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: