Abstract
In this paper, we aim to find sufficient conditions for the close-to-convexity of q-Bessel–Wright functions with respect to starlike functions, such as , and are in the open unit disc. Some consequences related to our main results are also included.
Keywords:
analytic functions; univalent functions; starlike functions; convex functions; close-to-convex functions; q-Wright functions MSC:
30C45; 30C50
1. Introduction and Preliminaries
Let denote the class of functions f of the form
which are analytic in the open unit disc Let be the subclass of which contains univalent functions in . For , the classes of starlike and close-to-convex functions of order can be analytically defined in as and and , respectively. It is clear that and are familiar classes of starlike and close-to-convex functions, respectively.
Now we give some basic notions and definitions about q-calculus. For , then q-number is defined by
Also, the q-factorial is given by
Let and Then the q-shifted factorial is defined by
Let Then q-Gamma function is given by
The q-derivative (or the q-difference) operator of a function f is defined, in a given subset of , by
provided exists. We can easily observe from the definition of that By using the q-derivative (or the q-difference) operator , the classes and of q-starlike and q-close-to-convex functions are defined as follows:
Definition 1
([1]). A function is said to be in the class if
Definition 2
([2]). A function is said to be in class if there exists a starlike function h such that
It is observed that, when the classes and reduce to the well-known classes and of starlike and close-to-convex functions, respectively.
Special functions play significant role in pure and applied mathematics. These functions have contributed a lot in geometric function theory, particularly in settling the famous Bieberbach conjecture. This use of special functions in function theory developed interest among researchers. There is an extensive literature dealing with geometric properties of different types of special functions. For instance, Owa and Srivastava [3] studied the univalence and starlikeness of hypergeometric functions. Srivastava and Dziok [4,5] introduced a convolution operator by using generalized hypergeometric function to study certain classes of univalent functions. Srivastava [6] introduced a convolution operator by using Fox–Wright function and studied certain classes of univalent functions while Baricz [7], Orhan and Yagmur [8], and Raza et al. [9] studied the properties of Bessel, Struve, and Wright functions respectively. Futher, a few more recent developements about Wright and Bessel functions can be accessed from [10,11,12,13,14].
Let and j be positive real number, let either and or , and Then, the q-Bessel–Wright function is defined by
The q-Bessel–Wright function was studied by Shahed and Salem [15], see also [16]. When the q-Bessel–Wright function reduces to the classical Bessel–Wright given as
The q-Bessel–Wright function generalizes various functions. It follows from the definition of the q-Bessel–Wright function (5) that where is q-analogue of exponential function which is given in [17] and defined as
We also see that the Jackson’s third q-Bessel function and modified third q-Bessel function can be written in the forms of q-Bessel–Wright function as
The q-error function complement is also a special case of q-Bessel–Wright function
The Wright function has a number of applications in the applied sciences. It is being used in the asymptotic theory of partitions, in Mikusinski operational calculus, and in the theory of integral transforms of the Hankel type. Wright functions have been found in the solution of partial differential equations of fractional order. It was found that the corresponding Green functions can be written in terms of the Wright function [18,19]. It has recently been used in the theory of coherent states [20]. For detailed applications of this outstanding function, refer to [21,22].
The function does not belong to the class . We consider the following form of as
Basic (or q-) calculus plays an important role in geometric function theory. In the context of function theory, the utilization of q-calculus was first applied by Srivastava [23], in which the basis of q-hypergeometric functions was also provided. Recently, by making use of the concept of basic (or q-) calculus, various families of q-extensions of starlike functions were introduced. After the study of q-hypergeometric functions, many researchers have shown keen interest in the q-analogues of some special functions. We include few of those. In [24,25,26] the authors discussed the radii of starlikeness and convexity of q-Bessel functions, whereas Hardy spaces of the same function were explored by Aktas [27]. Toklu [28] investigated the radii problem for q-Mittag–Leffler functions. Oraby and Mansour [29,30] investigated the zeros and radii of starlikeness and convexity for Bessel–Struve functions.
The q-close-to-convexity of q-hypergeometric function was first studied in [31]. Srivastava and Bansal [32], and Raza and Din [33] have studied q-close to convexity of q-Mittag–Leffler functions and the same problem for q-Bessel functions has recently been studied by Aktas and Din [34]. Motivated by these developments, we aim to study q-close to convexity of q-Bessel–Wright functions with respect to certain starlike functions.
