions that are q-starlike with respect to m-symmetrical points and subordinate to the q-Janowski function. We investigate inclusion results, sufficient conditions, coefficients estimates, bounds for Fekete–Szego functional and convolution properties for the functions belonging to this new class. Several consequences of main results are also obtained.
Keywords:
analytic functions; univalent functions; q-difference operator; q-starlike functions; m-symmetric points; Janowski functions; subordination; convolution MSC:
30C45; 30C50
1. Introduction
The concept of quantum calculus or q-calculus is ordinary calculus without the notion of limits. Recently, due to its wide applications in applied sciences [1,2,3], the area of q-calculus has attracted the serious attention of researchers [4,5,6,7]. Jackson [8,9] was the first who initiated the study of q-calculus by introducing q-analogue of ordinary derivative and integral. He defined and studied q-difference operator and q-integral operator in a systematic way. Ismail et al. [10] used the q-difference operator for the first time in geometric function theory by introducing the class of q-starlike functions. Later the study of q-calculus in geometric function theory was developed by many authors [11,12,13,14]. Several researchers studied the subclasses of analytic functions associated with the q-difference operator [13,15,16,17,18,19]. Raghavendar and Swaminathan [20] defined and studied some basic properties of q-close-to-convex functions. Agrawal and Sahoo [21] introduced the family of q-starlike functions of the order . The aim of the present work is to explore some properties of a subclass of analytic functions associated with q-Janowski functions involving a q-difference operator.
Let denote the family of functions f of the form
which are analytic in the open unit disc . Any function f is said to be univalent in a domain if it never takes the same value twice in . Let us denote by S the subclass of consisting of univalent functions in E. For two functions f and , we say that f is subordinate to g, written as , if there exists a Schwartz function which is analytic in E with and , for all , such that . If is univalent in E, then and For any function f defined by Equation (1) and given by , the convolution or Hadamard product of f and g is defined by
For the q-difference operator of a function is defined as
For , a natural generalization of Equation (3) is given by the convolution operator
which for , becomes the derivative and for , is equivalent to Equation (3). For f given by Equation (1), we have
where
We denote by P, the class of analytic functions p with
such that in E. Any function of the form in Equation (6) is said to be in the class if and only if
where The class was introduced by Janowski [22].
A function is said to belong to the class of starlike functions if, and only if,
which is equivalent to
Let denote the subclass of S, defined by
It is known that is the class of starlike functions of the order . This class consists of the functions with the property that
Chand and Singh [23] introduced and studied the class of starlike functions with respect to m-symmetric points, consisting of the functions such that
where , and It can be noted that
where
Kwon and Sim [24] studied the class which consists of the functions such that
In [10], Ismail et al. introduced the class as:
Definition 1.
A function is said to belong to the class if
or equivalently
By taking motivation from above-mentioned work and using a q-difference operator , for , we introduce the following new subclasses of analytic functions.
Definition 2.
A function is said to be in class if
or equivalently
Definition 3.
A function is in class if
where,
and
It is important to note that
Remark 1.
It is worth mentioning that the functions in class are not necessarily to be univalent in E. For example, is not univalent in E but one can easily verify that it belongs to classes and
1.1. Special Cases
- For is the class studied by Ismail et al. [10].
- For , is the class studied by Chand and Singh [23].
- For and , is the familiar class of starlike functions.
- For , is the class studied by Kwon and Sim [24].
- For , is the class studied by Janowski [22].
- For , is the class of starlike functions of the order , defined and studied by Roberston [25].
- For , is the class of starlike functions defined by Alexander [26].
- For , is the class of odd starlike functions studied by Sakaguchi [27].
1.2. Geometrical Interpretation
A function is in the class if, and only if, takes all values in the circular domain centred at and radius
2. A Set of Lemmas
The following lemmas are needed to prove our main results in the subsequent section.
Lemma 1
([28]). If is an analytic function with a positive real part in E and μ is a complex number, then This result is sharp for the functions given by
Lemma 2
([29]). If is an analytic function with a positive real part in E, then This result is sharp for the function given by
Lemma 3
([30]). Let . Then
Lemma 4
([31]). Let , and in E. If is convex univalent in E, then
3. Main Results
Theorem 1.
