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Article

Starlike Functions of the Miller–Ross-Type Poisson Distribution in the Janowski Domain

by
Gangadharan Murugusundaramoorthy
1,
Hatun Özlem Güney
2,* and
Daniel Breaz
3
1
Department of Mathematics, School of Advanced Sciences, Vellore Institute of Technology (VIT), Vellore 632014, India
2
Department of Mathematics, Faculty of Science, Dicle University, Diyarbakır 21280, Türkiye
3
Department of Exact Sciences and Engineering, Universitatea 1 Decembrie 1918 din Alba Iulia, 510009 Alba Iulia, Romania
*
Author to whom correspondence should be addressed.
Mathematics 2024, 12(6), 795; https://doi.org/10.3390/math12060795
Submission received: 6 February 2024 / Revised: 1 March 2024 / Accepted: 5 March 2024 / Published: 8 March 2024

Abstract

:
In this paper, considering the various important applications of Miller–Ross functions in the fields of applied sciences, we introduced a new class of analytic functions f , utilizing the concept of Miller–Ross functions in the region of the Janowski domain. Furthermore, we obtained initial coefficients of Taylor series expansion of f , coefficient inequalities for f 1 and the Fekete–Szegö problem. We also covered some key geometric properties for functions f in this newly formed class, such as the necessary and sufficient condition, convex combination, sequential subordination and partial sum findings.

1. Introduction

Let A 0 represent the collections of analytic functions f inside open unit disc D = z C : z < 1 with normalization f ( 0 ) = 0 = f ( 0 ) 1 and be of the form
f z = z + n = 2 a n z n , z D .
Furthermore, all functions that are univalent in D comprise the class denoted by S , a subclass of A 0 . If for every point in set B C the line segment joining origin to that point lies inside B , then that set is said to be starlike with respect to origin. Starlike functions are defined as functions f A 0 that map D to a starlike domain, and S * designates this class of functions. Analytically, a function f A 0 is called a starlike function if
Re z f z f ( z ) > 0 , ( z D ) .
If the line segment connecting any two points in set B ,   z 1 and z 2 , lies inside B , then the set B C is convex. A set B C is convex if the line segment joining any two points in set z 1 , z 2 B , falls inside convex domain B . Analytically, a function f A 0 is called a convex function if
Re ( z f ( z ) ) f ( z ) > 0 , ( z D ) .
The coefficients of functions f in a particular subclass of A 0 have been the subject of attention for numerous mathematicians since the early 1900s. De Branges solved the most important and inspirational problem, the Bieberbach hypothesis, seventy years after it was first put forth in 1984. Over time, many interesting subclasses have emerged with respect to these coefficients. The Fekete–Szegö inequalities introduced in 1933 (see [1]) and functional a 3 a 2 2 are also among the important findings for the coefficients of the functions f . The Fekete–Szegö problem is to maximize a 3 μ a 2 2 for a real as well as complex μ . Fekete and Szegö gave sharp estimates of a 3 μ a 2 2 for a real μ and f S , the class of univalent functions [2,3].
Miller and Ross [4] proposed the special function as the basis of the solution of fractional order initial value problem, which is called the Miller–Ross function, defined as
E ν , μ ( z ) = z ν e μ z Υ * ( ν , μ z ) , ν , μ , z C , with Re ν > 0 , Re μ > 0 ,
where Υ * is the incomplete gamma function (p. 314, [4]). Using the properties of the incomplete gamma functions, the Miller–Ross function can easily be written as
E ν , μ ( z ) : = z ν n = 0 ( μ z ) n Γ ( n + ν + 1 ) , ν , μ , z C , with Re ν > 0 , Re μ > 0 ,
which can be stated as
E ν , μ ( z ) z ν E 1 , 1 + ν ( μ z )
where in the right hand member, E 1 , 1 + ν ( μ z ) is the Mittag–Leffler function of two parameters [5]. Some of special values of the Miller–Ross functions can be given as follows:
E ν , μ ( 0 ) = 0 , Re ( ν ) > 0 , E 0 , μ ( z ) = e μ z , E 0 , 1 ( z ) = e z .
Recently, Eker and Ece [6] showed that for μ > 0 and if ν > 2 μ 1 , the normalized Miller–Ross function E ν , μ is univalent and starlike in D 1 2 = { z C : | z | < 1 2 } . They also proved that if ν > ( 2 + 2 ) μ 1 , then the normalized Miller–Ross function E ν , μ is univalent and convex in D 1 2 . For more details, refer to Miller and Ross [4].
Simple distributions, including the Pascal, Poisson, logarithmic, binomial and beta-negative binomial, have been substantially examined from a theoretical perspective in geometric function theory; for detailed study, refer to [7,8,9,10,11,12]. The probability mass function of the Miller–Ross-type Poisson distribution is given by
P ν , μ ( m , k ) : = ( m μ ) k m ν E ν , μ ( m ) Γ ( ν + k + 1 ) , k = 0 , 1 , 2 , ,
where ν > 1 , μ > 0 and E ν , μ is the Miller–Ross function given in (2). The normalized form of the Miller–Ross-type Poisson distribution is given by
M ν , μ m ( z ) = z + n = 2 ( m μ ) n 1 m ν E ν , μ ( m ) Γ ( ν + n ) z n .
In the study of geometric function theory, operators are a crucial subject. The convolution of specific analytic functions can be used to express a wide variety of differential and integral operators. It has been noted that this formalism facilitates more mathematical investigation and aids in a better understanding of the symmetric and geometric characteristics of such operators. The work of [13,14] makes it easy to see the significance of convolution in the theory of operators. We consider the linear operator
Q ν , μ m : A A
as below:
Q ν , μ m f z = f z M ν , μ m ( z ) = z + n = 2 Υ n a n z n ,
where
Υ n = ( m μ ) n 1 m ν E ν , μ ( m ) Γ ( ν + n )
and the symbol * specifies the Hadamard product (convolution) of two series.
Moreover, for two analytic functions f and g in D , we say that the function f is subordinate to the function g and write it as
f g or f z g z ,
if there exists a Schwarz function w which is analytic in D with
w 0 = 0 and w z < 1 ,
such that
f z = g w z .
Furthermore, if the function g is univalent in D , then it follows that:
f ( z ) g ( z ) ( z D ) f ( 0 ) = g ( 0 ) and f ( D ) g ( D ) .
Janowski [15] introduced the subclass of starlike functions as follows:
S * ( A , B ) = f ( z ) A : z f ( z ) f ( z ) 1 + A z 1 + B z ( 1 B < A 1 ; z D ) .
Note that 1 + A z 1 + N z maps D conformally onto a symmetrical disc with respect to the real axis, which is centered at 1 A B 1 B 2 ( B ± 1 ) , and with a radius A B 1 B 2 ( B ± 1 ) .
Inspired by all of the aforementioned discussions and recent work by Khan et al. [16], wherein they presented a class of analytic functions with Mittag–Leffler-type Poisson distribution in the Janowski domain; analytic functions with Mittag–Leffler-type Borel distribution [17]; and the work presented in the articles [18,19,20], we now present a new class of analytic functions using operator (5) as follows:
Q ν , μ m A , B = f A : z ( Q ν , μ m f z ) Q ν , μ m f z 1 + A z 1 + B z ( z D ) ,
where 1 B < A 1 . By fixing the values of A and B, one can state new classes Q ν , μ m ( 1 2 α , 1 ) = Q ν , μ m ( α ) , analogues to the classes studied in [21] and Q ν , μ m ( 1 , 1 ) = Q ν , μ m ( φ ) where φ ( z ) = 1 + z 1 z .
In the following sections, for this newly defined function class, we determine the well-known results, like the Fekete–Szegö inequalities, necessary and sufficient conditions, growth and distortion bounds, convex combination, sequential subordination and partial-sum-type results.

2. Initial Coefficient Bounds and Fekete–Szegö Problem for f Q ν , m ( A , B )

To find initial estimates and the Fekete–Szegö problem, the following lemma is required.
Lemma 1
([22,23]). Let
h ( z ) = 1 + p 1 z + p 2 z 2 +
be in the class P of functions of the positive real part in D , then
p n 2 , n 1 ,
and for any complex number υ
p 2 υ p 1 2 2 max 1 , 1 2 υ .
In particular, if υ is a real parameter, then
| p 2 υ p 1 2 | 4 υ + 2 , if υ 0 , 2 , if 0 v 1 , 4 υ 2 , if υ 1 .
When υ < 0 or υ > 1 , the equality holds true in (1) if and only if
h ( z ) = 1 + z 1 z
or one of its rotations. If 0 < υ < 1 , then the equality holds true in (1) if and only if
h ( z ) = 1 + z 2 1 z 2
or one of its rotations. If υ = 0 , the equality holds true in (1) if and only if
h ( z ) = 1 + ρ 2 1 + z 1 z + 1 ρ 2 1 z 1 + z 0 ρ 1
or one of its rotations. If υ = 1 , then the equality in (1) holds true if h ( z ) is a reciprocal of one of the functions such that the equality holds true in the case when υ = 0 .
Theorem 1.
Let f A 0 be assigned to the class Q ν , μ m A , B . Then,
a 2 A B Υ 2 ,
a 3 A B 2 Υ 3 max 1 , | A 2 B | .
Furthermore, for a complex number ,
a 3 a 2 2 A B 2 Υ 3 max 1 , Θ , A , B 1 ,
where
Θ , A , B = ( 1 + 2 B A ) + 2 ( A B ) Υ 3 Υ 2 2 .
Υ 2 = ( m μ ) m ν E ν , μ ( m ) Γ ( ν + 2 ) and Υ 2 = ( m μ ) 2 m ν E ν , μ ( m ) Γ ( ν + 3 ) .
Proof. 
We begin by showing that the inequalities (12)–(14) hold true for f Q ν , μ m A , B . Since f Q ν , μ m A , B , we have the following subordination:
z ( Q ν , μ m f z ) Q ν , μ m f z 1 + A z 1 + B z .
The above subordination can also be written as:
z ( Q ν , μ m f z ) Q ν , μ m f z = 1 + A w z 1 + B w z = G w z , 1 B < A 1 .
Now, w z can be written as follows:
w z = 1 h z 1 + h z = p 1 z + p 2 z 2 + p 3 z 3 + 2 + p 1 z + p 2 z 2 + p 3 z 3 + .
Now,
G w z = 1 + 1 2 A B p 1 z + 1 4 2 A B p 2 A B 1 + B p 1 2 z 2 + .
And
z ( Q ν , μ m f z ) Q ν , μ m f z = 1 + Υ 2 a 2 z + 2 Υ 3 a 3 Υ 2 2 a 2 2 z 2 + .
After comparing (17) and (18), we obtain
a 2 = A B 2 Υ 2 p 1 ,
a 3 = A B 4 Υ 3 p 2 p 1 2 2 1 + 2 B A .
Applying (9) to (19) and (10) to (20), we obtain
a 2 A B Υ 2 ,
a 3 A B 2 Υ 3 max 1 , | A 2 B | .
Furthermore, from (19) and (20), we obtain
a 3 a 2 2 = A B 4 Υ 3 p 2 p 1 2 2 Θ , A , B ,
where
Θ , A , B = ( 1 + 2 B A ) + 2 ( A B ) Υ 3 Υ 2 2 .
Applying (10) to the above (23), we obtain the required results. □
Furthermore, for the real , when applying (11) to the above (23), we obtain the following results.
Theorem 2.
Let f A 0 be assigned to the class Q ν , μ m A , B . Then, for a real parameter ,
a 3 a 2 2 2 ( A 2 B ) Υ 2 2 2 A B Υ 3 Υ 2 2 < ( 1 + 2 B A ) Υ 2 2 2 A B Υ 3 , 2 ( 1 + 2 B A ) Υ 2 2 2 A B Υ 3 ( 1 2 B + A ) Υ 2 2 2 A B Υ 3 , 2 ( 2 B A ) Υ 2 2 + 2 A B Υ 3 Υ 2 2 > ( 1 2 B + A ) Υ 2 2 2 A B Υ 3
where Υ 2 and Υ 3 are as in (15).

