Let us consider the following second-order linear homogeneous differential equation (see for details [1] and [2]):
(1.1)
The function , which is called the generalized Bessel function of the first kind of order u, it is defined as a particular solution of (1.1). The function has the familiar representation as
(1.2)
Here Γ stands for the Euler gamma function. The series (1.2) permits the study of Bessel, modified Bessel, and spherical Bessel function altogether. It is worth mentioning that, in particular:
-
(1)
For in (1.2), we obtain the familiar Bessel function of the first kind of order u defined by
(1.3)
-
(2)
For and in (1.2), we obtain the modified Bessel function of the first kind of order u defined by
(1.4)
-
(3)
For and in (1.2), the function reduces to where is the spherical Bessel function of the first kind of order u, defined by
(1.5)
In [3], the author considered the function defined, in terms of the generalized Bessel function . From (1.2), it is clear that . Therefore, it follows from (1.2)
(1.6)
Let us set
where
Hence, (1.6) becomes
(1.7)
By using the well-known Pochhammer symbol (or the shifted factorial) defined, for and in terms of the Euler Γ function, by
(1.8)
where it is being understood conventionally that . Therefore, we obtain the following series representation for the function given by (1.6):
(1.9)
where , and , and therefore
(1.10)
where and . The function is called the generalized and ‘normalized’ Bessel function of the first kind of order u. We note that by the ratio test, the radius of convergence of the series is infinity. Moreover, the function is analytic in ℂ and satisfies the differential equation . For convenience, we write . Let denote the class of functions of the form
(1.11)
which are analytic in the open unit disk . Let be the subclass of consisting of univalent functions in with the normalized condition . A function is said to be starlike of order η if it satisfies () for some η () and we denote the class of functions which are starlike of order η in as . Also, a function is said to be convex of order η if it satisfies () for some η () and we denote by the class of all convex functions of order η in . It follows by the Alexander relation that . The classes and were introduced by Robertson [4] (see also Srivastava and Owa [5]). Let and . Then f is said to be close to convex of order γ and type η if and only if () where and . The classes were introduced by Libera [6] (see also Noor and Al-Kharsani [7], Silverman [8] and Shanmugam and Ramachandran [9]). Furthermore, we denote by and (), two interesting subclasses of consisting, respectively, of functions which are k-uniformly convex and k-starlike in defined for by
and
The class was introduced by Kanas and Wiśniowska in [10], where its geometric definition and connections with the conic domains were considered. The class was investigated in [11]. In fact, it is related to the class by means of the well-known Alexander equivalence between the usual classes of convex and starlike functions (see also the work of Kanas and Srivastava [12] for further developments involving each of the classes and ). In particular, when , we obtain and , where and are the familiar classes of uniformly convex functions and parabolic starlike functions in , respectively. We remark here that the classes and are related to the domain bounded by conical sections. Motivated by works of Kanas and Wiśniowska [10] and [11], Al-Kharsani and Al-Hajiry [13] introduced the classes k-uniformly convex functions and k-starlike functions of order η () as below:
(1.12)
and
(1.13)
In the case when the inequalities (1.12) and (1.13) reduce to the well-known classes of starlike and convex functions of order η, respectively. Further, as mentioned earlier, for the special choices of and the class reduces to the class of uniformly convex functions introduced by Goodman [14] and the class reduces to the class of parabolic starlike functions studied extensively by Rønning [15] (see also the work of Ma and Minda [16]). If f and g are analytic in , then we say that the function f is subordinate to g, if there exists a Schwarz function , analytic in with and (), such that (). We denote this subordination by or (). In view of the earlier works studied by Kanas and Kanas et al. [10–12, 17–22], Sim et al. [23] and Al-Kharsani [24] defined the domain for as
Note that, for ,
for ,
The explicit form of the extremal function that maps onto the conic domain is given by
where , is the Legendre elliptic integral of the first kind
and is chosen such that . In view of the definition of subordination and the extremal function ,
(1.14)
and
(1.15)
Therefore,
(1.16)
Define as the family of functions such that
(1.17)
Similarly, we define as the family of functions such that
(1.18)
We note that is the class of close to convex univalent functions of order η and type β and is the class of quasi-convex univalent functions of order η and type β. For given by (1.11) and given by , the Hadamard product (or convolution) of and is given by
Note that . For () and (), the generalized hypergeometric function is defined by the following infinite series (see the work of [25] and [26] for details):
(; ). Dziok and Srivastava [27] (also see [28]) considered the linear operator
defined by the Hadamard product
(1.19)
(; , ). If is given by (1.11), then we have
Now, by using the above idea of Dziok and Srivastava [27], Deniz [2] introduced the -operator as follows:
(1.20)
It easy to verify from the definition (1.20) that
(1.21)
where . In fact, the function given by (1.20) is an elementary transformation of the generalized hypergeometric function. That is, it is easy to see that and also . In special cases of the -operator we obtain the following operators related to the Bessel function:
-
(1)
Choosing in (1.20) or (1.21), we obtain the operator related with Bessel function, defined by
(1.22)
and its recursive relation
-
(2)
Choosing and in (1.20) or (1.21), we obtain the operator related with the modified Bessel function, defined by
(1.23)
and its recursive relation
-
(3)
Choosing and in (1.20) or (1.21), we obtain the operator related with the spherical Bessel function, defined by
(1.24)
and its recursive relation
Finally we recall the generalized Bernardi-Libera-Livingston integral operator, which is defined by