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Generalized Lommel–Wright function and its geometric properties
Journal of Inequalities and Applications volume 2022, Article number: 115 (2022)
Abstract
The normalization of the combination of generalized Lommel–Wright function \(\mathfrak{J}_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}(z)\) (, \(\kappa _{3}>0\) and ) defined by \(\mathfrak{J}_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}(z):=\Gamma ^{m}( \kappa _{1}+1)\Gamma (\kappa _{1}+\kappa _{2}+1)2^{2\kappa _{1}+ \kappa _{2}}z^{1-(\kappa _{2}/2)-\kappa _{1}}\mathcal{J}_{\kappa _{1},\kappa _{2}}^{ \kappa _{3},m}(\sqrt{z})\), where \(\mathcal{J}_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}(z):=(1-2\kappa _{1}-\kappa _{2})J_{\kappa _{1},\kappa _{2}}^{ \kappa _{3},m}(z)+z ( J_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}(z) ) ^{\prime}\) and
was previously introduced and some of its geometric properties have been considered. In this paper, we report conditions for \(\mathfrak{J}_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}(z)\) to be starlike and convex of order α, \(0\leq \alpha <1\), inside the open unit disk using some technical manipulations of the gamma and digamma functions, as well as inequality for the digamma function that has been proved (Guo and Qi in Proc. Am. Math. Soc. 141(3):1007–1015, 2013). In addition, a method presented by Lorch (J. Approx. Theory 40(2):115–120 1984) and further developed by Laforgia (Math. Compet. 42(166):597–600 1984) is applied to establish firstly sharp inequalities for the shifted factorial that will be used to obtain the order of starlikeness and convexity. We compare then the obtained orders of starlikeness and convexity with some important consequences in the literature as well as the results proposed by all techniques to demonstrate the accuracy of our approach. Ultimately, a lemma by (Fejér in Acta Litt. Sci. 8:89–115 1936) is used to prove that the modified form of the function \(\mathfrak{J}_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}(z)\) defined by \(\mathcal{I}_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}(z)=\mathfrak{J}_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}(z)\ast z/(1+z) \ \) is in the class of starlike and convex functions, respectively. Further work regarding the function \(\mathfrak{J}_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}(z)\ \) is underway and will be presented in a forthcoming paper.
1 Introduction and preliminaries
In the literature, there has been a growing interest in special functions that have applications in different fields of mathematical analysis, functional analysis, geometry, and physics. Special functions are an old subject, but due to their essential position in mathematics, they continue to play an essential role, for instance, in combinatorics, applied mathematics, and engineering. More recently, further progress has been made towards the geometric properties for the normalized form of some special functions such as univalence, starlikeness, convexity, and close to convexity inside the open unit disk. Regarding treatises on this investigation, we refer, e.g., to [7–9, 12, 13] for generalized Bessel function, to [3] for hyper-Bessel functions, to [25, 32, 34] for generalized Struve function, to [31] for Lommel function, to [24, 28, 29] for hypergeometric function, to [33] for generalized Lommel–Wright function, and [23] for Fox–Wright function. In addition, the radii of starlikeness and the convexity of Bessel and its q-analog, Struve and Lommel functions, were investigated by several authors (see [1, 2, 4–6, 10–12]). These results would be fruitful to enrich the understanding of the geometrical properties of such functions as tools in such applications of geometric function theory.
Over the past few years considerable attention has been given to the role played by generalized Lommel–Wright function in concrete problems in physics, mechanics, engineering, and astronomy. In continuation of [33], we report conditions for \(\mathfrak{J}_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}(z)\) to be starlike and convex of order α, \(0\leq \alpha <1\), inside the open unit disk using some technical manipulations of the gamma and digamma functions as well as an inequality for the digamma function that has been proved [18]. In addition, a method presented by Lorch [22], and further developed by Laforgia [21], is applied to establish firstly sharp inequalities for the shifted factorial that will be used to obtain the order starlikeness and convexity. We compare then the obtained orders of starlikeness and convexity with some important consequences in the literature as well as the results proposed by all techniques to demonstrate the accuracy of our approach. Ultimately, a lemma by [16] is used to prove that the modified form of the function \(\mathfrak{J}_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}(z)\) defined by \(\mathcal{I}_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}(z)=\mathfrak{J}_{\kappa _{1},\kappa _{2}}^{\lambda _{3},m}(z)\ast z/(1+z)\) is in the class of starlike and convex functions, respectively.
Throughout this paper, let \(\mathcal{H}\) indicate the family of all functions that are analytic in . Denote by \(\mathcal{A}\) the subfamily of \(\mathcal{H}\) consisting of functions of the form
and by \(\mathcal{S}\) the subfamily of \(\mathcal{A}\) which are univalent in . If \(g\in \mathcal{A}\) is given by
then the convolution of the functions f and g is given by
The above definition of convolution arises from the formula (see [15])
Let us recall now the subclasses of the class of analytic functions which are considered the cornerstone of the univalent function theory such as the subclasses of starlike and convex functions. These classes admit geometrical and analytical characteristics, which do not pass in the status of those functions that are utilized in the ordinary analysis. The interested reader is referred for further information to [15, 17, 27], whereas general aspects are found in [19]. Traditionally, a domain is called starlike with respect to an interior point \(z_{0}\) if the line segment joining \(z_{0}\) to any other point in D lies entirely in D. In particular, if \(z_{0}=0\), then the domain D is called starlike domain. A function \(f(z)\in \mathcal{S}\) is called starlike with respect to the origin (or starlike), denoted by \(\mathcal{S}^{\ast}\), if is a starlike domain. The well-known analytical characterization of starlikeness is given by the following theorem.
Theorem A
Let \(f\in \mathcal{S}\). Then f is starlike if and only if
Further, if the line segment joining any two points of lies entirely in D, then the domain is convex. A function \(f(z)\in \mathcal{S}\) is called convex, denoted by \(\mathcal{K}\), if is a convex domain. The following theorem gives an analytic description of the convex functions.
Theorem B
Let \(f\in \mathcal{S}\). Then f is convex if and only if
For instance, \(f(z)=z/(1-z)^{2}\in \mathcal{S}^{\ast}\) because of
while \(f(z)=-\log (1-z)\in \mathcal{K}\) since
It is noteworthy to mention that the classes \(\mathcal{S}^{\ast}\) and \(\mathcal{K }\) have a particular interest if more restrictions are enjoined, it gives us various types of classes of functions. Moreover, thanks to the positivity of \(\operatorname{Re} ( zf^{\prime}(z)/f(z) ) \) and \(1+ \operatorname{Re} ( zf^{\prime \prime}(z)/f^{\prime}(z) ) \) for \(\mathcal{S}^{\ast}\) and \(\mathcal{K}\), respectively, it allows us to study several families of conformal transformation with other motivating geometric properties. On the other hand, \(f\in \mathcal{A }\) is starlike functions of order α, \(0\leq \alpha \leq 1\), if and only if
and is in the class of convex functions of order α, denoted by \(\mathcal{K}(\alpha )\), if and only if
It is well-known that \(\mathcal{S}^{\ast}(\alpha )\subset \mathcal{S}^{\ast }(0)=\mathcal{S}^{\ast}\), \(\mathcal{K}(\alpha ) \subset \mathcal{K}(0)=\mathcal{K }\), and \(\mathcal{K}\subset \mathcal{S}^{\ast}\subset \mathcal{S}\).
In [14], Oteiza et al. defined the generalized Lommel–Wright function \(J_{\lambda _{2},\kappa _{1}}^{\kappa _{3},m}(z)\) as
for , , and \(\kappa _{3}>0\). Noting that \(_{p} \Psi _{q}\) stands the Fox–Wright function which is defined by
with
for (\(i=1,\dots ,p\), \(j=1,\dots ,q\)) and . It is worthy to note that (1.4) converges absolutely in the entire complex z-plane when \(\Delta :=\sum_{j=1}^{q}\mathrm{B}_{j}-\sum_{i=1}^{p} \mathrm{A}_{i}>-1\), while if \(\Delta =-1\), it is absolutely convergent for \(\vert z \vert <\rho \) and \(\vert z \vert =\rho \) under the restriction \(\operatorname{Re}(\sigma )>1/2\), where
For more details concerning the Fox–Wright functions, we refer to [20] and the references therein.
We processed to insert some special cases of the generalized Lommel–Wright function. The Bessel–Maitland function introduced by Pathak [26] as
is obtained by taking \(m=1\) in (1.3) for \(\kappa _{3}>0\) and . Putting \(\kappa _{1}=1/2\) and \(m=\kappa _{3}=1\) in (1.3), we obtain the Struve function defined by
For \(\kappa _{1}=0\) and \(m=\kappa _{3}=1\) in (1.3), we have the Bessel function defined by
where \(z\neq 0\), , and \(\operatorname{Re}\kappa _{2}>-1\).
We shall need the following definition.
Definition 1
The normalization of the combination of generalized Lommel–Wright function is defined by
where \(\mathcal{J}_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}(z):=(1-2 \kappa _{1}-\kappa _{2})J_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}(z)+z ( J_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}(z) ) ^{ \prime}\) with , , and . Clearly, \(\mathfrak{J}_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}(z)\) can be written as
where \((\lambda )_{n}\) stands for the Pochhammer symbol given by
The next technical lemmas will be helpful to obtain the main results.
Lemma 1
([18])
For \(x\in (0,\infty )\) and , the following inequalities hold:
Lemma 2
([16])
Suppose that is a sequence of nonnegative real numbers such that \(A_{1}=1\). If \(nA_{n}-(n+1)A_{n+1}\geq 0 \) and \(nA_{n}-2(n+1)A_{n+1}+(n+2)A_{n+2} \geq 0\) for all . Then \(f(z)=\sum_{n=1}^{\infty}A_{n}z^{n}\) is starlike in .
Lemma 3
Suppose that \(a>0\), \(\kappa _{3}\geq 1\), \(4\kappa _{3}^{2}\geq ( \kappa _{3}-1 ) a\) and \(\gamma \geq \max \{\gamma _{1},\gamma _{2}\}\), where \(\gamma _{1}\) is the greatest root of the quadratic equation
whilst \(\gamma _{2}\) is the greatest root of the equation
then the following inequality
holds for all \(n\geq 3\).
Proof
We have to start by defining the functions \(f(a)\) and \(g(a)\) as follows:
and
Therefore,
Consider the function defined by
We proceed to establish for which values of a, γ, and \(\kappa _{3}\), the function \(\chi (n)\) is increasing on \([3,\infty )\). This means that \(\chi (n)\geq \chi (3)\) for all \(n \geq 3\). On the other hand, if \(\chi (3)\geq 0\), this implies to \(\chi (n)\geq 0\), which leads to \(a\mapsto g(a)\) is increasing for \(n\geq 3\), \(\kappa _{3}\geq 1\), and \(\gamma \geq \max \{\gamma _{1}, \gamma _{2}\}\). Now,
The last expression is positive if
It is worth mentioning that \(\chi (3)\geq 0\) if
which holds if
where \(\gamma _{2}\geq 0\) if
which implies that
If \(\kappa _{3}\geq 1\), then the term between the brackets is positive if \(4\kappa _{3}^{2}\geq ( \kappa _{3}-1 ) a\). In addition, by making use of the asymptotic expansion of the ratio of gamma function \(\Gamma (z+\alpha )/\Gamma (z+\beta )\), that is,
we obtain
for \(a>0\), \(\kappa _{3}\geq 1\), \(4\kappa _{3}\geq ( \kappa _{3}-1 ) a\), and \(\gamma \geq \max \{\gamma _{1},\gamma _{2}\}\), where \(\gamma _{1}\) and \(\gamma _{2}\) are given above and \(\lim_{a\rightarrow \infty}g(a)=1\). Bearing in mind that the function g is increasing for all \(a>0\), \(\kappa _{3}\geq 1\), \(4 \kappa _{3}\geq ( \kappa _{3}-1 ) a\), and \(\gamma \geq \max \{\gamma _{1},\gamma _{2}\}\), then \(g(a)\leq 1\). Moreover, \(f(a+1)\leq f(a)\), which leads to \((a)_{n\kappa _{3}}\geq a(a+\gamma )^{ ( n-1 ) \kappa _{3}} \) for all \(a>0\), \(\kappa _{3}\geq 1\), and \(\gamma \geq \max \{\gamma _{1}, \gamma _{2}\}\). This completes the proof. □
2 Main results
Our first two theorems of this section contain some interesting and applicable results involving the order of starlikeness and the order of convexity inside using some technical manipulations of the gamma and digamma functions which improve slightly the results given in [33].
Theorem 1
Let \(\kappa _{1},\kappa _{2}\geq 0\) such that \(\kappa _{1}+\kappa _{2}\geq \frac{1}{2}\). Also, assume that and
then \(\mathfrak{J}_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}(z)\in \mathcal{S}^{\ast}(\alpha )\).
Proof
To prove that \(\mathfrak{J}_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}(z)\in \mathcal{S}^{\ast}(\alpha )\) for all , it is sufficient to show that
for . Using the maximum modulus theorem of an analytic function as well as the well-known inequality \(\vert z_{1}+z_{2} \vert \leq \vert z_{1} \vert + \vert z_{2} \vert \), we get
for and . Using the fact that the gamma function satisfies \(\Gamma (z+1)=z\Gamma (z)\), we get
and so
Now,
Suppose that
Differentiating (2.3) logarithmically with respect to n, we find
here, ψ stands for the digamma function defined by
By using the fact that the digamma function is increasing on \((0,\infty )\) and \(\psi (z)\geq 0\) for all \(z\geq x^{\ast}\), where \(x^{\ast}\simeq 1.461632144\ldots\) is the abscissa of the minimum of the gamma function, and with the help of (2.4), we deduce that the sequence \(\{ \mathrm{F}(n) \} _{n\geq 1}\) is decreasing. Then we get
On the other hand,
for and . Putting everything together, we see that
and then we conclude that \(\mathfrak{J}_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}(z)\in \mathcal{S}^{\ast}(\alpha )\). □
Theorem 2
Suppose that \(\kappa _{1}\geq 0\), \(\kappa _{2}\geq 0, \kappa _{3}\), , and
then \(\mathfrak{J}_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}(z)\in \mathcal{K}(\alpha )\).
Proof
To prove that \(\mathfrak{J}_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}(z)\in \mathcal{K}(\alpha )\) for all , it is sufficient to show that
for . As in Theorem 1, we shall base the proof on the maximum modulus theorem of an analytic function to get
for . Using the increasing property of the digamma functions, it is easy to observe that
is a strictly decreasing function of n. Thus, we get
Further computations yield
Combining everything together to get
and from the above inequality, we conclude that \(\mathfrak{J}_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}(z)\in \mathcal{K}(\alpha )\). □
Remark 1
It is worth noting that special cases will follow if we set \(\kappa _{1}=0\), \(\kappa _{3}=m=1\), and \(\kappa _{1}=1/2\), \(\kappa _{3}=m=1\), respectively, in Theorems 1 and 2.
In the following results, that is, Theorems 3 and 4, the starlikeness and convexity with its order have been evaluated where the leading concept of the proofs comes from Lemma 1.
Theorem 3
Assume that \(\kappa _{1}\), \(\kappa _{2}\), \(\kappa _{3}\) are positive numbers, such that
and
then \(\mathfrak{J}_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}(z)\in \mathcal{S}^{\ast}(\alpha )\).
Proof
From Theorem 1, we have
for . Letting
Hence,
and
From Lemma 1, we have
under the given hypotheses, which leads to \(\mathrm{D}_{2}(x)\) is a strictly decreasing function on \([1,\infty )\) with \(\mathrm{D}_{2}(1)<0\) to conclude that \(\mathrm{D}_{2}(x)<0\) for all \(x\geq 1\). Consequently, \(\mathrm{D}_{1}^{\prime}(x)<0\) under the given hypotheses, that is, \(\mathrm{D}_{1}(x)\) is a strictly decreasing function on \([1,\infty )\) and
Similarly, we can show that
for , which ultimates our proof. □
Using arguments similar to Theorem 3, we get the following result regarding the order of convexity by using (1.6) and (1.7).
Theorem 4
Assume that \(\kappa _{1}\), \(\kappa _{2}\), \(\kappa _{3}\) are positive numbers, such that
and
then \(\mathfrak{J}_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}(z)\in \mathcal{K}(\alpha )\).
In the next two theorems, we are going with other results including the order of starlikeness and the order of convexity that are evaluated using the sharp inequalities for the shifted factorial, which improve slightly the results given in [33].
Theorem 5
Suppose that
where
and
with \(\kappa _{1}>-1\), \(\kappa _{2}\geq 0\), \(\kappa _{3}\geq 1\), \(\gamma \geq \max \{\gamma _{1},\gamma _{2}\}\), where \(\gamma _{1}\) and \(\gamma _{2}\) are given in Lemma 3and \(\mathrm{R}_{2}>0\), then \(\mathfrak{J}_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}\in \mathcal{S}^{\ast }(\alpha )\).
Proof
To begin with, we note that if \(f\in \mathcal{A }\) satisfies \(\sum_{n=2}^{\infty} ( n-\alpha ) \vert A_{n} \vert \leq 1-\alpha \), then \(f\in \mathcal{S}^{\ast} ( \alpha ) \) (see [30, Theorem 1]). Therefore, according to (1.5), it is sufficient to show that
Since \(\kappa _{1}>-1\), \(\kappa _{2}\geq 0\), and \(\kappa _{3}\geq 1\), we have
Using the fact that
which can be verified using the concept of mathematical induction and
for all \(\kappa _{1}>-1\), \(\kappa _{2}\geq 0\), \(\kappa _{3}\geq 1\), and \(\gamma \geq \max \{\gamma _{1},\gamma _{2}\}\) that follows from Lemma 3, we obtain
Thus, we conclude that \(\mathfrak{J}_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}\in \mathcal{S}^{\ast}(\alpha )\), as required. □
Theorem 6
Suppose that
where
and
with \(\kappa _{1}>-1\), \(\kappa _{2}\geq 0\), \(\kappa _{3}\geq 1\), \(\gamma \geq \max \{\gamma _{1},\gamma _{2}\}\), where \(\gamma _{1}\) and \(\gamma _{2}\) are given in Lemma 3and \(\mathrm{T}_{2}>0\), then \(\mathfrak{J}_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}\in \mathcal{K}(\alpha )\).
Proof
Using the Alexander duality relation and according to [30, Corollary on p. 110], it suffices to show that
Since \(\kappa _{1}>-1\), \(\kappa _{2}\geq 0\), and \(\kappa _{3}\geq 1\), we have
Recalling the fact that
and Lemma 3, it follows that
This proves the claim that \(\mathfrak{J}_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}\in \mathcal{K}(\alpha )\). □
Remark 2
1. Theorem 1, Theorem 3, and Theorem 5 assign sufficient conditions for starlikeness of \(\mathfrak{J}_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}\). As it appears in Table 1, the first one gives better result than the second and the third ones for suitable choices of the parameters.
2. Due to Theorem 2, Theorem 4, and Theorem 6, which assign sufficient conditions for convexity of \(\mathfrak{J}_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}\), it is important to observe as that Theorem 2 sometimes gives a better estimation than the others, while occasionally Theorem 4 is the best. See Table 2.
In the remainder of this section, we shall use Lemma 2 to prove \(\mathcal{I}_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}(z)= \mathfrak{J}_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}(z)\ast z/(1+z)\) is in the class of starlike and convex functions, respectively.
Theorem 7
If \(\kappa _{1}\geq (\sqrt{13}-3)/2\simeq 0.302776\ldots\) and , then \(\mathfrak{J}_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}(z) \ast z/(1+z)\) is starlike in .
Proof
From (1.5) and bearing in mind that \(z/(1+z)\) can be expressed as
we have
where
Thanks to Lemma 2, we shall prove that \(nA_{n}\geq (n+1)A_{n+1}\) and \(nA_{n}-2(n+1)A_{n+1}+(n+2)A_{n+2}\geq 0\) for all where \(A_{1}=1\), \(A_{n}>0\) for all \(n\geq 2\). Bearing in mind that
for \(\kappa _{1}\geq (\sqrt{13}-3)/2\) and , it is easy to observe that
that is,
where
Since \(\kappa _{1}\geq (\sqrt{13}-3)/2\) and , we have
It is worth mentioning that \((n+1)A_{n+1}\leq nA_{n}\) if \(\widetilde {\mathrm{U}}(n)\geq 0\) for all . Noting that
which holds for \(\kappa _{1}\geq (\sqrt{13}-3)/2\) and , it follows that
Furthermore, since \(\kappa _{1}\geq (\sqrt{13}-3)/2\) and , we have
and so
Continuing in this manner we get
It remains to show that \(nA_{n}+(n+2)A_{n+2}\geq 2(n+1)A_{n+1}\) for all . Since \(A_{n+2}>0\) for all , we easily get
Using (2.11), we have
and so,
where
Since \(\kappa _{1}\geq (\sqrt{13}-3)/2\) and , we have
Again, since \(\kappa _{1}\geq (\sqrt{13}-3)/2\) and , we have
which ends the proof. □
Theorem 8
Suppose that \(\kappa _{1}\geq 0\) and . Then \(\mathfrak{J}_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}(z)\ast z/(1+z)\) is starlike in .
Proof
Under the hypotheses \(\kappa _{1}\geq 0\) and , Lemma 2 and Theorem 7, we proceed to showing that \((n+1)A_{n+1}\leq nA_{n}\) and \(nA_{n}+(n+2)A_{n+2} \geq 2(n+1)A_{n+1}\) for all . At first, for \(n=1\), \(\mathrm{U}(1)=4(\kappa _{1}+1)^{m}(\kappa _{1}+\kappa _{2}+1)-6\geq 4( \kappa _{1}+1)(\kappa _{1}+2)-6>0\) for \(\kappa _{1}\geq 0 \), whilst for \(n\geq 2\), we find
Further, it can be shown that
is a decreasing function with respect to n as follows:
Since \(\kappa _{1}\geq 0\) and , we get \(\psi (\kappa _{1}+n)\geq 0\) and \(\psi (\kappa _{1}+\kappa _{2}+1+(n-1)\kappa _{3} )\geq 0\), these together with (2.12) lead to \(nA_{n}\geq (n+1)A_{n+1}\), \(n\geq 2\). A similar argument may be used to prove that \(nA_{n}+(n+2)A_{n+2}\geq 2(n+1)A_{n+1}\). For \(n=1,2\), it is easy to prove \(nA_{n}+(n+2)A_{n+2}\geq 2(n+1)A_{n+1}\), whereas for \(n\geq 3\), we have
and since \(\mathrm{V}(n)\) is a decreasing function with respect to \(n, n\geq 3\), this would lead to \(nA_{n}+(n+2)A_{n+2}\geq 2(n+1)A_{n+1}\) for , which asserts our claim. □
Remark 3
It is important to note that Theorem 8 extends the range of validity for parameter \(\kappa _{1}\) to \(\kappa _{1}\geq 0\).
