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Article

Classes of Multivalent Spirallike Functions Associated with Symmetric Regions

by
Luminiţa-Ioana Cotîrlǎ
1,*,† and
Kadhavoor R. Karthikeyan
2,†
1
Department of Mathematics, Technical University of Cluj-Napoca, 400114 Cluj-Napoca, Romania
2
Department of Applied Mathematics and Science, National University of Science & Technology, Muscat P.O. Box 620, Oman
*
Author to whom correspondence should be addressed.
These authors contributed equally to this work.
Symmetry 2022, 14(8), 1598; https://doi.org/10.3390/sym14081598
Submission received: 22 June 2022 / Revised: 26 July 2022 / Accepted: 1 August 2022 / Published: 3 August 2022
(This article belongs to the Special Issue Symmetry in Quantum Calculus)

Abstract

:
We define a function to unify the well-known class of Janowski functions with a class of spirallike functions of reciprocal order. We focus on the impact of defined function on various conic regions which are symmetric with respect to the real axis. Further, we have defined a new subclass of multivalent functions of complex order subordinate to the extended Janowski function. This work bridges the studies of various subclasses of spirallike functions and extends well-known results. Interesting properties have been obtained for the defined function class. Several consequences of our main results have been pointed out.

1. Introduction and Definitions

Let N , R , and C represent the respective sets of natural numbers, real numbers, and complex numbers. For p N , we let N p denote the class of functions ϕ of the form
ϕ ( z ) = z p + n = p + 1 a n z n
which are analytic in the open unit disc E = { z : z C and | z | < 1 } . We let C and S * denote the well-known subclass of N 1 which are convex and starlike in E . Additionally, let P consist of functions χ which are analytic and is given by
χ ( z ) = 1 + n = 1 R n z n , z E , R 1 > 0
and satisfies Re χ ( z ) > 0 , z E . For π / 2 < σ < π / 2 , a function ϕ N p is said to be σ -spiral in E if
R e e i σ z ϕ ( z ) ϕ ( z ) > 0 , ( z E ) .
Similarly, a function ϕ N p is said to be convex σ -spiral in E if
R e e i σ 1 + z ϕ ( z ) ϕ ( z ) > 0 , ( z E ) .
We denote σ -spiral functions and convex σ -spiral functions, respectively, by SL p ( σ ) and CS p ( σ ) .
The reciprocal class of σ -spiral functions was defined by Uyanik et al. in [1], by replacing > 0 in the right hand side of the inequality (3) by < λ , ( λ > p cos σ ) . We denote the reciprocal class by RS p ( σ , λ ) . Similar generalization was used to define reciprocal convex σ -spiral, by replacing > 0 in the right hand side of the inequality (4) by < λ , ( λ > p cos σ ) and is denoted by RC p ( σ , λ ) . Further, it was established in [1] that the function ϕ ( z ) R S p ( σ , λ ) if and only if
e i σ z ϕ ( z ) ϕ ( z ) 2 λ p e i σ + 2 p cos σ λ 1 z , ( z E ) ,
where π 2 < σ < π 2 and λ > p cos σ . Here ≺ denotes the usual subordination of analytic function. Similarly, ϕ N p is said to be in RC p ( σ , λ ) if and only if it satisfies the condition
e i σ 1 + z ϕ ( z ) ϕ ( z ) 2 λ p e i σ + 2 p cos σ λ 1 z , ( z E ) .

Purpose, Motivation and Novelty

The main purpose of this paper is to define a function Δ σ λ ( z ) (see (7)) so as to unify the superordinate function in (5) with the well-known class of Janowski functions. Our study would consolidate or unify the study of various subclasses related to spirallike and reciprocal spirallike functions.
Aouf [2] ([Equation 1.4]) defined the class P ( U , V , p , λ ) which consists of functions h ( z ) = p + n = 1 p n z n analytic in the unit disc such that h ( z ) P ( U , V , p , λ ) if and only if
h ( z ) = p + p V + ( U V ) ( p λ ) w ( z ) 1 + V w ( z ) , ( 1 V < U 1 , 0 λ < 1 )
where w ( z ) is the Schwartz function. The class P ( U , V , p , λ ) is an extension of the famous Janowski class of functions [3]. Motivated by the class recently studied by Breaz et al. [4] and in view of generalizing the superordinate function in (5), we now define and study the following relation
Δ σ λ ( z ) = ( 1 + U e 2 i σ ) p e i σ + λ ( V U ) χ ( z ) + ( 1 U e 2 i σ ) p e i σ λ ( V U ) ( V + 1 ) χ ( z ) + ( 1 V ) ,
where 1 V < U 1 , π 2 < σ < π 2 , λ > p cos σ and χ ( z ) P .
To study the impact of Δ σ λ ( z ) on various conic regions, we consider the following:
  • χ ( z ) = 1 1 z which maps unit disc onto the half plane Re ( w ) > 0.5
  • χ ( z ) = z 2 + 2 z + 2 which maps the unit disc onto interior of the cardioid region with cusp on the left hand side
For an admissible choice of the parameter U = 0.5 , V = 0.5 , p = 1 , σ = π 3 and λ = 0.6 , if the function
  • χ ( z ) = 1 1 z , then Δ σ λ ( z ) maps the unit disc on to the interior of the circular domain (See Figure 1a).
  • χ ( z ) = z 2 + 2 z + 2 , then Δ σ λ ( z ) maps unit disc onto a cardioid region which is magnified and the cusp of the cardioid gets rotated on to the right hand side (see Figure 1b).
Hence, the type of impact of Δ σ λ ( z ) on various regions is not the same.
Remark 1.
Now we will list some recent studies, which are special cases of Δ σ λ ( z ) .
1
If we let σ = 0 in (7), then Δ σ λ ( z ) reduces to
( z ) = ( 1 + U ) p + λ ( V U ) χ ( z ) + ( 1 U ) p λ ( V U ) ( V + 1 ) χ ( z ) + ( 1 V ) .
The function ( z ) was defined and studied by Breaz et al. in [4].
2
If we let U = 1 , V = 1 and χ ( z ) = ( 1 + z ) / ( 1 z ) in (7), then Δ σ λ ( z ) reduces to 2 λ p e i σ + 2 p cos σ λ 1 z (see the superordinate function in (5)).
For the function ϕ N p given by (1) and h N p of the form h ( z ) = z p + n = p + 1 Γ n z n , the Hadamard product (or convolution) of these two function is defined by
Ω ( z ) : = ( ϕ h ) ( z ) : = z p + n = p + 1 a n Γ n z n , z E .
Unless otherwise mentioned
1 V < U 1 , | σ | < π 2 , λ > p cos σ .
Definition 1.
For π 2 < σ < π 2 , 0 η 1 , λ p cos σ , b C { 0 } and Ω = ϕ h defined as in (8), we say that the function ϕ belongs to the class LS σ ( λ , η ; b ; χ ; h ; U , V ) if it satisfies the subordination condition
e i σ p + 1 b η z 2 Ω ( z ) + [ p ( 1 η ) + η ] z Ω ( z ) p ( 1 η ) Ω ( z ) + η z Ω ( z ) p Δ σ λ ( z ) ,
where “≺” denotes subordination and Δ σ λ ( z ) is defined as in (7).
Remark 2.
Recall that RS p ( σ , λ ) were defined as a generalization of the class RS 1 ( 0 , λ ) introduced by Uralegaddi [5]. Further, the class RS p ( σ , λ ) was extended and studied by various authors (see [1,6,7,8,9,10]). Very recently, Altınkaya in [11] introduced and studied a new subclass of spirallike functions closely related to the defined function class LS σ ( λ , η ; b ; χ ; h ; U , V ) . We note that all the above mentioned studies can be obtained as special cases of our class LS σ ( λ , η ; b ; χ ; h ; U , V ) . The details of the special cases will be pointed out when we derive applications of our main results.

2. Preliminaries

Here, we prepare the groundwork that is required to obtain our main results. Firstly, we begin with the discussion of obtaining the Maclaurin series for the function Δ σ λ ( z ) . From (7), we see that
Δ σ λ ( z ) = λ ( V U ) ( 1 U e 2 i σ ) p e i σ ( V 1 ) 1 ( 1 + U e 2 i σ ) p e i σ + λ ( V U ) χ ( z ) λ ( V U ) ( 1 U e 2 i σ ) p e i σ × 1 ( V + 1 ) χ ( z ) V 1 1 = λ ( V U ) ( 1 U e 2 i σ ) p e i σ ( V 1 ) + λ ( V U ) ( 1 U e 2 i σ ) p e i σ ( V + 1 ) ( V 1 ) 2 ( 1 + U e 2 i σ ) p e i σ + λ ( V U ) ( V 1 ) χ ( z ) + λ ( V U ) ( 1 U e 2 i σ ) p e i σ ( V + 1 ) 2 ( V 1 ) 3 ( 1 + U e 2 i σ ) p e i σ + λ ( V U ) ( V + 1 ) ( V 1 ) 2 χ ( z ) 2 + = 2 p e i σ V 1 1 + V + 1 V 1 + V + 1 V 1 2 + + 2 U ( p e i σ λ ) V ( p e i σ λ ) R 1 ( V 1 ) 2 1 + 2 V + 1 V 1 + 3 V + 1 V 1 2 + z + = 2 p e i σ V 1 1 V + 1 V 1 1 + 2 U ( p e i σ λ ) V ( p e i σ λ ) R 1 ( V 1 ) 2 1 V + 1 V 1 2 z +
Hence, (7) can be rewritten as
Δ σ λ ( z ) = p e i σ + U ( p e i σ λ ) V ( p e i σ λ ) R 1 2 z +
Remark 3.
In [12], Karthikeyan et al. have showed that convex function becomes starlike by varying the parameters in Δ 0 λ ( z ) . Hence, the function Δ σ λ ( z ) may be convex univalent or starlike univalent depending on the function χ ( z ) . It cannot be concluded that impact of Δ σ λ ( z ) on a convex region does not affect the convexity. However, if Δ σ λ ( z ) is to be convex univalent, it is always possible to find a function χ such that Δ σ λ ( z ) is convex univalent in E . For example, if we choose χ ( z ) = 1 + z then Δ σ λ ( z ) is convex univalent in E for all admissible values of the parameters involved. It is well-known that 1 + z is convex univalent in E (see Lemma 2.5 [13]), the function Δ σ λ ( z ) does not alter the conic 1 + z except for translation, magnification, and rotation. That is, it does not affect the convexity or univalence as we vary the parameters involved (see Figure 2a–d).
We need the following result to obtain the coefficient inequality.
Lemma 1
([14], Theorem VII). Let χ ( z ) = n = 1 a n z n be analytic in E and g ( z ) = n = 1 b n z n be analytic and convex in E . If χ ( z ) g ( z ) , then a n b 1 for n = 1 , 2 , .
We will use the following results to obtain the solution of the Fekete–Szegő problem for the functions that belong to the classes we defined in the first section.
Lemma 2.
([15], page 41). If ϑ ( z ) = 1 + n = 1 ϑ n z n P , then | ϑ n | 2 for all n 1 , and the inequality is sharp for ϑ μ ( z ) = 1 + μ z 1 μ z , | μ | 1 .
Lemma 3.
([16]). If ϑ ( z ) = 1 + n = 1 ϑ n z n P , and v is complex number, then
ϑ 2 v ϑ 1 2 2 max 1 ; | 2 v 1 | ,
and the result is sharp for the functions
ϑ 1 ( z ) = 1 + z 1 z and ϑ 2 ( z ) = 1 + z 2 1 z 2 .

3. Main Results

3.1. Integral Representation of LS σ ( λ , η ; b ; χ ; h ; U , V )

For ϕ LS σ ( λ , η ; b ; χ ; h ; U , V ) , we have by the definition of subordination
η z Ω ( z ) + [ p ( 1 η ) + η ] Ω ( z ) p ( 1 η ) Ω ( z ) + η z Ω ( z ) p z = b e i σ Δ σ λ [ w ( z ) ] p z ,
where w is analytic in E with w ( 0 ) = 0 and | w ( z ) | < 1 . Integrating (11), we have (integrating z 0 to z with z 0 0 and then let z 0 0 )
log ( 1 η ) Ω ( z ) + ( η / p ) z Ω ( z ) z p = 0 z b e i σ Δ σ λ [ w ( t ) ] p t d t .
Equivalently (12) can be rewritten as
( 1 η ) Ω ( z ) + ( η / p ) z Ω ( z ) = z p exp 0 z b e i σ Δ σ λ [ w ( t ) ] p t d t .
We have two cases, namely
  • For η = 0 , trivially we have
    Ω ( z ) = z p exp 0 z b e i σ Δ σ λ [ w ( t ) ] p t d t .
  • For 0 < η 1 ,
    Ω ( z ) = p η z p 1 1 η 0 z u p η 1 exp 0 u b e i σ Δ σ λ [ w ( t ) ] p t d t d u .
Summarizing the above discussion, we have
Theorem 1.
If ϕ LS σ η ( λ , η ; b ; χ ; h ; U , V ) , then
(i) 
for 0 < η 1 ,
Ω ( z ) = p η z p 1 1 η 0 z u p η 1 exp 0 u b e i σ Δ σ λ [ w ( t ) ] p t d t d u .
(ii) 
for η = 0 ,
Ω ( z ) = z p exp 0 z b e i σ Δ σ λ [ w ( t ) ] p t d t .
Corollary 1.
If ϕ RS p ( σ , λ ) , then
ϕ ( z ) = z p exp ( 2 λ p cos σ ) e i σ 0 z [ w ( t ) ] t ( 1 w ( t ) ) d t .
Similarly, if ϕ RC p ( σ , λ ) , then
ϕ ( z ) = p 0 z u p 1 exp ( 2 λ p cos σ ) e i σ 0 u [ w ( t ) ] t ( 1 w ( t ) ) d t d u .
Proof. 
Setting U = 1 , V = 1 , h ( z ) = z p + n = p + 1 z n and χ ( z ) = ( 1 + z ) / ( 1 z ) in (13), we get
( 1 η ) ϕ ( z ) + ( η / p ) z ϕ ( z ) = z p exp ( 2 λ p cos σ ) e i σ 0 z [ w ( t ) ] t ( 1 w ( t ) ) d t .
We get (16) if we let η = 0 in (18). If we let η = 1 in (18) and then integrate the resulting equation, we obtain (17). □
Remark 4.
Note that Uyanik et al. [1] did not obtain the integral representation for the classes RS p ( σ , λ ) and RC p ( σ , λ ) . However, Shi et al. in [17] (Theorem 1 & Corollary 1) obtained the integral representation for the meromorphic analogue of RS p ( σ , λ ) and RC p ( σ , λ ) .