3. Coefficient Inequalities for f 1 Q ν , μ m A , B

The Koebe one quarter theorem [24] ensures that the image of D for every univalent function f A 0 contains a disk of radius 1 4 . Thus, every univalent function f has an inverse f 1 satisfying
f 1 ( f ( z ) ) = z , ( z D ) and f ( f 1 ( w ) ) = w , ( | w | < r 0 ( f ) , r 0 ( f ) 1 4 ) .
A function f A 0 is said to be bi-univalent in D if both f and f 1 are univalent in D . We notice that the class of bi-univalent functions defined in the unit disk D is not empty. For example, the functions z, z 1 z , log ( 1 z ) and 1 2 log 1 + z 1 z are members of the bi-univalent function class; however, the Koebe function is not a member.
Theorem 3.
If f Q ν , μ m A , B and f 1 ( w ) = w + n = 2 d n w n is the inverse function of f with | w | < r 0 ( f ) ; r 0 ( f ) 1 4 the Koebe domain of the class f Q ν , μ m A , B , then
| d 2 | A B Υ 2 ,
| d 3 | A B 2 Υ 3 max { 1 , | Θ 2 , A , B 1 | } ,
and for any complex number ℏ, we have
d 3 d 2 2 A B 2 Υ 3 max { 1 , | Θ 2 , A , B + 2 ( A B ) Υ 3 Υ 2 2 1 | } ,
where Θ 2 , A , B = ( 1 + 2 B A ) + 4 ( A B ) Υ 3 Υ 2 2 ; Υ 2 and Υ 3 are as in (15).
Proof. 
As
f 1 ( w ) = w + n = 2 d n w n
is the inverse function of f, it can be seen that
f 1 ( f ( z ) ) = f { f 1 ( z ) } = z .
From (1) and (30), we obtain
f 1 ( z + n = 2 a n z n ) = z .
From Equations (30) and (31), one can obtain
z + ( a 2 + d 2 ) z 2 + ( a 3 + 2 a 2 d 2 + d 3 ) z 3 + = z .
By equating the corresponding coefficients of (32), we have
d 2 = a 2 ,
d 3 = 2 a 2 2 a 3 .
From relations (19) and (33)
d 2 = A B 2 Υ 2 p 1 ; | d 2 | A B Υ 2 .
To find | d 3 | , from (34), we set = 2 in (23). From (23) we have
a 3 a 2 2 = A B 4 Υ 3 p 2 p 1 2 2 Θ , A , B ,
thus
| d 3 | = a 3 2 a 2 2 = A B 4 Υ 3 p 2 p 1 2 2 Θ 2 , A , B ; A B 2 Υ 3 max { 1 , | Θ 2 , A , B 1 | }
where
Θ 2 , A , B = ( 1 + 2 B A ) + 4 ( A B ) Υ 3 Υ 2 2 .
For any complex number , consider
d 3 d 2 2 = A B 4 Υ 3 p 2 p 1 2 2 Θ 2 , A , B ( A B ) 2 4 Υ 2 2 p 1 2 ; = A B 4 Υ 3 p 2 p 1 2 2 Θ 2 , A , B + 2 ( A B ) Υ 3 Υ 2 2 .
Taking the modulus on both sides and by applying Lemma 1 and (9), on the right hand side of (38), one can obtain the result
| d 3 d 2 2 | A B 2 Υ 3 max { 1 , | Θ 2 , A , B + 2 ( A B ) Υ 3 Υ 2 2 1 | }
as in (28). Hence, this completes the proof. □

4. Initial Logarithmic Coefficient Bounds and Fekete–Szegö Problem for f Q ν , m A , B

Inspired by recent works like [25,26], in this section, we determine the coefficient bounds and Fekete–Szegö problem associated with the logarithmic function.
If the function f is analytic in D , such that f ( z ) z 0 for all z D , then the well-known logarithmic coefficients d n : = d n ( f ) , n N , of f are given by
log f ( z ) z = 2 n = 1 d n z n , z D .
For a function f Q ν , m A , B , the left hand side of the subordination of the function defined in (8) should be an analytic function in D ; hence, f ( z ) z 0 for all z D . Therefore, for all functions f Q ν , m , n A , B , the relation (40) is well defined.
Theorem 4.
Let f Q ν , m A , B with the logarithmic coefficients given by (40). Then,
| d 1 | A B 2 Υ 2 , | d 2 | A B 4 Υ 3 max 1 ; 2 B A + ( A B ) Υ 3 Υ 2 2
and for μ C we have
| d 2 μ d 1 2 | A B 4 Υ 3 max 1 ; 2 B A + ( 1 + μ ) ( A B ) Υ 3 Υ 2 2
where Υ 2 and Υ 3 are as in (15).
Proof. 
If f Q ν , m , n A , B has the form (8), equating the first two coefficients of the relation (40), we obtain
d 1 = a 2 2 ,
d 2 = 1 2 a 3 a 2 2 2 .
Replacing a 2 and a 3 in the above equalities with those of (19) and (20), we obtain
d 1 = A B 4 Υ 2 p 1 , d 2 = 1 2 a 3 a 2 2 2 = A B 8 Υ 3 p 2 p 1 2 2 1 + 2 B A ( A B ) 2 16 Υ 2 2 p 1 2 = A B 8 Υ 3 p 2 p 1 2 2 1 + 2 B A + ( A B ) Υ 3 Υ 2 2 .
Using (9), it follows that
| d 1 | A B 2 Υ 2 ,
and using (10), the last equality leads to
| d 2 | A B 4 Υ 3 max 1 ; 2 B A + ( A B ) Υ 3 Υ 2 2 .
Furthermore, we have
d 2 μ d 1 2 = A B 8 Υ 3 p 2 p 1 2 2 1 + 2 B A + ( A B ) Υ 3 Υ 2 2 μ ( A B ) 2 16 Υ 2 2 p 1 2 = A B 8 Υ 3 p 2 p 1 2 2 1 + 2 B A + ( 1 + μ ) ( A B ) Υ 3 Υ 2 2
and in view of (10), we obtain desired result. □

5. Characterization Properties

In this section, we obtain the necessary and sufficient conditions, growth and distortion bounds and convex combination for the newly defined class.
Theorem 5.
Let f A 0 be assigned to the class Q ν , μ m A , B if it fulfills the inequality
n = 2 A B n + n 1 Υ n a n A B ,
equivalently, we may write
n = 2 Ξ n a n A B ,
where
Ξ n = A B n + n 1 Υ n
and Υ n as given in (6). Inequality (41) is sharp.
Proof. 
Assume that inequality (41) holds, and | z | = 1 . Then, one can put (8) in the form of a Schwarz function w z as
z ( Q ν , μ m f z ) Q ν , μ m f z = 1 + A w z 1 + B w z ( z D ) .
It must be shown that the values satisfy the condition
z ( Q ν , μ m f z ) Q ν , μ m f z A Q ν , μ m f z B z ( Q ν , μ m f z ) < 1 .
Then, we have
z ( Q ν , μ m f z ) Q ν , μ m f z A Q ν , μ m f z B z ( Q ν , μ m f z ) = n = 2 n 1 Υ n a n z n A B z + n = 2 A B n Υ n a n z n n = 2 n 1 Υ n | a n | A B n = 2 A B n Υ n | a n | < 1 .
This shows that the values of z ( Q ν , μ m f z ) Q ν , μ m f z lie in a circle centered at w = 1 whose radius is 1 . Hence, f ( z ) Q ν , μ m A , B .
Now, for the function
f z = z + n = 2 A B A B n + n 1 Υ n k n z n , z D ,
such that n = 2 k n = 1 , we have
n = 2 A B n + n 1 Υ n a n = n = 2 A B n + n 1 Υ n A B A B n + n 1 Υ n k n = ( A B ) n = 2 k n = A B .
Thus, f z Q ν , μ m A , B , and the approximation (41) is sharp. □
A function f ( z ) defined by (1) and belonging to the class A 0 is said to be in the class Q ¯ ν , μ m A , B if it is also satisfies the coefficient inequality (41).
Using the technique of proof of distortion theorems given by Silverman [27], we state the following results without proof.
Theorem 6.
If a function f Q ¯ ν , μ m A , B , then
| z | ( A B ) A 2 B + 1 Υ 2 | z | 2 f z | z | + ( A B ) A 2 B + 1 Υ 2 | z | 2 .
The approximation is sharp for the function defined as:
f z = z + ( A B ) A 2 B + 1 Υ 2 z 2 .
Theorem 7.
If a function f Q ¯ ν , μ m A , B , then
1 2 ( A B ) A 2 B + 1 Υ 2 | z | f z 1 + 2 ( A B ) A 2 B + 1 Υ 2 | z | .
The result is sharp for the extreme function defined in (45).
Theorem 8.
Let f i Q ¯ ν , μ m A , B and have the form
f i z = z + n = 2 a i , n z n , for i = 1 , 2 , 3 , , k .
Then, H Q ¯ ν , μ m A , B , where
H z = i = 1 k c i f i z with i = 1 k c i = 1 .
Proof. 
Consider f i Q ¯ ν , μ m A , B . Then, we can write
n = 2 A B n + n 1 Υ n a n A B .
Furthermore,
H z = i = 1 k c i z + n = 2 a i , n z n = z + n = 2 i = 1 k c i a i , n z n ,
therefore
n = 2 A B n + n 1 Υ n i = 1 k c i a i , n = i = 1 k n = 2 A B n + n 1 Υ n a i , n c i i = 1 k ( A B ) c i = ( A B ) i = 1 k c i = A B ,
thus H z Q ¯ ν , μ m A , B .
Theorem 9.
Let f i Q ¯ ν , μ m A , B , for i = 1 , 2 , , j . Then, the arithmetic mean G of f i is given by
G z = 1 j n = 1 j f i z ,
and also belongs to class Q ¯ ν , μ m A , B .
Proof. 
From (49), we can write
G z = 1 j n = 1 j f i z = 1 j n = 1 j z + n = 2 a j , n z n = z + n = 2 1 j n = 1 j a j , n z n .
To show G z belongs to Q ¯ ν , μ m A , B , it is sufficient to show that
n = 2 A B n + n 1 Υ n 1 j n = 1 j a j , n A B .
Consider
n = 2 A B n + n 1 Υ n 1 j n = 1 j a j , n = 1 j n = 1 j n = 2 A B n + n 1 Υ n a j , n 1 j n = 1 j ( A B ) = A B ,
which yields G z Q ¯ ν , μ m A , B .

6. Subordination Results

Now, we recall the following results of Wilf [28], which are very much needed for our study.
Definition 1 (subordinating factor sequence).
A sequence { b n } n = 1 of complex numbers is said to be a subordinating sequence if, whenever f ( z ) = n = 1 a n z n , a 1 = 1 is regular, univalent and convex in U , we have
n = 1 b n a n z n f ( z ) , z D .
Lemma 2.
The sequence { b n } n = 1 is a subordinating factor sequence if and only if
R e 1 + 2 n = 1 b n z n > 0 , z D .
Theorem 10.
Let f Q ¯ ν , μ m A , B and g ( z ) be any function in the usual class of convex functions C , then
Ξ 2 2 [ A B + Ξ 2 ] ( f g ) ( z ) g ( z )
and
R e f ( z ) > [ A B + Ξ 2 ] Ξ 2 , z D .
where
Ξ 2 = ( A 2 B + 1 ) Υ 2 = ( A 2 B + 1 ) ( m μ ) m ν E ν , μ ( m ) Γ ( ν + 2 )
The constant factor Ξ 2 2 [ A B + Ξ 2 ] in (52) cannot be replaced by a larger number.
Proof. 
Let f Q ¯ ν , μ m A , B and suppose that g ( z ) = z + n = 2 b n z n C . Then,
Ξ 2 2 [ A B + Ξ 2 ] ( f * g ) ( z ) = Ξ 2 2 [ A B + Ξ 2 ] z + n = 2 b n a n z n .
Thus, by Definition 1, the subordination result holds true if
Ξ 2 2 [ A B + Ξ 2 ] n = 1
is a subordinating factor sequence, with a 1 = 1 . In view of Lemma 2, this is equivalent to the following inequality
R e 1 + n = 1 Ξ 2 [ A B + Ξ 2 ] a n z n > 0 , z D .
By noting the fact that Ξ 2 [ A B + Ξ 2 ] is an increasing function for n 2 , and in particular
Ξ 2 A B Ξ n A B , n 2 ,
then for | z | = r < 1 , we have
R e 1 + Ξ 2 [ A B + Ξ 2 ] n = 1 a n z n = R e 1 + Ξ 2 [ A B + Ξ 2 ] z + n = 2 Ξ 2 a n z n [ A B + Ξ 2 ] 1 Ξ 2 [ A B + Ξ 2 ] r n = 2 Ξ n a n r n [ A B + Ξ 2 ] 1 Ξ 2 [ A B + Ξ 2 ] r A B [ A B + Ξ 2 ] r > 0 , | z | = r < 1 ,
where we have also made use of assertion (41) of Theorem 5. This evidently proves inequality (56) and hence also the subordination result (52) asserted by (41).
Inequality (53) follows from (52) by taking
g ( z ) = z 1 z = z + n = 2 z n C .
Next, we consider the function
F ( z ) : = z A B Ξ 2 z 2
where Ξ 2 is given by (54). Clearly F Q ¯ ν , μ m A , B . For this function, (52) becomes
Ξ 2 2 [ A B + Ξ 2 ] F ( z ) z 1 z .
It is easily verified that
min Re Ξ 2 2 [ A B + Ξ 2 ] F ( z ) = 1 2 , z D .
This shows that the constant Ξ 2 2 [ A B + Ξ 2 ] cannot be replaced by any larger one. □

7. Partial Sums

In 1997, Silverman [29] examined partial sums results for the class of starlike and convex functions f given by (1) and established through
f 1 z = z , f j z = z + n = 2 a n z n , j = 2 , 3 , 4 , .
Many authors have investigated partial sums for different subclasses; for some recent investigations, we refer to [16,30] and references cited therein.
Theorem 11.
If f of the form (1) satisfies condition (41), then
f z f j z 1 1 Λ j + 1 z D
and
f j z f z Λ j + 1 1 + Λ j + 1 z D ,
where
Λ j = A B n + n 1 A B Υ n .
Proof. 
To prove the approximation (57), we put:
Λ j + 1 f z f j z 1 1 Λ j + 1 = 1 + n = 2 j a n z n 1 + Λ j + 1 n = j + 1 a n z n 1 1 + n = 2 j a n z n 1 = 1 + ψ 1 z 1 + ψ 2 z .
We now set:
1 + ψ 1 z 1 + ψ 2 z = 1 + w z 1 w z .
Then, we find after some worthwhile simplification:
w z = ψ 1 z ψ 2 z 2 + ψ 1 z + ψ 2 z .
Thus, clearly, we find that:
w z = Λ j + 1 n = j + 1 a n z n 1 2 + 2 n = 2 j a n z n 1 + Λ j + 1 n = j + 1 a n z n 1
By implementation of the triangle inequalities with z < 1 , we arrive at the following inequality:
w z Λ j + 1 n = j + 1 a n 2 2 n = 2 j a n Λ j + 1 n = j + 1 a n .
We can now see that:
w z 1
if and only if
2 Λ j + 1 n = j + 1 a n 2 2 n = 2 j a n ,
which hints that:
n = 2 j a n + Λ j + 1 n = j + 1 a n 1 .
Finally, to prove the inequality in (57), it suffices to show that the left hand side of (60) is bounded above by the following sum:
n = 2 Λ n a n ,
which is equivalent to
n = 2 j Λ n 1 a n + n = j + 1 Λ n Λ j + 1 a n 0 .
In light of (61), this is evidence that the proof of the inequality in (57) is now completed.
Next, in order to prove inequality (58), we set:
1 + Λ j + 1 f j z f z Λ j + 1 1 + Λ j + 1 = 1 + n = 2 j a n z n 1 Λ j + 1 n = j + 1 a n z n 1 1 + n = 2 a n z n 1 = 1 + w z 1 w z ,
where
w z 1 + Λ j + 1 n = j + 1 a n 2 2 n = 2 j a n Λ j + 1 1 n = j + 1 a n 1 .
This last inequality in (62) is equivalent to
n = 2 j a n + Λ j + 1 n = j + 1 a n 1 .
Finally, we can see that the left hand side of the inequality in (63) is bounded above by the following sum:
n = 2 Λ n a n ,
so we have completed the proof of assertion (58), which completes the proof of Theorem 11. □
We next turn to ratios involving derivatives.
Theorem 12.
If f of the form (1) satisfies condition (41), then
f z f j z 1 j + 1 Λ j + 1 z D
and
f j z f z Λ j + 1 Λ j + 1 + j + 1 z D ,
where Λ j is given by (59).
Proof. 
The proof of Theorem 12 is similar to that of Theorem 11; we here choose to omit the analogous details. □

8. Conclusions

In this paper, for this newly defined functions class, we have examined several well-known results, including the Fekete–Szegö inequalities, necessary and sufficient conditions, growth and distortion bounds, convex combination, sequential subordination and partial-sum-type results. Furthermore, we believe that this study will motivate a number of researchers to extend this idea for meromorphic functions and harmonic functions. One may also apply this idea to the shell-like and petal-shaped domains instead of the Janowski domain. Several analytic function classes involving Miller–Ross functions have been developed using the concept of subordination based on the geometrical interpretation of their image domains, including the right half plane, circular disc, oval- and petal-type domains, conic domain, leaf-like domain and generalized conic domain, which have all been defined and studied (see [31,32,33,34,35,36,37] for details).

Author Contributions

Conceptualization, G.M., H.Ö.G. and D.B.; investigation, G.M., H.Ö.G. and D.B.; methodology, G.M., H.Ö.G. and D.B.; writing—original draft, G.M., H.Ö.G. and D.B.; writing—review and editing, G.M., H.Ö.G. and D.B. All authors have read and agreed to the published version of the manuscript.

Funding

This research received no external funding.

Data Availability Statement

No data is used in this research.

Conflicts of Interest

The authors declare no conflicts of interest.

References

  1. Fekete, M.; Szegö, G. Eine Bemerkung über ungerade schlichte Funktionen. J. Lond. Math. Soc. 1933, 8, 85–89. [Google Scholar] [CrossRef]
  2. Dziok, J. A general solution of the Fekete-Szegö problem. Bound. Value Probl. 2013, 98, 13. [Google Scholar] [CrossRef]
  3. Kanas, S. An unified approach to the Fekete-Szegö problem. Appl. Math. Comput. 2012, 218, 8453–8461. [Google Scholar] [CrossRef]
  4. Miller, K.S.; Ross, B. An Introduction to the Fractional Calculus and Fractional Differentials; John Wiley and Sons, New York Press: New York, NY, USA, 1993. [Google Scholar]
  5. Wiman, A. Über die Nullstellen der Funktionen Ea(x). Acta Math. 1905, 29, 217–234. [Google Scholar] [CrossRef]
  6. Sümer Eker, S.; Ece, S. Geometric Properties of the Miller-Ross Functions. Iran. J. Sci. Technol. Trans. Sci. 2022, 46, 631–636. [Google Scholar] [CrossRef]
  7. Altınkaya, Ş.; Yalçın, S. Poisson distribution series for certain subclasses of starlike functions with negative coefficients. Annal. Oradea Univ. Math. Fascicola 2017, 24, 5–8. [Google Scholar]
  8. El-Deeb, S.M.; Bulboaca, T.; Dziok, J. Pascal distribution series connected with certain subclasses of univalent functions. Kyungpook Math. J. 2019, 59, 301–314. [Google Scholar]
  9. Nazeer, W.; Mehmood, Q.; Kang, S.M.; Haq, A.U. An application of Bionomial distribution series on certain analytic functions. J. Comput. Anal. Appl. 2019, 26, 11–17. [Google Scholar]
  10. Porwal, S.; Kumar, M. A unified study on starlike and convex functions associated with Poisson distribution series. Afr. Mat. 2016, 27, 10–21. [Google Scholar] [CrossRef]
  11. Wanas, A.K.; Al-Ziadi, N.A. Applications of beta negative binomial distribution series on holomorphic funxtions. Earthline J. Math. Sci. 2021, 6, 271–292. [Google Scholar] [CrossRef]
  12. Wanas, A.K.; Khuttar, J.A. Applications of Borel distribution series on analytic functions. Earthline J. Math. Sci. 2020, 4, 71–82. [Google Scholar] [CrossRef]
  13. Ahmad, B.; Khan, M.G.; Aouf, M.K.; Mashwani, W.K.; Salleh, Z.; Tang, H. Applications of a new q-difference operator in Janowski-type meromorphic convex functions. J. Funct. 2021, 2021, 5534357. [Google Scholar] [CrossRef]
  14. Srivastava, H.M.; Murugusundaramoorthy, G.; Sivasubramanian, S. Hypergeometric functions in the parabolic starlike and uniformly convex domains. Integr. Transf. Spec. Func. 2007, 18, 511–520. [Google Scholar] [CrossRef]
  15. Janowski, W. Some extremal problems for certain families of analytic functions. Bull. Acad. Plolon. Sci. Ser. Sci. Math. Astronomy 1973, 21, 17–25. [Google Scholar] [CrossRef]
  16. Khan, M.G.; Ahmad, B.; Khan, N.; Mashwani, W.K.; Arjika, S.; Khan, B.; Chinram, R. Applications of Mittag–Leffler type poisson distribution to a subclass of analytic functions involving conic-type regions. J. Funct. Spaces 2021, 2021, 4343163. [Google Scholar]
  17. Srivastava, H.M.; El-Deeb, S.M. Fuzzy differential subordinations based upon the Mittag–Leffler type Borel distribution. Symmetry 2021, 13, 1023. [Google Scholar] [CrossRef]
  18. El-Deeb, S.M.; Murugusundaramoorty, G.; Alburaikan, A. A bi-Bazilevič functions based on the Mittag–Leffler-Type Borel distribution associated with Legendre polynomials. J. Math. Comput. Sci. 2021, 24, 235–245. [Google Scholar] [CrossRef]
  19. Srivastava, H.M.; Murugusundaramoorty, G.; El-Deeb, S.M. Faber polynomial coefficient estimates of bi-close-to-convex functions connected with Borel distribution of the Mittag–Leffler-type. J. Nonlinear Var. Anal. 2021, 5, 103–118. [Google Scholar]
  20. Sümer Eker, S.; Murugusundaramoorthy, G.; Şeker, B.; Çekiç, B. Spiral-like functions associated with Miller–Ross-type Poisson distribution series. Boletin Soc. Matematica Mex. 2023, 29, 16. [Google Scholar] [CrossRef]
