1. Introduction
The basic (or
q-) calculus is the ordinary classical calculus without the notion of limits, while
q stands for the quantum. The application of the
q-calculus was initiated by Jackson [
1,
2]. Later, geometrical interpretation of the
q-analysis was recognized through studies on quantum groups. It also suggests a relation between integrable systems and
q-analysis. Aral and Gupta [
3,
4,
5] defined and studied the
q-analogue of the Baskakov-Durrmeyer operator, which is based on the
q-analogue of the beta function. Some other important
q-generalizations and
q-extensions of complex operators are the
q-Picard and the
q-Gauss-Weierstrass singular-integral operators, which are discussed in [
6,
7,
8].
In Geometric Function Theory, several subclasses of the normalized analytic function class
have already been analyzed and investigated through various perspectives. The
q-calculus provides valuable tools that have been extensively used in order to examine several subclasses of the normalized analytic function class
in the open unit disk
. Ismail et al. [
9] were the first to use the
q-derivative operator
in order to study a certain
q-analogue of the class
of starlike functions in
(see Definition 6 below). Mohammed and Darus [
10] studied the approximation and geometric properties of these
q-operators in some subclasses of analytic functions in a compact disk. These
q-operators are defined by using the convolution of normalized analytic functions and
q-hypergeometric functions, where several interesting results were obtained (see [
11,
12]). Certain basic properties of the
q-close-to-convex functions were studied by Raghavendar and Swaminathan [
13]. Aral et al. [
14] successfully studied the applications of the
q-calculus in operator theory. Kanas and Raducanu [
15] used the fractional
q-calculus operators in investigations of certain classes of functions, which are analytic in the open unit disk
by using the idea of the canonical domain. The coefficient inequality problems for
q-closed-to-convex functions with respect to Janowski starlike functions were studied recently (see, for example, [
16]). In the year 2016, Wongsaijai and Sukantamala [
17] published a paper, in which they generalized certain subclasses of starlike functions in a systematic way. In fact, they made a very significant usage of the
q-calculus basically in the context of Geometric Function Theory. Moreover, the generalized basic (or
q-) hypergeometric functions were first used in Geometric Function Theory in a book chapter by Srivastava (see, for details [
18], (p. 347 et seq.); see also [
19]).
Motivated by the works of Wongsaijai and Sukantamala [
17] and other related works cited above in this paper, we shall consider three new subfamilies of
q-starlike functions with respect to Janowski functions. Several properties and characteristics, for example, sufficient conditions, inclusion results, distortion theorems, and radius problems, shall be discussed in this investigation. We shall also point out some relevant connections of our results with the existing results.
We denote by
the class of functions that are analytic in the open unit disk:
where
is the set of complex numbers. Let
be the subclass of functions
, which are represented by the following Taylor-Maclaurin series expansion:
that is, which satisfy the normalization condition given by
Furthermore, let be the class of functions in , which are univalent in .
The familiar class of starlike functions in
will be denoted by
which consists of normalized functions
that satisfy the following conditions:
For two functions
f and
g, which are analytic in
, we say that the function
f is subordinate to
g and write
if there exists a Schwarz function
w, which is analytic in
with
such that
In particular, if the function
g is univalent in
, then we have the following equivalence (cf., e.g., [
20]; see also [
21]):
We next denote by
the class of analytic functions
p in
, which are normalized by
such that
In the next section (
Section 2), we first give some basic definitions and concept details. Thereafter we will demonstrate three (presumably new) subclasses of the class
of
q-starlike functions associated with the Janowski functions.
2. A Set of Definitions
Throughout this paper, we suppose that
and that
Definition 1. (See [
22])
A given function h with is said to belong to the class if and only if The analytic function class
was introduced by Janowski [
22], who showed that
if and only if there exists a function
such that
Definition 2. A function is said to belong to the class if and only if there exists a function such that Definition 3. Let , and define the q-number by Definition 4. Let , and define the q-factorial by Definition 5. (See [
1,
2])
The q-derivative (or the q-difference) operator of a function f is defined, in a given subset of byprovided that exists. We note from Definition 5 that
for a function
f, which is differentiable in a given subset of
. It is readily deduced from (
1) and (
5) that
Definition 6. (See [
9])
A function is said to belong to the class of q-starlike functions in ifand We readily observe that, as
, the closed disk:
becomes the right-half complex plane, and the class
of
q-starlike functions in
reduces to the familiar class
of normalized starlike functions with respect to the origin
. Equivalently, by using the principle of subordination between analytic functions, we can rewrite the conditions in (
7) and (
8) as follows (see [
16]):
We now introduce three (presumably new) subclasses of the class of q-starlike functions associated with the Janowski functions in the following way.
Definition 7. A function is said to belong to the class if and only ifWe call the class of q-starlike functions of Type 1 associated with the Janowski functions. Definition 8. A function is said to belong to the class if and only if We call the class of q-starlike functions of Type 2 associated with the Janowski functions.
Definition 9. A function is said to belong to the class if and only if We call the class of q-starlike functions of Type 3 associated with the Janowski functions.
Each of the following special cases of the above-defined
q-starlike functions:
is worthy of note.
If we put
in Definition 7, we get the class
, which was introduced and studied by Wongsaijai and Sukantamala (see [
17], Definition 1).