3.2. Coefficient Inequalities and Solution to The Fekete–Szegő Problem

We need the following result to obtain the coefficient estimate for functions in the class LS σ ( λ , η ; b ; χ ; h ; U , V ) .
Lemma 4.
Let Δ σ λ ( z ) be convex univalent in E . If r ( z ) = p e i σ + n = 1 r n z n is analytic in E and satisfies
r ( z ) ( 1 + U e 2 i σ ) p e i σ + λ ( V U ) χ ( z ) + ( 1 U e 2 i σ ) p e i σ λ ( V U ) ( V + 1 ) χ ( z ) + ( 1 V ) ,
then
r n U ( p e i σ λ ) V ( p e i σ λ ) R 1 2 , n 1 .
Proof. 
Note that from Remark 3, it is possible to find a function χ so that Δ σ λ ( z ) is convex univalent in E . From (10), we have
Δ σ λ ( z ) = p e i σ + U ( p e i σ λ ) V ( p e i σ λ ) R 1 2 z + , z E .
The assumption (19) is equivalent to
r ( z ) p e i σ Δ σ λ ( z ) p e i σ .
Additionally, because the convexity of Δ σ λ ( z ) implies the convexity of Δ σ λ ( z ) p e i σ , from Lemma 1 it follows the conclusion (20). □
Theorem 2.
Let ϕ LS σ ( λ , η ; b ; χ ; h ; U , V ) and χ be chosen so that Δ σ λ ( z ) is convex univalent in E . If 1 V < 0 , then, for k = 1 , 2 , 3 ,
a p + k p p + k η Γ p + k j = 0 k 1 b U ( p e i σ λ ) V ( p e i σ λ ) R 1 + 2 j 2 ( j + 1 ) .
Proof. 
Consider
η z 2 Ω ( z ) + [ p ( 1 η ) + η ] z Ω ( z ) = p + b e i σ r ( z ) p p ( 1 η ) Ω ( z ) + η z Ω ( z )
where r ( z ) = p e i σ + n = 1 r n z n is analytic in E and satisfies the subordination condition r ( z ) Δ σ λ ( z ) . Equivalently, (22) can be rewritten as
p 2 z p + n = p + 1 n p ( 1 η ) + n η a n Γ n z n = p + n = 1 b r n e i σ z n p z p + n = p + 1 p ( 1 η ) + n η a n Γ n z n .
On equating the coefficient of z p + k , we get
( p + k ) p + η k a p + k Γ p + k = p p + η k Γ p + k a p + k + b e i σ i = 0 k 1 p ( 1 η ) + ( p + i ) η r k i Γ p + i a p + i ,
where a p = 1 , Γ p = 1 . On computation, we have
a p + k | b | k ( p + η k ) | Γ p + k | × i = 0 k 1 r n i p ( 1 η ) + ( p + i ) η Γ p + i a p + i
Using (20) in the above inequality, we have
a p + k | b | | R 1 | U ( p e i σ λ ) V ( p e i σ λ ) 2 k ( p + η k ) | Γ p + k | i = 0 k 1 p ( 1 η ) + ( p + i ) η Γ p + i a p + i .
Taking k = 1 in (23), we get
a p + 1 p | b | | R 1 | U ( p e i σ λ ) V ( p e i σ λ ) 2 ( p + η ) | Γ p + 1 |
The hypothesis is true for k = 1 . Now let k = 2 in (23), we get
a p + 2 | b | | R 1 | U ( p e i σ λ ) V ( p e i σ λ ) 4 ( p + 2 η ) | Γ p + 2 | p + | Γ p + 1 | { p + η | a p + 1 | } p | b | | R 1 | U ( p e i σ λ ) V ( p e i σ λ ) 4 ( p + 2 η ) | Γ p + 2 | 1 + | b | | R 1 | U ( p e i σ λ ) V ( p e i σ λ ) 2 .
If we let k = 2 in (21), we have
a p + 2 p p + 2 η Γ p + k [ b U ( p e i σ λ ) V ( p e i σ λ ) R 1 2 × b U ( p e i σ λ ) V ( p e i σ λ ) R 1 + 2 4 ] p | b | | R 1 | U ( p e i σ λ ) V ( p e i σ λ ) 4 ( p + 2 η ) | Γ p + 2 | 1 + | b | | R 1 | U ( p e i σ λ ) V ( p e i σ λ ) 2 .
Therefore hypothesis of the theorem is true for k = 2 . Now let us suppose (21) is valid for k = 2 , 3 , m , we get
a p + m p p + m η Γ p + m j = 0 m 1 b U ( p e i σ λ ) V ( p e i σ λ ) R 1 + 2 j 2 ( j + 1 ) .
By induction hypothesis, we have
| b | | R 1 | U ( p e i σ λ ) V ( p e i σ λ ) 2 m p i = 0 m 1 p ( 1 η ) + ( p + i ) η Γ p + i a p + i j = 0 m 1 b U ( p e i σ λ ) V ( p e i σ λ ) R 1 + 2 j 2 ( j + 1 ) .
From the above inequality, we have
j = 0 m b U ( p e i σ λ ) V ( p e i σ λ ) R 1 + 2 j 2 ( j + 1 ) | b | | R 1 | U ( p e i σ λ ) V ( p e i σ λ ) 2 p m b U ( p e i σ λ ) V ( p e i σ λ ) R 1 + 2 m 2 ( m + 1 ) i = 0 m 1 p ( 1 η ) + ( p + i ) η Γ p + i a p + i | b | | R 1 | U ( p e i σ λ ) V ( p e i σ λ ) 2 p ( m + 1 ) [ p ( 1 η ) + ( p + m ) η Γ p + m a p + m + i = 0 m 1 p ( 1 η ) + ( p + i ) η Γ p + i a p + i ] = | b | | R 1 | U ( p e i σ λ ) V ( p e i σ λ ) 2 p ( m + 1 ) i = 0 m p ( 1 η ) + ( p + i ) η Γ p + i a p + i ,
implies that inequality is true for k = m + 1 . Hence the assertion of the Theorem. □
If we let χ ( z ) = 1 + n = 1 2 z n , U = 1 , V = 1 , b = 1 , η = 0 and Γ n = 1 ( n p + 1 ) in Theorem 2, we get
Corollary 2.
([1] ([Theorem 2])). If ϕ RS p ( σ , λ ) , then
a p + k 1 k ! j = 0 k 1 2 ( λ p cos σ ) + j , ( k = 1 , 2 , 3 , ) .
Letting χ ( z ) = 1 + n = 1 2 z n , U = 1 , V = 1 , b = 1 , η = 1 and Γ n = 1 ( n p + 1 ) in Theorem 2, we get
Corollary 3.
If ϕ RC p ( σ , λ ) , then
a p + k p ( p + k ) k ! j = 0 k 1 2 ( λ p cos σ ) + j , ( k = 1 , 2 , 3 , ) .
Theorem 3.
If ϕ ( z ) = z p + a p + 1 z p + 1 + a p + 2 z p + 2 + LS σ ( λ , η ; b ; χ ; h ; U , V ) , then we have for all μ C we have
a p + 2 μ a p + 1 2 p U ( p e i σ λ ) V ( p e i σ λ ) b R 1 4 ( p + 2 η ) Γ p + 2 max 1 , | 2 Q 1 1 | ,
where Q 1 is given by
Q 1 = 1 4 ( V + 1 ) R 1 + 2 1 R 2 R 1 p e i σ b U ( p e i σ λ ) V ( p e i σ λ ) R 1 ( p + η ) Γ p + 1 + 2 μ p e i σ b R 1 U ( p e i σ λ ) V ( p e i σ λ ) ( p + 2 η ) Γ p + 2 ( p + η ) 2 Γ p + 1 2 .
The inequality is sharp for each μ C .
Proof. 
As ϕ LS σ ( λ , η ; b ; χ ; h ; U , V ) , by (9) we have
p + 1 b η z 2 Ω ( z ) + [ p ( 1 η ) + η ] z Ω ( z ) p ( 1 η ) Ω ( z ) + η z Ω ( z ) p = e i σ Δ σ λ [ w ( z ) ] .
Thus, let ϑ P be of the form ϑ ( z ) = 1 + k = 1 ϑ n z n and defined by
ϑ ( z ) = 1 + w ( z ) 1 w ( z ) , z E .
On computation, we have
w ( z ) = 1 2 ϑ 1 z + 1 2 ϑ 2 1 2 ϑ 1 2 z 2 + 1 2 ϑ 3 ϑ 1 ϑ 2 + 1 4 ϑ 1 3 z 3 + , z E .
The right hand side of (24)
p + b e i σ Δ σ λ [ w ( z ) ] p = p + b e i σ U ( p e i σ λ ) V ( p e i σ λ ) R 1 2 1 2 ϑ 1 z + 1 2 ϑ 2 1 2 ϑ 1 2 z 2 + + b e i σ U ( p e i σ λ ) V ( p e i σ λ ) 2 R 2 R 1 2 2 ( V + 1 ) 2 1 2 ϑ 1 z + 1 2 ϑ 2 1 2 ϑ 1 2 z 2 + 2 + = p + b e i σ R 1 ϑ 1 U ( p e i σ λ ) V ( p e i σ λ ) 4 z + b e i σ U ( p e i σ λ ) V ( p e i σ λ ) R 1 4 ϑ 2 ϑ 1 2 ( V + 1 ) R 1 + 2 1 R 2 R 1 4 z 2 + .
The left hand side of (24) is given by
η z 2 Ω ( z ) + [ p ( 1 η ) + η ] z Ω ( z ) p ( 1 η ) Ω ( z ) + η z Ω ( z ) = p + ( p + η ) p Γ p + 1 a p + 1 z + 2 ( p + 2 η ) p Γ p + 2 a p + 2 ( p + η ) p Γ p + 1 a p + 1 2 z 2 + .
From (25) and (26), we obtain
a p + 1 = p e i σ b R 1 ϑ 1 U ( p e i σ λ ) V ( p e i σ λ ) 4 ( p + η ) Γ p + 1
and
a p + 2 = p e i σ b U ( p e i σ λ ) V ( p e i σ λ ) R 1 8 ( p + 2 η ) Γ p + 2 [ ϑ 2 1 4 ( V + 1 ) R 1 + 2 1 R 2 R 1 p e i σ b U ( p e i σ λ ) V ( p e i σ λ ) R 1 ( p + η ) Γ p + 1 ϑ 1 2 ] .
To prove the Fekete–Szegő inequality for the class LS σ ( λ , η ; b ; χ ; h ; U , V ) , we consider
a p + 2 μ a p + 1 2 = | p e i σ b U ( p e i σ λ ) V ( p e i σ λ ) R 1 8 ( p + 2 η ) Γ p + 2 [ ϑ 2 1 4 ( V + 1 ) R 1 + 2 1 R 2 R 1 p e i σ b U ( p e i σ λ ) V ( p e i σ λ ) R 1 ( p + η ) Γ p + 1 ϑ 1 2 ] μ p 2 e 2 i σ b 2 R 1 2 ϑ 1 2 U ( p e i σ λ ) V ( p e i σ λ ) 2 16 ( p + η ) 2 Γ p + 1 2 |
= | p e i σ b U ( p e i σ λ ) V ( p e i σ λ ) R 1 8 ( p + 2 η ) Γ p + 2 [ ϑ 2 ϑ 1 2 4 ( V + 1 ) R 1 + 2 1 R 2 R 1 p e i σ b U ( p e i σ λ ) V ( p e i σ λ ) R 1 ( p + η ) Γ p + 1 + 2 μ p e i σ b R 1 U ( p e i σ λ ) V ( p e i σ λ ) ( p + 2 η ) Γ p + 2 ( p + η ) 2 Γ p + 1 2 |
p b U ( p e i σ λ ) V ( p e i σ λ ) R 1 8 ( p + 2 η ) Γ p + 2 2 + | ϑ 1 | 2 4 2 R 2 R 1 ( V + 1 ) R 1 2 1 R 2 R 1 p e i σ b U ( p e i σ λ ) V ( p e i σ λ ) R 1 ( p + η ) Γ p + 1 2 μ p e i σ b R 1 U ( p e i σ λ ) V ( p e i σ λ ) ( p + 2 η ) Γ p + 2 ( p + η ) 2 Γ p + 1 2 } | 2 .
Denoting
H : = | 2 R 2 R 1 ( V + 1 ) R 1 p e i σ b U ( p e i σ λ ) V ( p e i σ λ ) R 1 ( p + η ) Γ p + 1 2 μ p e i σ b R 1 U ( p e i σ λ ) V ( p e i σ λ ) ( p + 2 η ) Γ p + 2 ( p + η ) 2 Γ p + 1 2 } | ,
if H 2 , from (29) we obtain
a p + 2 μ a p + 1 2 p b U ( p e i σ λ ) V ( p e i σ λ ) R 1 4 ( p + 2 η ) Γ p + 2 .
Further, if H 2 from (29) we deduce
a p + 2 μ a p + 1 2 p b U ( p e i σ λ ) V ( p e i σ λ ) R 1 4 ( p + 2 η ) Γ p + 2 ( | 2 R 2 R 1 ( V + 1 ) R 1 p e i σ b U ( p e i σ λ ) V ( p e i σ λ ) R 1 ( p + η ) Γ p + 1 2 μ p e i σ b R 1 U ( p e i σ λ ) V ( p e i σ λ ) ( p + 2 η ) Γ p + 2 ( p + η ) 2 Γ p + 1 2 } | ) .
The equality for (30) will be attained if ϑ 1 = 0 , ϑ 2 = 2 . Equivalently, by Lemma 3 we have ϑ ( z 2 ) = ϑ 2 ( z ) = 1 + z 2 1 z 2 . Therefore, the extremal function of the class LS σ ( λ , η ; b ; χ ; h ; U , V ) is given by
p + 1 b η z 2 Ω ( z ) + [ p ( 1 η ) + η ] z Ω ( z ) p ( 1 η ) Ω ( z ) + η z Ω ( z ) p = e i σ ( 1 + U ) p + σ ( V U ) ϑ ( z 2 ) + ( 1 U ) p σ ( V U ) ( V + 1 ) ϑ ( z 2 ) + ( 1 V ) .
Similarly, the equality for (30) holds if ϑ 2 = 2 . Equivalently, by Lemma 3 we have ϑ ( z ) = ϑ 1 ( z ) = 1 + z 1 z . Therefore, the extremal function in LS σ ( λ , η ; b ; χ ; h ; U , V ) is given by
p + 1 b η z 2 Ω ( z ) + [ p ( 1 η ) + η ] z Ω ( z ) p ( 1 η ) Ω ( z ) + η z Ω ( z ) p = e i σ ( 1 + U ) p + σ ( V U ) ϑ 1 ( z ) + ( 1 U ) p σ ( V U ) ( V + 1 ) ϑ 1 ( z ) + ( 1 V ) ,
and the proof of the theorem is complete. □
Corollary 4.
If ϕ ( z ) = z + a 2 z 2 + a 3 z 3 + S * ( ψ ) and ψ ( z ) = 1 + R 1 z + R 2 z 2 + , with R 1 , R 2 R , R 1 > 0 , then for all μ C we have
a 3 μ a 2 2 R 1 2 max 1 ; R 1 + R 2 R 1 2 μ R 1 .
The inequality is sharp for the function ϕ * given by
ϕ * ( z ) = z exp 0 z ψ ( t ) 1 t d t , i f | R 1 + R 2 R 1 2 μ R 1 | 1 , z exp 0 z ψ ( t 2 ) 1 t d t , i f | R 1 + R 2 R 1 2 μ R 1 | 1 .
Proof. 
In Theorem 3, taking U = 1 , V = 1 , Γ n = p = b = 1 and σ = η = 0 we get the inequality
a 3 μ a 2 2 R 1 2 , if | R 1 + R 2 R 1 2 μ R 1 | 1 , R 1 2 R 1 + R 2 R 1 2 μ R 1 , if | R 1 + R 2 R 1 2 μ R 1 | 1 .