The following lemmas are very useful for our study. These are based on the q-derivative of function f of the form (1). These results give sufficient conditions for q-close-to-convexity of functions with respect to certain starlike functions.
Lemma 1
([2]). Let and , and be a sequence of real numbers such that
Let
or
Then,
where
Lemma 2
([31]). Let be a sequence of real numbers such that
Let
or
Then,
where
Lemma 3
([35]). Let be analytic in and in addition or then, f is a close-to-convex function with respect to the convex function Moreover, if the odd function is analytic in and if or then h is univalent in .
2. Main Results
Theorem 1.
Let , and
Then, is q-close-to-convex in with respect to starlike function
Proof.
Consider
This expression can also be represented as
where
To prove that q-Bessel–Wright function is q-close-to-convex, we consider
so that
It can easily be seen that and all the values of are positive for all positive integers. Furthermore, from the Lemma 1, we have
Next, we will prove that
This implies that
which is equivalent to
To verify the inequality (9), consider
By the definition of q-gamma function, the above inequality becomes
From the above relation, we may write
This implies that
Now by the condition , we have
therefore,
Thus,
Hence the required result. □
Corollary 1.
The function where
Corollary 2.
The function Erfc where
Remark 1.
If we put in then it takes the form
which is true for . Hence the normalized q-Bessel–Wright function is q-close-to-convex in with respect to starlike function
Theorem 2.
Let , and
Then, the normalized q-Bessel–Wright function where
Proof.
Consider
This expression can also be represented as
where
To prove , consider
so that
It can easily be observed that and all the values of are positive for all positive integers. Furthermore, from the Lemma 2, we have
Next, we prove that
From the above inequality
which is equivalent to
To verify the inequality (13), consider
By the definition of q-gamma function, the above inequality takes the form
From the above relation, we may write
This implies that
Now, by the condition , we have
therefore,
Thus,
Hence we obtain the required result. □
Corollary 3.
The function where
Corollary 4.
The function Erfc where
Corollary 5.
If we put in then it takes the form
which holds true if and the normalized q-Bessel–Wright function where
Theorem 3.
Let , and
Then, the normalized q-Bessel–Wright function where
Proof.
Set
where
It is easy to see that for all and by a simple computation, we observe that
To prove that we use Lemma 3. Therefore, we have to show that is a decreasing sequence. Consider
For
we see that for all thus is a decreasing sequence. By Lemma 3, it follows that for □
Corollary 6.
Let , and
Then, where
Corollary 7.
Let , and
Then, Erfc where
Theorem 4.
Let , and
Then, where
Proof.
Set
Here therefore we have
and for all To prove our result we will prove that is a decreasing sequence. Take
For
we observe that for all ; thus, is a decreasing sequence. By Lemma 3, it follows that is close-to-convex with respect to the function □
Corollary 8.
Let , , and
Then, where
Corollary 9.
Let , , and
Then, Erfc where
3. Conclusions
We have presented here the study of q-Bessel–Wright functions. We have found sufficient conditions for the close-to-convexity of these functions with respect to the starlikeness of the functions , and in the open unit disc. In addition to that, certain consequences of our results as corollaries have also been discussed for reference.
These results will motivate researchers to study q-close-to-convexity of some other special functions such as q-Struve–Bessel functions, q-Lommel functions. Furthermore, q-close-to-convexity with respect to some other starlike functions such as and can be studied.
Author Contributions
Conceptualization, M.U.D., M.R. and Q.X.; methodology, M.U.D., M.R. and Q.X.; software, S.N.M.; validation, S.N.M. and S.Y.; formal analysis, M.R. and S.Y.; investigation, M.U.D., M.R. and Q.X.; resources, S.N.M.; data curation, S.Y.; writing—original draft preparation, S.N.M. and M.R.; writing—review and editing, S.N.M.; visualization, M.R. and S.Y.; supervision, M.R.; project administration, M.R., M.U.D. and S.N.M.; funding acquisition, M.R. and S.N.M. 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 is used in this work.
Acknowledgments
The authors acknowledge the heads of their institutes for support and providing research facilities.
Conflicts of Interest
The authors declare no conflict of interest.
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