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https://doi.org/10.5831/HMJ.2019.41.1.101

GEOMETRIC PROPERTIES OF GENERALIZED DINI FUNCTIONS

Erhan Deniz and S¸eyma G¨oren

Abstract. In this paper our aim is to establish some geometric properties (like starlikeness, convexity and close-to-convexity) for the generalized and normalized Dini functions. In order to prove our main results, we use some inequalities for ratio of these functions in normalized form and classical result of Fejer.

1. Introduction and preliminaries Let A be the class of functions of the from

f (z) = z +

X

n=2

anzn, which are analytic in the open unit disk

U = {z : |z| < 1, z ∈ C}.

Bessel functions of the first kind play an important role in applied math- ematics and other branches of engineering. Many authors who study on geometric funtions theory are interested in some geometric proper- ties such as univalency, starlikeness, convexity and close-to-convexity of Bessel functions (see, [1, 2, 3, 4, 5, 6, 7], [10]). We denote by S the subclass of A consisting of functions f (z) ∈ A which are univalent in U . A function f ∈ S is said to be starlike of order β(0 ≤ β < 1) if and only if

< zf0(z) f (z)



> β.

Received May 22, 2018. Accepted January 14, 2019.

2010 Mathematics Subject Classification. 33C10, 30C45.

Key words and phrases. Bessel functions of the fist kind, convex functions, starlike functions, close-to-convex functions, Dini function.

This research has been supported by Kafkas University Scientific Research Projects Coordination Unit. Project Number 2018-FEF-15.

*Corresponding author

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We detone by S(β) the class of all such functions. Also, we note that S(0) = S is the usual class of starlike funtions in U . A function f ∈ S is said to be convex of order β(0 ≤ β < 1) if and only if

<



1 +zf00(z) f0(z)



> β.

We detone by C(β) the class of all such functions. Also, we note that C(0) = C is the usual class of convex functions in U . A function f ∈ S , g ∈ S is said to be close-to-convex of order β(0 ≤ β < 1) if and only if

< zf0(z) g (z)



> β.

We detone by K (β) the class of all such functions. Also, we note that K (0) = K is the usual close-to- convex functions in U .

Let us consider the following second-order linear homogenaus differential equation (see, for details, [11]):

(1) z2ω00(z) + bzω0(z) +cz2− ν2+ (1 − b)ν ω(z) = 0 (b, c, ν ∈ C) . The function ων,b,c(z), which is called the generalized Bessel function of the first kind of order ν, is defined as a particular solution of (1). We have the following familiar series representation for the function ων,b,c(z) (2) ων,b,c(z) =

X

n=0

(−c)n

n!Γ (ν + n + (b + 1) /2)

z 2

2n+ν

(z ∈ C) where Γ stands for the Euler gamma function. The series (2) permits the study of Bessel, modifiye Bessel and spherical Bessel functions in a unified manner. Each of these particular cases of the function ων,b,c(z) is worthy of mention here.

For b = c = 1 in (2) , we obtain the familiar Bessel function of the first kind of order ν defined by

Jν(z) =

X

n=0

(−1)n n!Γ (ν + n + 1)

z 2

2n+ν

(z ∈ C) .

For b = 1 and c = −1 in (2) , we obtain the modified Bessel function of the first kind of order ν defined by

Iν(z) =

X

n=0

1 n!Γ (ν + n + 1)

z 2

2n+ν

(z ∈ C) . For b = 2 and c = 1 in (2), the function ων,b,c(z) reduces to√

2jν(z)√ π, where jν is the spherical Bessel function of the first kind of order ν

(3)

defined by

jν(z) =r π 2

X

n=0

(−1)n n!Γ (ν + n + 32)

z 2

2n+ν

(z ∈ C) .

Deniz et al. [6] considered the function ψν,b,c(z) defined, in terms of the generalized and normalized Bessel function ων,b,c(z), by the transforma- tion

(3) ψν,b,c(z) = 2νΓ



ν + b + 1 2



z1−ν/2ων,b,c(√ z).

By using the well-known Pochhammer symbol (or the shifted factorial) (λ)µdefined, for λ, µ ∈ C and in terms of the Euler Γ- function, by

(λ)µ= Γ (λ + µ) Γ (λ) =

 1

λ (λ + 1) ... (λ + n − 1)

(µ = 0; λ ∈ C − {0}) (µ = n ∈ N; λ ∈ C) . It is being understood conventionally that (0)0 := 1, and we obtain the following series representation for the function ψν,b,c(z) given by (3)

ψν,b,c(z) = z +

X

n=1

(−c)n 4n(κ)n

zn+1 n!

where N := {1, 2, 3, ...}, Z0 := {0, −1, −2, ...} and κ := ν + b+12 ∈ Z/ 0 In [7] authors defined and studied the generalized Dini functions Dν,a,b,c: C → C by

Dν,a,b,c(z) = (a − ν) ων,b,c(z) + zω0ν,b,c(z) (a, b, c, ν ∈ C) and its normalized form

ϕν,a,b,c(z) = 2 a

ν

Γ



ν + b + 1 2



z1−ν2Dν,a,b,c √ z

where ων,b,c is the generalized Bessel function of first kind. From the definition of ϕν,a,b,c(z) we obtain series representation as

ϕν,a,b,c(z) = z +

X

n=1

(−c)n(2n + a) a4nn! (κ)n zn+1. To prove our main results we need the following Lemmas.

Lemma 1.1. [8] If the function f (z) = P

n=1Anzn, where A1 = 1 and An ≥ 0 for all n ≥ 2 is analytic in U , and the sequences {nAn− (n + 1)An+1}n≥1 and {nAn}n≥1 both are decreasing, then f is starlike in U .

(4)

Lemma 1.2. [9] If f ∈ A satisfy

f (z) z − 1

< 1 for each z ∈ U , then f is starlike in U1/2=z : |z| < 12 .

Lemma 1.3. [9] If f ∈ A satisfy |f0(z) − 1| < 1 for each z ∈ U , then f is convex in U1/2 =z : |z| < 12 .

Lemma 1.4. [9] If f ∈ A satisfy |f0(z) − 1| < 2

5 for each z ∈ U , then f is starlike in U = {z : |z| < 1}.

Lemma 1.5. [10] If 0 ≤ β < 1, f ∈ A satisfy |zf00(z)| < 1−β4 for each z ∈ U , then <(f0(z)) > 1+β4 in U = {z : |z| < 1}.

Recently Baricz et al [4] studied the close-to-convexity of Dini func- tions. Some monotonicity properties and functional inequalities for the modified Dini function are discussed in [5]. Further some geometric prop- erties of Dini functions are studied in [7]. In this paper we determine the conditions on parameters that ensure the generalized and normal- ized Dini function ϕν,a,b,c(z) to be starlike of order β, convex of order β and close-to-convex of the given order in U and U1/2. We also study the starlikeness by using the Fejer lemma (Lemma 1.1) which completely different method.

2. Geometric Properties of generalized Dini Functions Throughout our present investigation, we tacitly assume that κ :=

ν + b+12 .

Theorem 2.1. Let a ∈ R+, b ∈ R, c ∈ C, κ ∈ R − {Z∪ {0}} with β ∈ [0, 1) and z ∈ U . If

κ >

a,c,β−q

2a,c,β− 8a(β −1) |c| (−8(2 + a)(β −2) + (16 + a − 2β) |c|) 16a(β − 1)

then ϕv,a,b,c(z) ∈ S(β), where

a,c,β = 4(β − 2) |c| + a(8 − 5 |c| + β(3 |c| − 8)).

Proof. We use the inequality

0ν,a,b,c(z) ϕν,a,b,c(z) − 1

< 1 − β to prove the starlikeness of order β for the function ϕv,a,b,c(z). So by using the well- known triangle inequality

|z1+ z2| ≤ |z1| + |z2|

(5)

and following inequalities

(4) 8(n − 1)!(κ + 1)n−1≥ n [2(κ + 1)]n−1,

2(n − 1)!(κ + 1)n−1≥ [2(κ + 1)]n−1, n ∈ N we obtain

ϕ0ν,a,b,c(z)−ϕν,a,b,c(z) z

=

X

n=1

n(2n + a) (−c)n a4nn! (κ)n zn

X

n=1

n(2n + a) |c|n a4nn! (κ)n

= |c|

2κa

X

n=1

n

4n−1(n − 1)! (κ + 1)n−1|c|n−1 + |c|

X

n=1

1

4n−1(n − 1)! (κ + 1)n−1|c|n−1

≤ |c|

2κa+|c|

4κ+ 4 |c|

κa + |c|

 X

n=2

 |c|

8 (κ + 1)

n−1

=|c|2[14 + a] + |c| 8 (κ + 1) (2 + a) 4aκ (8 (κ + 1) − |c|) . Furthermore, if we use reverse triangle inequality

|z1+ z2| ≥ ||z1| − |z2||

and the inequalities (4) then we get

ϕν,a,b,c(z) z

≥ 1 −

X

n=1

(2n + a) (−c)n a4nn! (κ)n zn

= 1 −

"

2 |c|

4κa +2 |c|

4κa

X

n=2

|c|n−1

4n−1(n − 1)! (κ + 1)n−1

#

"

|c|

4κ+ |c|

X

n=2

|c|n−1 4n−1n! (κ + 1)n−1

#

≥ 1 −

"

|c|

2κa + |c|

4κ+ |c|

κa + |c|

 X

n=2

 |c|

8 (κ + 1)

n−1#

= −2 |c|2− |c| 4 (aκ + 2 (a + 2) (κ + 1)) + 32aκ (κ + 1) 4aκ (8 (κ + 1) − |c|) .

(6)

By combining the above inequalities, we obtain

0ν,a,b,c(z) ϕν,a,b,c(z) − 1

≤ |c|2[14 + a] + |c| 8 (κ + 1) (2 + a)

−2 |c|2− |c| 4 (aκ + 2 (a+2) (κ+1)) + 32aκ (κ + 1). Consequently, by the hypothesis of theorem we have

|c|2[14 + a] + |c| 8 (κ + 1) (2 + a)

−2 |c|2− |c| 4 (aκ + 2 (a + 2) (κ + 1)) + 32aκ (κ + 1) < 1 − β that is,

0ν,a,b,c(z) ϕν,a,b,c(z) − 1

< 1 − β.

So, ϕv,a,b,c(z) is starlike function of order β.

Theorem 2.2. Let a ∈ R+, b ∈ R, c ∈ C, κ ∈ R − {Z∪ {0}} with β ∈ [0, 1) and z ∈ U . If

κ > 20 |c| + a−8√

5 + 10 +√

5 |c| + p5Ψa,c,β 16√

5a then ϕv,a,b,c(z) ∈ S, where

Ψa,c,β = 80 |c|2+ 8a |c|

h 8√

5 + 10 |c| + 9√ 5 |c|

i +a2

h

64 + |c|



−16 + 32√

5 + 21 |c| + 8

√ 5 |c|

i . Proof. To prove this teorem, we use Lemma 1.4. From the well-known triangle inequality and the inequalities (4) we have

ϕ0ν,a,b,c(z) − 1 ≤

X

n=1

2n2+ n (a + 2) + a a4nn! (κ)n |c|n

X

n=1

2n

a4n(n − 1)! (κ)n|c|n +a + 2

a

X

n=1

1

4n(n − 1)! (κ)n|c|n+

X

n=1

1

4nn! (κ)n|c|n

≤ |c|

2κa+(a + 2) |c|

4κa + |c|

4κ + 4 |c|

κa +(a + 2) |c|

2κa + |c|

 X

n=2

 |c|

8 (κ + 1)

n−1

= (16 + a) |c|2+ 16 (a + 2) (κ + 1) |c|

4aκ (8 (κ + 1) − |c|) .

(7)

Therefore from hypothesis of theorem we obtain

ϕ0ν,a,b,c(z) − 1

≤ (16 + a) |c|2+ 16 (a + 2) (κ + 1) |c|

4aκ (8 (κ + 1) − |c|) < 2

√ 5. So, from Lemma 1.4 ϕv,a,b,c(z) is starlike function.

Theorem 2.3. Let a ∈ R+, b ∈ R, c ∈ C, κ ∈ R − {Z∪ {0}} with β ∈ [0, 1) and z ∈ U . If

κ >

Θa,c,β−q

Θ2a,c,β+ Πa,c,β+ Γa,c,β 16a(β − 1)

then ϕv,a,b,c(z) ∈ C(β), where

Θa,c,β = 8(β − 2) |c| + a(6 − 7 |c| + β(5 |c| − 8)), Πa,c,β = 8a(β − 1)(4 |c| (−16 − 15 |c| + 4β(|c| + 2)),

Γa,c,β = a(−8 + |c| (−23 + 6 |c| + β(16 + |c|))).

To prove the convexity of order β of function ϕv,a,b,c(z), we have to show that

00ν,a,b,c(z) ϕ0ν,a,b,c(z)

< 1 − β. By using the well-known triangle inequality

|z1+ z2| ≤ |z1| + |z2|

and the inequalities (4) and 32(n − 1)!(κ + 1)n−1≥ n2[2(κ + 1)]n−1 for n ∈ N, we have

(5)

z2ϕ00ν,a,b,c(z) ≤

X

n=1

(2n + a) (n + 1) a4n(n − 1)! (κ)n|c|n

≤ |c|

2aκ

X

n=1

n2

4n−1(n − 1)! (κ + 1)n−1 |c|n−1 +(a + 2) |c|

4aκ

X

n=1

n

4n−1(n − 1)! (κ + 1)n−1 |c|n−1 +|c|

X

n=1

1

4n−1(n − 1)! (κ + 1)n−1 |c|n−1

(8)

≤ |c|

2κa +16 |c|

κa

X

n=2

 |c|

8 (κ + 1)

n−1

+ a + 2 a

 |c|

4κ+ a + 2 a

 2 |c|

κ

X

n=2

 |c|

8 (κ + 1)

n−1

+|c|

4κ+ |c|

X

n=2

 |c|

8 (κ + 1)

n−1

= (44 − 7a) |c|2+ (8 (κ + 1) (a + 4) − a) |c| + 8a (κ + 1)

4aκ (8 (κ + 1) − |c|) .

Moreover, if we use reverse triangle inequality

|z1+ z2| ≥ ||z1| − |z2||

and the inequalities (4), we have

0ν,a,b,c(z) (6)

≥ 1 −

X

n=1

2n2+ n (a + 2) + a a4nn! (κ)n |c|n

≥ 1 −

" X

n=1

2n

a4n(n − 1)! (κ)n|c|n+

X

n=1

a + 2

a4n(n − 1)! (κ)n|c|n

#

X

n=1

a

a4nn! (κ)n|c|n

≥ 1 −

"

|c|

2κa +4 |c|

κa

X

n=2

 |c|

8 (κ + 1)

n−1#

"

 a + 2 a

 |c|

4κ+ a + 2 a

 |c|

X

n=2

 |c|

8 (κ + 1)

n−1#

−|c|

4κ− |c|

X

n=2

 |c|

8 (κ + 1)

n−1

= − (16 + a) |c|2− (4aκ + 8 (κ + 1) (2a + 4)) |c| + 32aκ (κ + 1)

4aκ (8 (κ + 1) − |c|) .

(9)

Consequently, from (5), (6) and by the hypothesis of teorem we get

00ν,a,b,c(z) ϕ0ν,a,b,c(z)

≤ (44 − 7a) |c|2+ (8 (κ + 1) (a + 4) − a) |c| + 8a (κ + 1)

−(16+a) |c|2−(4aκ+8 (κ+1)(2a+4)) |c| + 32aκ (κ+1)

< 1 − β

Theorem 2.4. Let a ∈ R+, b ∈ R, c ∈ C, κ ∈ R − {Z∪ {0}} with β ∈ [0, 1) and z ∈ U . If

κ > 4 |c| + a(3 |c| − 8) + q

64a2+ 16a(a + 4) |c| + (a + 4)(9a + 4) |c|2 16a

then ϕv,a,b,c(z) is starlike in U1/2.

Proof. By using the well-known triangle inequality and the second inequality in (4) we get

ϕν,a,b,c(z)

z − 1

X

n=1

(2n + a) (−c)n a4nn! (κ)n zn

≤ |c|

2κa + |c|

2κa

X

n=2

|c|n−1

4n−1(n − 1)! (κ + 1)n−1 +|c|

4κ+ |c|

X

n=2

|c|n−1 4n−1n! (κ + 1)n−1

≤ |c|

2κa + |c|

4κ+ |c|

κa + |c|



X

n=2

 |c|

8 (κ + 1)

n−1

= 2 |c|2+ 8(κ + 1)(2 + a) |c|

4aκ(8(κ + 1) − |c|) . Since the hypothesis of theorem we obtain

2 |c|2+ 8(κ + 1)(2 + a) |c|

4aκ(8(κ + 1) − |c|) < 1.

Consequently, from Lemma 1.2 ϕv,a,b,c(z) is starlike in U1/2.

Theorem 2.5. Let a ∈ R+, b ∈ R, c ∈ C, κ ∈ R − {Z∪ {0}} with β ∈ [0, 1) and z ∈ U . If

κ > a(5 |c|−8)+8 |c|+

q

64a2+16a(3a+8) |c| + [64+a(33a+208)] |c|2 16a

then ϕv,a,b,c(z) is convex in U1/2.

(10)

Proof. By using the well-known triangle inequality and the inequali- ties (4) for n ∈ N, we have

ϕ0ν,a,b,c(z) − 1 ≤

X

n=1

2n2+ n (a + 2) + a a4nn! (κ)n |c|n

= 2 a

X

n=1

n

4n(n − 1)! (κ)n|c|n +a + 2

a

X

n=1

1

4n(n − 1)! (κ)n|c|n+

X

n=1

1

4nn! (κ)n|c|n

≤ |c|

2κa +4 |c|

κa

X

n=2

 |c|

8 (κ + 1)

n−1

+ a + 2 a

 |c|

4κ+ a + 2 a

 |c|

X

n=2

 |c|

8 (κ + 1)

n−1

+|c|

4κ+ |c|

X

n=2

 |c|

8 (κ + 1)

n−1

= (16 + a) |c|2+ 16 (a + 2) (κ + 1) |c|

4aκ (8 (κ + 1) − |c|) . Thus, from the hypothesis of theorem we obtain

(16 + a) |c|2+ 16 (a + 2) (κ + 1) |c|

4aκ (8 (κ + 1) − |c|) < 1 and so we have required result by using Lemma 1.3.

Theorem 2.6. Let a ∈ R+, b ∈ R, c ∈ C, κ ∈ R − {Z∪ {0}} with β ∈ [0, 1) and z ∈ U . If

κ >

$a,c,β −q

$2a,c,β+ ξa,c,β+ κa,c,β

16a(β − 1)

then <ϕ0v,a,b,c(z) > 1+β4 or ϕv,a,b,c(z) is close-to-convexity of order 1+β4 where,

$a,c,β = 8(β − 5) |c| + a [β(5 |c| − 8) − 13 |c|] , ξa,c,β = 8a(β − 1)(16 |c| [β(2 + |c| − 2(5 + 6 |c|)]), κa,c,β = a(−32 + |c| [−44 + 27 |c| + β(16 + |c|)] .