4. Properties of Q-Spirallike Functions

Keeping with the recent trend of research, in this section we will define a class replacing the classical derivative with a quantum derivative in LS σ ( λ , η ; b ; χ ; h ; U , V ) .
We begin with a brief introduction on quantum calculus. For ϕ N p given by (1) and 0 < q < 1 , the Jackson’s q-derivative operator or q-difference operator for a function ϕ N p is defined by (see [18,19])
T q ϕ ( z ) : = ϕ ( 0 ) , if z = 0 , ϕ ( z ) ϕ ( q z ) ( 1 q ) z , if z 0 .
From (33), if ϕ has the power series expansion (1) we can easily see that T q ϕ ( z ) = p z p 1 + n = p + 1 [ n ] q a n z n 1 , for z 0 , where [ n ] q is defined by
[ n ] q : = 1 q n 1 q ,
and note that lim q 1 T q ϕ ( z ) = ϕ ( z ) . Throughout this paper, we let denote
( [ n ] q ) k : = [ n ] q [ n + 1 ] q [ n + 2 ] q [ n + k 1 ] q .
The q-Jackson integral is defined by (see [20])
I q ϕ ( z ) : = 0 z ϕ ( t ) d q t = z ( 1 q ) n = 0 q n ϕ ( z q n )
provided the q-series converges. Srivastava et al. [21,22,23,24,25,26,27,28] introduced several function classes using quantum derivative and also studied its impact involving conic regions. Let T q 2 ϕ ( z ) = T T q ϕ ( z ) denote the second order q-difference.
Definition 2.
For π 2 < σ < π 2 , 0 η 1 , λ p cos σ , b C { 0 } and Ω = ϕ h defined as in (8), we say that the function ϕ belongs to the class QS σ ( λ , η ; b ; χ ; h ; U , V ) if it satisfies the subordination condition
e i σ [ p ] q + 1 b η q z 2 T q 2 Ω ( z ) + ( [ p ] q ( 1 η ) + η ) z T q Ω ( z ) [ p ] q ( 1 η ) Ω ( z ) + η z T q Ω ( z ) [ p ] q Υ q ( σ , λ ; z ) ,
where Υ q ( σ , λ ; z ) is the q -analogue of Δ σ λ ( z ) , which is defined by
Υ q ( σ , λ ; z ) = ( 1 + U e 2 i σ ) [ p ] q e i σ + λ ( V U ) χ ( z ) + ( 1 U e 2 i σ ) [ p ] q e i σ λ ( V U ) ( V + 1 ) χ ( z ) + ( 1 V ) .
Remark 5.
We note that everything in classical calculus cannot be generalized to quantum calculus, notably the chain rule needs adaptation. Hence, logarithmic differentiation needs some application of analysis. In [29], Agrawal and Sahoo obtained the following result on logarithmic differentiation. For ϕ N 1 and 0 < q < 1 , we have
I q T q ϕ ( z ) ϕ ( z ) = q 1 ln q log ϕ ( z ) ,
where I q ϕ is the Jackson q-integral, defined as in (34).

Integral Representation, Coefficient Estimates and Fekete-Szegö Inequalities of QS σ ( λ , η ; b ; χ ; h ; U , V )

Analogous to the result obtained in Theorem 1, we now present the integral representation for functions f belonging to the family QS σ ( λ , η ; b ; χ ; h ; U , V ) .
Theorem 4.
Let ϕ QS σ ( λ , η ; b ; χ ; h ; U , V ) and e i σ Δ σ λ ( z ) is convex in E with Re b e i σ Δ σ λ [ w ( z ) ] [ p ] q > 0 , then
Ω ( z ) = z p exp ln q q 1 0 z b e i σ Δ σ λ [ w ( t ) ] [ p ] q t d q t , i f   η = 0 0 z u p 1 exp ln q q 1 0 u b e i σ Δ σ λ [ w ( t ) ] p t d q t d q u , i f   η = 1 .
Proof. 
Suppose that M η p ( z ) = [ p ] q ( 1 η ) Ω ( z ) + η z T q Ω ( z ) , then the condition (35) can be rewritten as
T q M η p ( z ) M η p ( z ) [ p ] q z = b e i σ Δ σ λ [ w ( z ) ] [ p ] q z .
Integrating the above expression (see (37)), we have
q 1 ln q log M η p ( z ) z p = 0 z b e i σ Δ σ λ [ w ( t ) ] [ p ] q t d q t .
or equivalently,
[ p ] q ( 1 η ) Ω ( z ) + η z T q Ω ( z ) = z p exp ln q q 1 0 z b e i σ Δ σ λ [ w ( t ) ] [ p ] q t d q t .
Thus, if ϕ QS σ η ( λ , η ; b ; ψ ; h ; U , V ) , then we have
Ω ( z ) = z p exp ln q q 1 0 z b e i σ Δ σ λ [ w ( t ) ] [ p ] q t d q t , ( if   η = 0 ) ,
and
Ω ( z ) = 0 z u p 1 exp ln q q 1 0 u b e i σ Δ σ λ [ w ( t ) ] [ p ] q t d q t d q u , ( if   η = 1 ) .
Hence the proof of the Theorem. □
Theorem 5.
Let ϕ QS σ ( λ , η ; b ; χ ; h ; U , V ) and χ be chosen so that Υ q ( σ , λ ; z ) is convex univalent in E . If 1 V < 0 , then, for k = 1 , 2 , 3 ,
a p + k [ p ] q [ p ] q ( 1 η ) + [ p + k ] q η Γ p + k j = 0 k 1 b U ( [ p ] q e i σ λ ) V ( [ p ] q e i σ λ ) R 1 + 2 q p [ j ] q 2 q p [ j + 1 ] q .
Proof. 
Consider
η q z 2 T q 2 Ω ( z ) + [ p ( 1 η ) + η ] z T q Ω ( z ) = p + b e i σ r ( z ) p p ( 1 η ) Ω ( z ) + η z T q Ω ( z )
where r ( z ) = p e i σ + n = 1 r n z n is analytic in E and satisfies the subordination condition r ( z ) Δ σ λ ( z ) . Using the equality q [ p 1 ] q = [ p ] q 1 , we can rewrite (40) as
[ p ] q 2 z p + n = p + 1 [ n ] q [ p ] q ( 1 η ) + [ n ] q η a n Γ n z n = [ p ] q + n = 1 b r n e i σ z n [ p ] q z p + n = p + 1 [ p ] q ( 1 η ) + [ n ] q η a n Γ n z n .
On equating the coefficient of z p + k , we get
[ p + k ] q [ p ] q ( 1 η ) + [ p + k ] q η a p + k Γ p + k = [ p ] q [ p ] q ( 1 η ) + [ p + k ] q η Γ p + k a p + k + b e i σ i = 0 k 1 [ p ] q ( 1 η ) + [ p + i ] q η r k i Γ p + i a p + i ,
where a p = 1 , Γ p = 1 . On computation, we have
| a p + k | | b | [ p ] q ( 1 η ) + [ p + k ] q η [ p + k ] q [ p ] q | Γ p + k | × i = 0 k 1 r n i [ p ] q ( 1 η ) + [ p + i ] q η | Γ p + i | | a p + i |
Using (20) in the above inequality, we have
a p + n | b | | R 1 | U ( [ p ] q e i σ λ ) V ( [ p ] q e i σ λ ) 2 [ p ] q ( 1 η ) + [ p + k ] q η [ p + k ] q [ p ] q | Γ p + k | i = 0 k 1 [ p ] q ( 1 η ) + [ p + i ] q η Γ p + i | a p + i | .
Using the equality [ p + k ] q [ p ] q = q p [ k ] q and following the steps as Theorem 2, we can establish the assertion of the Theorem. □
For completeness, we just state the following result.
Theorem 6.
If ϕ ( z ) = z p + a p + 1 z p + 1 + a p + 2 z p + 2 + QS σ ( λ , η ; b ; χ ; h ; U , V ) , then we have for all μ C we have
a p + 2 μ a p + 1 2 [ p ] q U ( [ p ] q e i σ λ ) V ( [ p ] q e i σ λ ) b R 1 4 ( [ p ] q + 2 η ) Γ p + 2 max 1 , | 2 Q 2 1 | ,
where Q 2 is given by
Q 2 = 1 4 ( V + 1 ) R 1 + 2 1 R 2 R 1 [ p ] q e i σ b U ( [ p ] q e i σ λ ) V ( [ p ] q e i σ λ ) R 1 ( [ p ] q + η ) Γ p + 1 + 2 μ [ p ] q e i σ b R 1 U ( [ p ] q e i σ λ ) V ( [ p ] q e i σ λ ) ( [ p ] q + 2 η ) Γ p + 2 ( [ p ] q + η ) 2 Γ p + 1 2 .
The inequality is sharp for each μ C .

5. Conclusions

We have defined a new family of multivalent spirallike functions of reciprocal order, which was entirely motivated by Uyanik et al. [1]. Integral representation and solutions to the Fekete–Szegö problem are the main results of this paper. We also point out relevant connections which we investigate here, with those in several related earlier works on this subject.
This study can be extended by replacing χ ( z ) in Δ σ λ ( z ) with special functions such as exponential function, Legendre polynomial, q-Hermite polynomial, Chebyshev polynomial, or Fibonacci sequence. Additionally, notice that in definition of LS σ ( λ , η ; b ; χ ; h ; U , V ) we have used convolution of two functions which opens the door to many real life applications. Further, if h ( z ) in (8) is replaced with generalized Mittag–Leffler function, we enter the fascinating world of fractional differential equations.

Author Contributions

Conceptualization, L.-I.C. and K.R.K.; methodology, L.-I.C. and K.R.K.; software, L.-I.C. and K.R.K.; validation, L.-I.C. and K.R.K.; formal analysis, L.-I.C. and K.R.K.; investigation, L.-I.C. and K.R.K.; resources, L.-I.C. and K.R.K.; data curation, L.-I.C. and K.R.K.; writing—original draft preparation, L.-I.C. and K.R.K.; writing—review and editing, L.-I.C. and K.R.K.; visualization, L.-I.C. and K.R.K.; supervision, L.-I.C. and K.R.K.; project administration, L.-I.C. and K.R.K. All authors have read and agreed to the published version of the manuscript.

Funding

This research study received no external funding.

Institutional Review Board Statement

Not applicable.

Informed Consent Statement

Not applicable.

Data Availability Statement

Not applicable.

Acknowledgments

The authors would like to thank all the reviewers for their helpful comments and suggestions, which helped us remove the mistakes and also led to improvement in the presentation of the results.

Conflicts of Interest

Both the authors declare that they have no conflict of interest.

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Figure 1. Impact of Δ σ λ ( z ) on the conic region χ ( z ) if U = 0.5 , V = 0.5 , p = 1 , σ = π 3 and λ = 0.6 (a) The image of the unit disc under the mapping of Δ σ λ ( z ) , if χ ( z ) = 1 / 1 z . (b) The image of the unit disc under the mapping of Δ σ λ ( z ) , if χ ( z ) = z 2 + 2 z + 2 .
Figure 1. Impact of Δ σ λ ( z ) on the conic region χ ( z ) if U = 0.5 , V = 0.5 , p = 1 , σ = π 3 and λ = 0.6 (a) The image of the unit disc under the mapping of Δ σ λ ( z ) , if χ ( z ) = 1 / 1 z . (b) The image of the unit disc under the mapping of Δ σ λ ( z ) , if χ ( z ) = z 2 + 2 z + 2 .
Symmetry 14 01598 g001
Figure 2. Impact of Δ σ λ ( z ) on the conic region χ ( z ) = 1 + z . (a) if U = 0.5 , V = 0.5 , p = 1 , σ = π 3 and λ = 0.6 ; (b) if U = 1 , V = 1 , p = 1 , σ = π 3 and λ = 0.6 ; (c) if U = 1 , V = 1 , p = 2 , σ = π 3 and λ = 0.6 ; (d) if U = 0 , V = 0.5 , p = 1 , σ = π 3 and λ = 0.6 .
Figure 2. Impact of Δ σ λ ( z ) on the conic region χ ( z ) = 1 + z . (a) if U = 0.5 , V = 0.5 , p = 1 , σ = π 3 and λ = 0.6 ; (b) if U = 1 , V = 1 , p = 1 , σ = π 3 and λ = 0.6 ; (c) if U = 1 , V = 1 , p = 2 , σ = π 3 and λ = 0.6 ; (d) if U = 0 , V = 0.5 , p = 1 , σ = π 3 and λ = 0.6 .
Symmetry 14 01598 g002
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Cotîrlǎ, L.-I.; Karthikeyan, K.R. Classes of Multivalent Spirallike Functions Associated with Symmetric Regions. Symmetry 2022, 14, 1598. https://doi.org/10.3390/sym14081598

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Cotîrlǎ L-I, Karthikeyan KR. Classes of Multivalent Spirallike Functions Associated with Symmetric Regions. Symmetry. 2022; 14(8):1598. https://doi.org/10.3390/sym14081598

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Cotîrlǎ, Luminiţa-Ioana, and Kadhavoor R. Karthikeyan. 2022. "Classes of Multivalent Spirallike Functions Associated with Symmetric Regions" Symmetry 14, no. 8: 1598. https://doi.org/10.3390/sym14081598

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Cotîrlǎ, L. -I., & Karthikeyan, K. R. (2022). Classes of Multivalent Spirallike Functions Associated with Symmetric Regions. Symmetry, 14(8), 1598. https://doi.org/10.3390/sym14081598

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