If we put
in Definition 8, we are led to the class
, which was introduced and studied by Wongsaijai and Sukantamala (see [
17], Definition 2).
If we put
in Definition 9, we have the class
, which was introduced and studied by Wongsaijai and Sukantamala (see [
17], Definition 3).
If we put
in Definition 8, we obtain the class
, which was introduced and studied by Agrawal and Sahoo [
23].
If we put
in Definition 8, we get the class
introduced and studied by Ismail et al. [
9].
In Definition 8, if we let
and put
and
, then we will arrive at the function class, studied by Ponnusamy and Singh (see [
24]).
Geometrically, for
the quotient:
lies in the domains
given by
and
respectively.
In this paper, many properties and characteristics, for example sufficient conditions, inclusion results, distortion theorems, and radius problems, are discussed. We also indicate relevant connections of our results with a number of other related works on this subject.
3. Main Results and Their Demonstration
We first derive the inclusion results for the following generalized
q-starlike functions:
which are associated with the Janowski functions.
Theorem 1. If then Proof. First of all, we suppose that
Then, by Definition 9, we have
so that
By using the triangle inequality and Equation (10), we find that
The last expression in (11) now implies that
that is, that
Next, we let
so that
by Definition 8.
This last equation now shows that
that is, that
which completes the proof of Theorem 1. □
As a special case of Theorem 1, if we put
we get the following known result due to Wongsaijai and Sukantamala (see [
17]).
Corollary 1. (See [
17])
For Next, we present a remarkable simple characterization of functions in the class of q-starlike functions of Type 2 associated with the Janowski functions.
Theorem 2. Let . Then if and only ifwhere Proof. The proof of Theorem 2 can be easily obtained from the fact that
and Definition 8 of the class
of
q-starlike functions of Type 2 associated with the Janowski functions.□
Upon setting
in Theorem 2, we get the following known result.
Corollary 2. (See [
23])
Let . Then, if and only if Our next result is directly obtained by using Theorem 1 and a known result given in [
23].
Theorem 3. The classesof the generalized q-starlike functions of Type 1, Type 2, and Type 3, respectively, satisfy the following properties:and Finally, by means of a coefficient inequality, we give a sufficient condition for the class of generalized q-starlike functions of Type 3, which also provides a corresponding sufficient condition for the classes and of Type 1 and Type 2, respectively.
Theorem 4. A function and of the form (
1)
is in the class if it satisfies the following coefficient inequality: 4. Analytic Functions with Negative Coefficients
In this section, we introduce new subclasses of
q-starlike functions associated with the Janowski functions, which involve negative coefficients. Let
be a subset of
consisting of functions with a negative coefficient, that is,
Theorem 5. If then Proof. In view of Theorem 1, it is sufficient here to show that
Indeed, if we assume that
then we have
so that
After a simple calculation, we thus find that
that is, that
which can be written as follows:
The last expression in (15) implies that
which satisfies (12). By Theorem 4, the proof of Theorem 5 is completed.□
In its special case, when
Theorem 5 reduces to the following known result.
Corollary 3. (See [
17], Theorem 8)
If then The assertions of Theorem 5 imply that the Type 1, Type 2, and Type 3 generalized q-starlike functions associated with the Janowski functions are exactly the same. For convenience, therefore, we state the following distortion theorem by using the notation in which it is tacitly assumed that
Theorem 6. If thenwhere Proof. We note that the following inequality follows from Theorem 4:
which yields
We have thus completed the proof of Theorem 6.□
In its special case, when
if we let
, Theorem 6 reduces to the following known result.
Corollary 4. (See [
25])
If then The following result (Theorem 7) can be proven by using arguments similar to those that were already presented in the proof of Theorem 6, so we choose to omit the details of our proof of Theorem 7.
Theorem 7. If thenwhere is given by (16). In its special case, when
if we let
, Theorem 6 reduces to the following known result.
Corollary 5. (See [
25])
If then Remark 1. By using Theorem 4, it is easy to see that the function:whereandbutatThat is, and also . Therefore, it is interesting to study the radius of univalency and starlikeness of class Theorem 8. Let Then, f is univalent and starlike in , whereand satisfies the following inequality: Proof. To prove Theorem 8, it is sufficient to show that
In light of Theorem 4, the inequality in (19) will be true if
Solving the inequality in (20) for
we have
Next, we need to find
satisfying (18). Let
be the function defined by
Differentiating on both sides of (22) logarithmically, we have
It is easy to see that the second term of (
23) is positive. Since
and
then the third and the last term in (
23) can be dominated by
when
x is sufficiently large. This implies that
f is an increasing function on
where
Therefore, the radius of univalence can be defined by
In view of (24), the proof of our Theorem is now completed.□
If, in Theorem 8, we let
we are led to the following known result:
Corollary 6. [
17]
Let Then, f is univalent and starlike in , whereand satisfies the following inequality: Now, below, we give an example that validates Theorem 8.
Example 1. Consider the class with . By Theorem 8, we obtain the radius of univalency of class given by Now, we consider the sharpness example function
defined in (17) with
and
that is,
Obviously, is locally univalent on because at outside the open disk By applying Theorem 8, function is univalent on .
The next Theorem (Theorem 9) can be derived by working in a similar way as in Theorem 8; here, we omit the proof.
Theorem 9. Let Then f is starlike of order α in , whereand satisfies the following inequality: