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Article

Coefficient Bounds for Symmetric Subclasses of q-Convolution-Related Analytical Functions

by
Sheza M. El-Deeb
1,†,‡ and
Luminita-Ioana Cotîrlă
2,*,‡
1
Department of Mathematics, Faculty of Science, Damietta University, New Damietta 34517, Egypt
2
Department of Mathematics, Technical University of Cluj-Napoca, 400114 Cluj-Napoca, Romania
*
Author to whom correspondence should be addressed.
Current address: Department of Mathematics, College of Science and Arts, Al-Badaya, Qassim University, Buraydah 51911, Saudi Arabia.
These authors contributed equally to this work.
Symmetry 2023, 15(6), 1133; https://doi.org/10.3390/sym15061133
Submission received: 22 April 2023 / Revised: 17 May 2023 / Accepted: 19 May 2023 / Published: 23 May 2023

Abstract

:
By using q-convolution, we determine the coefficient bounds for certain symmetric subclasses of analytic functions of complex order, which are introduced here by means of a certain non-homogeneous Cauchy–Euler-type differential equation of order m.

1. Introduction, Definitions and Preliminaries

Assume that A is the class of analytic functions in the open disc Λ : = { ζ C : | ζ | < 1 } of the form
Υ ( ζ ) = ζ + t = 2 + a t ζ t , ζ Λ .
If the function h A is given by
h ( ζ ) = ζ + t = 2 + c t ζ t , ζ Λ .
The Hadamard (or convolution) product of Υ and h is defined by
( Υ h ) ( ζ ) : = ζ + t = 2 + a t c t ζ t , ζ Λ .
A function Υ A belongs to the class S * ( η ) if
1 + 1 η ζ Υ ( ζ ) Υ ( ζ ) 1 > 0 ζ Λ ; η C * = C \ { 0 } .
Furthermore, a function Υ A be in the class C ( η ) if
1 + 1 η ζ Υ ( ζ ) Υ ( ζ ) > 0 ζ Λ ; η C * .
The classes S * ( η ) and C ( η ) were studied by Nasr and Aouf [1,2] and Wiatrowski [3].
In a wide range of applications in the mathematical, physical, and engineering sciences, the theory of q-calculus is important. Jackson [4,5] was the first to use the q-calculus in various applications and to introduce the q-analogue of the standard derivative and integral operators; see [6,7,8,9,10]. About coefficients’ interesting results, see [11,12,13,14,15,16]. The q-shifted factorial is defined for λ , q C and n N 0 = N { 0 } as follows
( λ ; q ) t =         1                 t = 0 , 1 λ 1 λ q 1 λ q t 1                         t N .
Using the q-gamma function Γ q ( ζ ) , we obtain
( q λ ; q ) t = 1 q t Γ q λ + t Γ q λ , t N 0 ,
where
Γ q ( ζ ) = 1 q 1 ζ q ; q q ζ ; q , q < 1 .
In addition, we note that
λ ; q = t = 0 1 λ q t , q < 1 ,
and the q-gamma function Γ q ( ζ ) is known
Γ q ( ζ + 1 ) = ζ q Γ q ( ζ ) ,
where t q denotes the basic q-number defined as follows
[ t ] q : = 1 q t 1 q ,                 t C , 1 + j = 1 t 1 q j ,                 t N .
Using the definition Formula (5), we have the next two products:
(i)
For any non negative integer t, the q-shifted factorial is given by
[ t ] q ! : = 1 , if t = 0 , n = 1 t [ n ] q , if t N .
(ii)
For any positive number r, the q-generalized Pochhammer symbol is defined by
r q , t : = 1 , if t = 0 , n = r r + t 1 [ n ] q , if t N .
It is known in terms of the classical (Euler’s) gamma function Γ ζ , that
Γ q ζ Γ ζ as q 1 .
In addition, we observe that
lim q 1 q λ ; q t 1 q t = λ t ,
where λ t is given by
λ t = 1 , if t = 0 , λ λ + 1 λ + t 1 , if t N . .
For 0 < q < 1 . El-Deeb et al. [17] defined that the q-derivative operator for Υ h is defined by
D q Υ h ( ζ ) : = D q ( ζ + t = 2 + a t c t ζ t ) = Υ h ( ζ ) Υ h ( q ζ ) ζ ( 1 q ) = 1 + t = 2 + [ t ] q a t c t ζ t 1 , ζ Λ ,
Let ϑ > 1 and 0 < q < 1 ; El-Deeb et al. [17] defined the linear operator R h ϑ , q : A A as follows:
R h ϑ , q Υ ( ζ ) N q , ϑ + 1 ( ζ ) = ζ D q Υ h ( ζ ) , ζ Λ ,
where the function M q , ϑ + 1 is given by
N q , ϑ + 1 ( ζ ) : = ζ + t = 2 + [ ϑ + 1 ] q , t 1 [ t 1 ] q ! ζ t , ζ Λ .
A simple computation shows that
R h ϑ , q Υ ( ζ ) : = ζ + t = 2 + [ t ] q ! [ ϑ + 1 ] q , t 1 a t c t ζ t , ζ Λ ( ϑ > 1 , 0 < q < 1 ) .
Remark 1 
([17]). From the definition relation (6), we can obtain that the next relations hold for all Υ A :
( i ) [ ϑ + 1 ] q R h ϑ , q Υ ( ζ ) = [ ϑ ] q R h ϑ + 1 , q Υ ( ζ ) + q ϑ ζ D q R h ϑ + 1 , q Υ ( ζ ) , ζ Λ ; ( ii ) I h ϑ Υ ( ζ ) : = lim q 1 R h ϑ , q Υ ( ζ ) = ζ + t = 2 + t ! ( ϑ + 1 ) t 1 a t c t ζ t , ζ Λ .
Remark 2 
([17]). By taking different particular cases for the coefficients c t , El-Deeb et al. [17] observed the following special cases for the operator R h ϑ , q :
(i) 
For c t = ( 1 ) t 1 Γ ( ρ + 1 ) 4 t 1 ( t 1 ) ! Γ ( t + ρ ) , ρ > 0 , El-Deeb and Bulboacă [18] and El-Deeb [19] obtained the operator N ρ , q ϑ studied by:
N ρ , q ϑ Υ ( ζ ) : = ζ + t = 2 + ( 1 ) t 1 Γ ( ρ + 1 ) 4 t 1 ( t 1 ) ! Γ ( t + ρ ) · [ t ] q ! [ ϑ + 1 ] q , t 1 a t ζ t = ζ + t = 2 + [ t ] q ! [ ϑ + 1 ] q , t 1 ψ t a t ζ t , ζ Λ , ( ρ > 0 , ϑ > 1 , 0 < q < 1 ) ,
where
ψ t : = ( 1 ) t 1 Γ ( ρ + 1 ) 4 t 1 ( t 1 ) ! Γ ( t + ρ ) ;
(ii) 
For c t = m + 1 m + t α , α > 0 , m 0 , El-Deeb and Bulboacă [20] and Srivastava and El-Deeb [21] obtained the operator N m , 1 , q ϑ , α = : M m , q ϑ , α studied by:
M m , q ϑ , α Υ ( ζ ) : = ζ + t = 2 + m + 1 m + t α · [ t ] q ! [ ϑ + 1 ] q , t 1 a t ζ t , ζ Λ ;
(iii) 
For c t = n t 1 ( t 1 ) ! e n , n > 0 , El-Deeb et al. [17] obtained the q-analogue of Poisson operator defined by:
I q ϑ , n Υ ( ζ ) : = ζ + t = 2 + n t 1 ( t 1 ) ! e n · [ t ] q ! [ ϑ + 1 ] q , t 1 a t ζ t , ζ Λ ;
(iv) 
For c t = 1 + + λ ( t 1 ) 1 + n , n Z , 0 , λ 0 , El-Deeb et al. [17] obtained the q-analogue of Prajapat operator defined by
J q , , λ ϑ , n Υ ( ζ ) : = ζ + t = 2 + 1 + + λ ( t 1 ) 1 + n · [ t ] q ! [ ϑ + 1 ] q , t 1 a t ζ t , ζ Λ .
In this paper, we define the following subclasses SC h ϑ , q η , γ , β and N h ϑ , q η , γ , β , m , μ ( η C * , 0 γ 1 , 0 β < 1 , ϑ > 1 , 0 < q < 1 , m N * = N \ { 1 } = { 2 , 3 , 4 , } , μ R \ , 1 ) as follows:
Definition 1.
For a function Υ has the form (1) and h is defined by (2), the function Υ belongs to the class SC h ϑ , q η , γ , β if
1 + 1 η ζ 1 γ R h ϑ , q Υ ( ζ ) + γ ζ R h ϑ , q Υ ( ζ ) 1 γ R h ϑ , q Υ ( ζ ) + γ ζ R h ϑ , q Υ ( ζ ) 1 > β
η C * ; 0 γ 1 ; 0 β < 1 ; ϑ > 1 , 0 < q < 1 ; ζ Λ .
Remark 3.
(i) 
For q 1 , we obtain that lim q 1 SC h ϑ , q η , γ , β = : G h ϑ η , γ , β , where G h ϑ η , γ , β represents the functions Υ A that satisfies (13) for R h ϑ , q replaced with I h ϑ (7).
(ii) 
For c t = ( 1 ) t 1 Γ ( ρ + 1 ) 4 t 1 ( t 1 ) ! Γ ( t + ρ ) , ρ > 0 , we obtain the subclass B ρ ϑ , q η , γ , β , that represents the functions Υ A that satisfies (13) for R h ϑ , q replaced with N ρ , q ϑ (8).
(iii) 
For c t = m + 1 m + t α , α > 0 , m 0 , we obtain the class M m , α ϑ , q η , γ , β , that represents the functions Υ A that satisfies (13) for R h ϑ , q replaced with M m , q ϑ , α (10).
(iv) 
For c t = n t 1 ( t 1 ) ! e n , n > 0 , we obtain the class I t ϑ , q η , γ , β , that represents the functions Υ A that satisfies (13) for R h ϑ , q replaced with I q ϑ , t (11).
(v) 
For c t = 1 + + λ ( t 1 ) 1 + n , n Z , 0 , λ 0 , we obtain the class J n , , λ ϑ , q η , γ , β , that represents the functions Υ A that satisfies (13) for R h ϑ , q replaced with J q , , λ ϑ , n (12).
The following lemma must be used in to show our study results:
Definition 2.
A function Υ A belongs to the class N h ϑ , q η , γ , β , m , μ if it satisfies the following non-homogeneous Cauchy–Euler type differential equation of order m:
ζ m d m w d ζ m + m 1 μ + m 1 ζ m 1 d m 1 w d ζ m 1 + + m m w j = 0 m 1 μ + j = g ( ζ ) j = 0 m 1 μ + j + 1
w = Υ ( ζ ) ; g ( ζ ) SC h ϑ , q η , γ , β ; η C * , 0 γ 1 , 0 β < 1 ; ϑ > 1 ; 0 < q < 1 ; m N * ; μ R \ , 1 .
Remark 4.
(i) 
Putting q 1 , we obtain that lim q 1 N h ϑ , q η , γ , β , m , μ = : T h ϑ η , γ , β , m , μ , where T h ϑ η , γ , β , m , μ represents the functions Υ A that satisfies (13) for R h ϑ , q replaced with I h λ (7).
(ii) 
Putting c t = ( 1 ) t 1 Γ ( ρ + 1 ) 4 t 1 ( t 1 ) ! Γ ( t + ρ ) , ρ > 0 , we get the subclass P ρ ϑ , q η , γ , β , m , μ , that represents the functions Υ A that satisfies (13) for R h ϑ , q replaced with N ρ , q ϑ (8).
(iii) 
Putting c t = m + 1 m + t α , α > 0 , m 0 , we have the class R m , α ϑ , q η , γ , β , m , μ , that represents the functions Υ A that satisfies (13) for R h ϑ , q replaced with M m , q ϑ , α (10).
(iv) 
Putting c t = n t 1 ( t 1 ) ! e n , n > 0 , we get the class D n ϑ , q η , γ , β , m , μ , that represents the functions Υ A that satisfies (13) for R h ϑ , q replaced with I q ϑ , n (11).
(v) 
Putting c t = 1 + + λ ( t 1 ) 1 + n , n Z , 0 , λ 0 , we have the class J n , , λ ϑ , q η , γ , β , m , μ , that represents the functions Υ A that satisfies (13) for R h ϑ , q replaced with J q , , λ ϑ , n (12).
The main object of the present investigation is to derive some coefficient bounds for functions in the subclasses SC h ϑ , q η , γ , β and N h ϑ , q η , γ , β , m , μ of A .

2. Coefficient Estimates for the Function Class SC h ϑ , q η , γ , β

Unless otherwise mentioned, we assume throughout this paper that:
η C * , 0 γ 1 , 0 β < 1 ; m N * ; μ R \ , 1 , ϑ > 1 ; 0 < q < 1 , ζ Λ .
Theorem 1.
Assume that the function Υ given by (1) belongs to the class SC h ϑ , q η , γ , β , then
a t [ ϑ + 1 ] q , t 1 i = 0 t 2 [ i + 2 ( 1 β ) | η | ] ( t 1 ) ! [ 1 + γ ( t 1 ) ] [ t ] q ! c t t N * .
Proof. 
The function Υ A be given by (1)and let the function F ( ζ ) be defined by
F ( ζ ) = 1 γ R h ϑ , q Υ ( ζ ) + γ ζ R h ϑ , q Υ ( ζ ) .
Then from (13) and the definition of the function F ( ζ ) above, it is easily seen that
1 + 1 η ζ F ( ζ ) F ( ζ ) 1 > β
with
F ( ζ ) = ζ + t = 2 + Θ t ζ t Θ t = [ t ] q ! [ ϑ + 1 ] q , t 1 1 + γ ( t 1 ) a t c t ; t N * .
Thus, by setting
1 + 1 η ζ F ( ζ ) F ( ζ ) 1 β 1 β = g ( ζ )
or, equivalently,
ζ F ( ζ ) = 1 + η 1 β g ( ζ ) 1 F ( ζ ) ,
we get
g ( ζ ) = 1 + d 1 ζ + d 2 ζ 2 + .
Since g ( ζ ) > 0 , we conclude that d t 2 t N (see [14]).
We get from (15) and (16) that
( t 1 ) Θ t = η 1 β d 1 Θ t 1 + d 2 Θ t 2 + + d t 1 .
For t = 2 , 3 , 4 , we have
Θ 2 = η 1 β d 1 Θ 2 2 1 β η ,
2 Θ 3 = η 1 β d 1 Θ 2 + d 2 Θ 3 2 1 β η 1 + 2 1 β η 2 ! ,
and
3 Θ 4 = η 1 β d 1 Θ 3 + d 2 Θ 2 + d 3 Θ 4 2 1 β η 1 + 2 1 β η 2 + 2 1 β η 3 ! ,
respectively. Using the principle of mathematical induction, we obtain
Θ t i = 0 t 2 i + 2 ( 1 β ) η ( t 1 ) ! t N * .
Using the relationship between the functions Υ ( ζ ) and F ( ζ ) , we get
Θ t = [ t ] q ! [ ϑ + 1 ] q , t 1 1 + γ ( t 1 ) a t c t t N * ,
and then we get
a t [ ϑ + 1 ] q , t 1 i = 0 t 2 i + 2 ( 1 β ) η ( t 1 ) ! 1 + γ ( t 1 ) [ t ] q ! c t t N * .
This completes the proof of Theorem 1. □
Putting q 1 in Theorem 1, we obtain the following corollary:
Corollary 1.
If the function Υ given by (1) belongs to the class G h ϑ η , γ , β , then
a t ϑ + 1 t 1 i = 0 t 2 i + 2 ( 1 β ) η t ( t 1 ) ! 2 1 + γ ( t 1 ) c t t N * .
Taking c t = ( 1 ) t 1 Γ ( ρ + 1 ) 4 t 1 ( t 1 ) ! Γ ( t + ρ ) , ρ > 0 in Theorem 1, we obtain the following special case:
Example 1.
If the function Υ given by (1) belongs to the class B ρ ϑ , q η , γ , β , then
a t 4 t 1 Γ ( t + ρ ) [ ϑ + 1 ] q , t 1 i = 0 t 2 i + 2 ( 1 β ) η ( 1 ) t 1 Γ ( ρ + 1 ) 1 + γ ( t 1 ) [ t ] q ! t N * .
Considering c t = m + 1 m + t α , α > 0 , m 0 in Theorem 1, we obtain the following result:
Example 2.
If the function Υ given by (1) belongs to the class M m , α ϑ , q η , γ , β , then
a t m + t α [ ϑ + 1 ] q , t 1 i = 0 t 2 i + 2 ( 1 β ) η ( t 1 ) ! 1 + γ ( t 1 ) [ t ] q ! m + 1 α t N * .
Putting c t = n t 1 ( t 1 ) ! e n , n > 0 in Theorem 1, we obtain the following special case:
Example 3.
If the function Υ given by (1) belongs to the class I n ϑ , q η , γ , β , then
a t [ ϑ + 1 ] q , t 1 i = 0 t 2 i + 2 ( 1 β ) η n t 1 1 + γ ( t 1 ) [ t ] q ! e n t N * .
Putting c t = 1 + + λ ( t 1 ) 1 + n , n Z , 0 , λ 0 in Theorem 1, we obtain the following special case:
Example 4.
If the function Υ given by (1) belongs to the class J n , , λ ϑ , q η , γ , β , m , μ , then
a t 1 + n [ ϑ + 1 ] q , t 1 i = 0 t 2 i + 2 ( 1 β ) η ( t 1 ) ! 1 + γ ( t 1 ) [ t ] q ! 1 + + λ ( t 1 ) n t N * .
Putting c t = 1 and ϑ = 1 in Corollary 1, we obtain the following special case:
Example 5.
If the function Υ given by (1) belongs to the class G ζ 1 ζ 1 η , γ , β , then
a t i = 0 t 2 i + 2 ( 1 β ) η ( t 1 ) ! 1 + γ ( t 1 ) t N * .

3. Coefficient Estimates for the Function Class N h ϑ , q η , γ , β , m , μ

Our main coefficient bounds for function in the class N h ϑ , q η , γ , β , m , μ are given by Theorem 2 below.
Theorem 2.
If the function Υ given by (1) belongs to the class N h ϑ , q η , γ , β , m , μ , then
a t [ ϑ + 1 ] q , t 1 i = 0 t 2 i + 2 ( 1 β ) η i = 0 m 1 μ + i + 1 ( t 1 ) ! 1 + γ ( t 1 ) [ t ] q ! i = 0 m 1 μ + i + t c t t N * .
Proof. 
Let the function Υ A be given by (1)and let the function g define as follows
g ( ζ ) = ζ + t = 2 + d t ζ t SC h ϑ , q η , γ , β ,
so that
a t = i = 0 m 1 μ + i + 1 i = 0 m 1 μ + i + 1 d t t , m N * ; μ R \ , 1 .
a t [ ϑ + 1 ] q , t 1 r = 0 t 2 r + 2 ( 1 β ) η i = 0 m 1 μ + i + 1 ( t 1 ) ! 1 + γ ( t 1 ) [ t ] q ! i = 0 m 1 μ + i + t c t j N * .
Thus, by using Theorem 1, we readily complete the proof of Theorem 2. □
Putting q 1 in Theorem 1, we obtain the following corollary:
Corollary 2.
If the function Υ given by (1) belongs to the class T h ϑ η , γ , β , m , μ , then
a t ϑ + 1 t 1 r = 0 t 2 r + 2 ( 1 β ) η i = 0 m 1 μ + i + 1 t ( t 1 ) ! 2 1 + γ ( t 1 ) i = 0 m 1 μ + i + t c t t N * .
Putting c t = 1 and ϑ = 1 in Corollary 2, we obtain the following example:
Example 6.
If the function Υ given by (1) belongs to the class T ζ 1 ζ 1 η , γ , β , m , μ , then
a j r = 0 t 2 r + 2 ( 1 β ) η i = 0 m 1 μ + i + 1 ( t 1 ) ! 1 + γ ( t 1 ) i = 0 m 1 μ + i + t t N * .

4. Conclusions

We investigated certain subclasses of analytic functions of complex order combined with the linear q-convolution operator. For the functions in this new class, we obtained the coefficient bounds and introduced here by means of a certain non-homogeneous Cauchy–Euler-type differential equation of order m. There was also consideration of several interesting corollaries and applications of the results by suitably fixing the parameters, as illustrated in Remark 1.

Author Contributions

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

Funding

This research received no external funding.

Data Availability Statement

Not applicable.

Conflicts of Interest

The authors declare no conflict of interest.

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El-Deeb, S.M.; Cotîrlă, L.-I. Coefficient Bounds for Symmetric Subclasses of q-Convolution-Related Analytical Functions. Symmetry 2023, 15, 1133. https://doi.org/10.3390/sym15061133

AMA Style

El-Deeb SM, Cotîrlă L-I. Coefficient Bounds for Symmetric Subclasses of q-Convolution-Related Analytical Functions. Symmetry. 2023; 15(6):1133. https://doi.org/10.3390/sym15061133

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El-Deeb, Sheza M., and Luminita-Ioana Cotîrlă. 2023. "Coefficient Bounds for Symmetric Subclasses of q-Convolution-Related Analytical Functions" Symmetry 15, no. 6: 1133. https://doi.org/10.3390/sym15061133

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