(11)

Proof. By using the well-known triangle inequality and the inequali- ties (4) and 32(n − 1)!(κ + 1)n−1≥ n2[2(κ + 1)]n−1, we have

00ν,a,b,c(z) ≤

X

n=1

(2n + a) (n + 1) a4n(n − 1)! (κ)n|c|n

= |c|

2aκ

X

n=1

n2

4n−1(n − 1)! (κ + 1)n−1|c|n−1 +(a + 2) |c|

4aκ

X

n=1

n

4n−1(n − 1)! (κ + 1)n−1|c|n−1 +|c|

X

n=1

1

4n−1(n − 1)! (κ + 1)n−1|c|n−1

≤ |c|

2κa +16 |c|

κa

X

n=2

 |c|

8 (κ + 1)

n−1

+ a + 2 a

 |c|

4κ+ a + 2 a

 2 |c|

κ

X

n=2

 |c|

8 (κ + 1)

n−1

+|c|

4κ+ |c|

X

n=2

 |c|

8 (κ + 1)

n−1

= (44 − 7a) |c|2+ (8 (κ + 1) (a + 4) − a) |c| + 8a (κ + 1)

4aκ (8 (κ + 1) − |c|) .

Thus, from the hypothesis of theorem we obtain

(44 − 7a) |c|2+ (8 (κ + 1) (a + 4) − a) |c| + 8a (κ + 1)

4aκ (8 (κ + 1) − |c|) < 1 − β 4 . Consequently by using Lemma 1.5, we have required result.

Theorem 2.7. Let a ∈ R+, b ∈ R and c < −0, 117874. If κ > N (c), then ϕν,a,b,c∈ S, where N (c) =√

143c2+ 152c + 64 − 12c − 8.

From the definition of the function ϕν,a,b,c we write ϕν,a,b,c(z) =

X

n=1

Anzn where

An= [2 (n − 1) + a] (−c)n−1

a4n−1(n − 1)! (κ)n−1 , A1 = 1.

(12)

Since c < −0, 117874 we have An> 0 for all n ≥ 1. Let An= Fn+ Gn, where

Fn= 2 (−c)n−1

a4n−1(n − 2)! (κ)n−1 > 0 and Gn= (−c)n−1

4n−1(n − 1)! (κ)n−1 > 0.

To prove the theorem we use Lemma 1.1. Namely we must prove that the sequences {nAn}n≥1 and {nAn− (n + 1)An+1}n≥1 are decreasing.

First we prove that the sequence {nAn}n≥1 is decreasing. For this we must show that the sequences {nFn}n≥2 and {nGn}n≥1 is also decreas- ing.

Firstly, we show that the sequence {nFn}n≥2 is decreasing. From the definition of Fn, we have

nFn−(n + 1)Fn+1 = 2n (−c)n−1

a4n−1(n − 2)! (κ)n−1 − 2 (n + 1) (−c)n a4n(n − 1)! (κ)n

= 2 (−c)n−1 a4n−1(n − 2)! (κ)n−1



n − (n + 1) (−c) 4 (n − 1) (κ + n − 1)



= Fn

 4n (n − 1) (κ + n − 1) + (n + 1) c 4 (n − 1) (κ + n − 1)

 .

Let U1(n) = 4n (n − 1) (κ + n − 1) + (n + 1) c. Since c is negative, κ >

N (c) > −3c8 − 1 > −c4 − 1 and (n − 1)2 ≥ 2(n − 1) − 1 for n ≥ 2, we obtain

U1(n) = nh

4 (n − 1)2+ 4 (n − 1) κ + ci + c

≥ n [8 (n − 1) − 4 + 4 (n − 1) κ + c] + c

≥ n [4 (κ + 1) + c] + c ≥ 8 (κ + 1) + 3c > 0.