  21. Robertson, M.S. Certain classes of starlike functions. Mich. Math. J. 1985, 32, 135–140. [Google Scholar] [CrossRef]
  22. Keogh, F.R.; Merkes, E.P. A coefficient inequality for certain classes of analytic functions. Proc. Am. Math. Soc. 1969, 20, 8–12. [Google Scholar] [CrossRef]
  23. Ma, W.; Minda, D. A unified treatment of some special classes of univalent functions. In Proceedings of the Conference on Complex Analysis, Tianjin, China, 19–23 June 1992; Li, Z., Ren, F., Yang, L., Zhang, S., Eds.; International Press: Cambridge, MA, USA, 1994; pp. 157–169. [Google Scholar]
  24. Duren, P.L. Univalent Functions. In Grundlehren der Mathematischen Wissenschaften; Band 259; Springer: New York, NY, USA; Berlin/Heidelberg, Germany; Tokyo, Japan, 1983. [Google Scholar]
  25. Alimohammadi, D.; Adegani, E.A.; Bulboaca, T.; Cho, N.E. Logarithmic coefficients for classes related to convex functions. Bull. Malays. Math. Sci. Soc. 2021, 44, 2659–2673. [Google Scholar] [CrossRef]
  26. Alimohammadi, D.; Adegani, E.A.; Bulboaca, T.; Cho, N.E. Logarithmic coefficients bounds and coefficient conjectures for classes associated with convex functions. J. Funct. Spaces 2021, 2021, 6690027. [Google Scholar] [CrossRef]
  27. Silverman, H. Univalent functions with negative coefficients. Proc. Am. Math. Soc. 1975, 51, 109–116. [Google Scholar] [CrossRef]
  28. Wilf, H.S. Subordinating factor sequence for convex maps of the unit circle. Proc. Am. Math. Soc. 1961, 12, 689–693. [Google Scholar] [CrossRef]
  29. Silverman, H. Partial sums of starlike and convex functions. J. Math. Anal. Appl. 1997, 209, 221–227. [Google Scholar] [CrossRef]
  30. Rosy, T.; Subramanian, K.G.; Murugusundaramoorthy, G. Neighbourhoods and Partial sums of Starlike Functions Based on Ruscheweyh Derivatives. J. Ineq. Pure Appl. Math. 2003, 64, 4. [Google Scholar]
  31. Cho, N.E.; Kumar, S.; Kumar, V.; Ravichandran, V. Radius problemsfor starlike functions associated with the sine function. Bull. Iran. Math. Soc. 2019, 45, 213–232. [Google Scholar] [CrossRef]
  32. Mendiratta, R.; Nagpal, S.; Ravichandran, V. On a subclass ofstrongly starlike functions associated with exponential functions. Bull. Malays. Math. Sci. Soc. 2015, 38, 365–386. [Google Scholar] [CrossRef]
  33. Sharma, K.; Jain, N.K.; Ravichandran, V. Starlike functionsassociated with cardioid. Afrika Math. 2016, 27, 923–939. [Google Scholar] [CrossRef]
  34. Wani, L.A.; Swaminathan, A. Starlike and convex functionsassociated with a Nephroid domain. Bull. Malays. Math. Sci. Soc. 2021, 44, 79–104. [Google Scholar] [CrossRef]
  35. Sokól, J. Radius problem in the class SL*. Appl. Math. Comput. 2009, 214, 569–573. [Google Scholar] [CrossRef]
  36. Raina, R.K.; Sokól, J. On Coefficient estimates for acertain class of starlike functions. Hacettepe. J. Math. Statist. 2015, 44, 1427–1433. [Google Scholar] [CrossRef]
  37. Gandhi, S. Radius estimates for three leaf functions and convexcombination of starlike functions. In Mathematical Analysis 1: Approximation Theory; Deo, N., Gupta, V., Acu, A., Agrawal, P., Eds.; Springer: Singapore, 2018; Volume 306. [Google Scholar]
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Murugusundaramoorthy, G.; Güney, H.Ö.; Breaz, D. Starlike Functions of the Miller–Ross-Type Poisson Distribution in the Janowski Domain. Mathematics 2024, 12, 795. https://doi.org/10.3390/math12060795

AMA Style

Murugusundaramoorthy G, Güney HÖ, Breaz D. Starlike Functions of the Miller–Ross-Type Poisson Distribution in the Janowski Domain. Mathematics. 2024; 12(6):795. https://doi.org/10.3390/math12060795

Chicago/Turabian Style

Murugusundaramoorthy, Gangadharan, Hatun Özlem Güney, and Daniel Breaz. 2024. "Starlike Functions of the Miller–Ross-Type Poisson Distribution in the Janowski Domain" Mathematics 12, no. 6: 795. https://doi.org/10.3390/math12060795

APA Style

Murugusundaramoorthy, G., Güney, H. Ö., & Breaz, D. (2024). Starlike Functions of the Miller–Ross-Type Poisson Distribution in the Janowski Domain. Mathematics, 12(6), 795. https://doi.org/10.3390/math12060795

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