Let , then
Proof.
Since , therefore
Replacing z by where , we have
Using the properties and , we obtain
Since is a convex function, therefore applying summation and dividing by m, we obtain
That is □
Theorem 2.
If then
Proof.
The proof follows directly by using and applying Lemma 3. □
Theorem 3.
Using and in Theorem 3, we obtain the results of Ahuja [32].
Corollary 1.
Using and in Theorem 3, we obtain the following result of Silverman [33].
Corollary 2.
Theorem 4.
For any with , the polynomial functions
belong to the class for all
Proof.
By choosing and in Equation (15) and then applying Theorem 3 we obtain the required result. □
Theorem 5.
For any with , the polynomial functions
belong to the class for all
Proof.
By choosing and in Equation (15) and then applying Theorem 3 we obtain the required result. □
Theorem 6.
Proof.
Let is given by Equation (1) then
Similarly for , we have
Next we calculate the values of and . Taking
we obtain
Therefore,
From Equation (26), we obtain
Applying Lemma 2, we obtain the first part of the result. For the second part, using Lemma 1 we obtain
Note that
Hence, the result follows. □
Theorem 7.
If is given by (1), then
Proof.
Let
Comparing the coefficients of , we obtain
Since
therefore, by Lemma 4
Taking the absolute value of Equation (33) and using Equation (35), we obtain the following inequality
We shall use principle of mathematical induction to prove Equation (30). By taking in Equation (36) and using Equation (18), we have
which shows that Equation (30) is true for . Let us suppose Equation (30) holds for all . For from Equation (36), we see that
which shows the result is true for . Hence Equation (30) holds for all . □
Theorem 8.
Let , then for any , we have
where
For and , we obtain the following result for the class defined by Janowski [22].
Corollary 3.
Let then
For and , we obtain the following result which is a special case of the result proved in [34] and can be found in [35].
Corollary 4.
Let , then
For and , we obtain the following familiar Fekete–Szego inequality for starlike functions.
Corollary 5.
Let , then
Theorem 9.
If given by Equation (1) is univalent, then contains an open disc of radius
Proof.
Let be a complex number such that for . Then
is analytic and univalent, therefore,
The triangle inequality yields
Using Equation (18) we obtain
which implies
which shows the image of E under must cover an open disk with centre at the origin and radius . □
Theorem 10.
If , then
where and . The converse holds if for all .
Proof.
Assume that , then we have if, and only if, for all and The last condition can be written as
On the other hand,
and
Conversely, if the assumption in Equation (42) holds for and for all , then the function is analytic in E and . Since we have shown that Equations (42) and (43) are equivalent, therefore
For , Relation (45) shows that . Therefore, the simply connected domain is contained in a connected component of . Using the fact that together with the univalence of function ψ, it follows that which shows that . □
4. Conclusions
The q-calculus is an important area of study in the field of mathematics. It usually deals with the generalization of differential and integral operators. In recent years, it has attracted many researchers due to its wide range of applications in different fields of sciences such as quantum mechanics, physics, special functions, orthogonal polynomials, combinatorics and the related areas.This article concerns a generalization of the class of starlike functions using the q-difference operator and the concepts of m-symmetrical points. This work includes sufficiency criteria, coefficient estimates, bounds for Fekete–Szego functional and convolution results for a newly defined class. During this study, it is noted that the classes defined by the q-difference operator are larger than that defined by ordinary derivatives because they also contains non-univalent functions. For example, the function is not univalent in E but this belongs to classes and By using the technique presented in this article, an infinite sequence of functions can be generated for a wide range of subclasses of analytic functions which are special cases of the newly defined class. Hopefully, the results proved in this article will be beneficial to researchers in the field of geometric function theory.
Author Contributions
Conceptualization, K.I.N.; Methodology, I.G. and S.H.; Validation, I.G. and S.H.; Formal analysis, I.G. and S.A.-S.; Writing—original draft, I.G.; Writing—review & editing, S.A.-S.; Supervision, K.I.N. and S.H. All authors have contributed equally in writing the paper. All authors have read and agreed to the published version of the manuscript.
Funding
This research received no external funding.
Data Availability Statement
No data were used to support this study.
Conflicts of Interest
The authors declare no conflict of interest.
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