Theorem 9
If , then, \(\mathfrak{J}_{\kappa _{1},\kappa _{2}}^{ \kappa _{3},m}(z)\ast z/(1+z)\) is convex in .
Proof
Using the classical Alexander theorem between the classes of starlike and convex functions, which asserts that \(f(z)\in \mathcal{K }\) if and only if \(zf^{\prime}(z)\in \mathcal{S}^{\ast}\), it is sufficient to prove that \(z(\mathfrak{J}_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}(z))^{\prime} \ast z/(1+z)\) is starlike in . We then have
where
To obtain the required result, we will use Lemma 2. It suffices to show that
We shall show that \((n+1)B_{n+1}\leq nB_{n}\) for all as follows:
where
Since , we have
Obviously, \(nB_{n}\geq (n+1)B_{n+1}\) if \(\widetilde{\mathrm{W}}(n)\geq 0\) for all . Bearing in mind that , it follows that
On the other hand, we prove that \(nB_{n}+(n+2)B_{n+2}\geq 2(n+1)B_{n+1}\) for all . We have
where
For , we find
which completes the proof. We can propose another proof for the same result as outlined below. For \(n=1\), \(\mathrm{W}(1)=4(\kappa _{1}+1)^{m}(\kappa _{1}+\kappa _{2}+1)-12 \geq 4(\kappa _{1}+1)(\kappa _{1}+2)-12>0\) for \(\kappa _{1}\geq 1\), whilst for \(n\geq 2\), we find
and since \(\mathrm{W}(n)\) is a decreasing function with respect to \(n, n\geq 2\), we get \(nB_{n}-(n+1)B_{n+1}\geq 0\), . Secondly, it is easy to prove that \(nB_{n}+(n+2)B_{n+2}\geq 2(n+1)B_{n+1}\) for \(n=1,2\), whereas for \(n\geq 3\), we have
and since \(\mathrm{Y}(n)\) is a decreasing function with respect to \(n, n\geq 3\), it follows that \(nB_{n}+(n+2)B_{n+2}\geq 2(n+1)B_{n+1}\) for , and according to Lemma 2, we end the proof of the theorem. □
3 Conclusions
In the current paper, we have reported conditions for \(\mathfrak{J}_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}(z)\) to be starlike and convex of order α, \(0\leq \alpha <1\), inside the open unit disk using some technical manipulations of the gamma and digamma functions as well as an inequality for the digamma function that has been proved in [18]. In addition, a method presented by Lorch [22] and further developed by Laforgia [21] has been applied to establish firstly sharp inequalities for the shifted factorial that would be used to obtain the order starlikeness and convexity. We then have compared the obtained orders of starlikeness and convexity with some important consequences in the literature as well as the results proposed by all techniques to demonstrate the accuracy of our approach. We conclude the paper showing that the modified form of the function \(\mathfrak{J}_{\kappa _{1},\kappa _{2}}^{\kappa _{3},m}(z)\) is in the class of starlike and convex functions. Further investigations on this topic are now underway and will be reported in forthcoming papers.
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HMZ has a major contributor to writing the main manuscript text and analyzing the results, reviewing, and editing. KH contributed to analyzing all the results and making necessary improvements. Both authors read and approved the final manuscript.
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Zayed, H.M., Mehrez, K. Generalized Lommel–Wright function and its geometric properties. J Inequal Appl 2022, 115 (2022). https://doi.org/10.1186/s13660-022-02851-8
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DOI: https://doi.org/10.1186/s13660-022-02851-8
MSC
- 30C45
- 33C50
Keywords
- Analytic
- Univalent
- Starlike
- Convex
- Generalized Lommel–Wright functions