Consequently we have shown that nFn− (n + 1)Fn+1 > 0. This shows that the sequence {nFn}n≥2 is strictly decreasing.

Next, we show that the sequence {nGn}n≥1 is decreasing. From the definition of Gn, we have

nGn− (n + 1)Gn+1 = n (−c)n−1

4n−1(n − 1)! (κ)n−1 −(n + 1) (−c)n 4n(n)! (κ)n

= (−c)n−1

4n−1(n − 1)! (κ)n−1



n + (n + 1) c 4n (κ + n − 1)



= Gn

 4n3+ n2(4κ − 4) + nc + c 4n (κ + n − 1)

 .

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Let V1(n) = 4n3 + n2(4κ − 4) + nc + c. Since n3 ≥ 3n2 − 3n + 1, n2 ≥ 2n − 1 for n ≥ 1 and κ > N (c) > −2c > −c+48 , we have

V1(n) = 4n3+ n2(4κ − 4) + nc + c

≥ 4 3n2− 3n + 1 + n2(4κ − 4) + nc + c

= n2(4κ + 8) + n (c − 12) + c + 4

≥ n (c + 4 + 8κ) + c − 4κ − 4 > 0.

Consequently we have nGn − (n + 1)Gn+1 > 0. This shows that the sequence {nGn}n≥1 is strictly decreasing. Therefore the sequence {nAn}n≥1 is strictly decreasing.

Second, we prove that the sequence {nAn−(n+1)An+1}n≥1 is de- creasing. For this we must show that the sequences {nFn−(n+1)Fn+1}n≥2 and {nGn− (n + 1)Gn+1}n≥1 are also decreasing.

Now, we show that the sequence {nFn− (n + 1)Fn+1}n≥2is decreas- ing. For convenience we denote Kn= nFn− (n + 1)Fn+1 for each n ≥ 1.

Thus we get

Kn− Kn+1= nFn− 2(n + 1)Fn+1+ (n + 2)Fn+2

= 2 (−c)n−1 a4n−1(n − 2)! (κ)n−1

×



n+ (n + 1) c

2 (n−1) (κ+n−1)+ (n + 2) c2

16n (n−1) (κ+n) (κ+n−1)



= Fn

 U2(n)

16n (n − 1) (κ + n) (κ + n − 1)



where

U2(n) = 16n5+ 16n4(2κ − 2) + 16n3 κ2− 3κ + 1 + c/2 +16n2 κ − κ2+ (κ + 1) c/2 + n 8cκ + c2 + 2c2.

Our aim is to show that U2(n) > 0. First we observe that n4 ≥ 4n3− 6n2+ 4n − 1 holds. By using this inequality we obtain

U2(n) ≥ n

16 4n3− 6n2+ 4n − 1 + 16n3(2κ − 2) +16n2 κ2− 3κ + 1 + c/2

+16n κ − κ2+ (κ + 1) c/2 + 8cκ + c2

+ 2c2

= n

 16n3(2κ + 2) + 16n2 κ2− 3κ + 5 + c/2

+16n 4 + κ − κ2+ (κ + 1) c/2 + 8cκ + c2− 16

 +2c2 : = X1(n).

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Clearly, the coefficient of n3in the above expression is nonnegative, since κ > N (c) > −1. Therefore using that n3 ≥ 3n2− 3n + 1, we obtain X1(n) ≥ n

16 3n2− 3n + 1 (2κ + 2) +16n2 κ2− 3κ + 5 + c/2

+16n 4 + κ − κ2+ (κ + 1) c/2 + 8cκ + c2− 16

+2c2

= n

16n2 κ2+ 3κ + 1 + c/2

+16n −2 − 5κ − κ2+ (κ + 1) c/2 + 32κ + 8cκ + c2+ 16

+ 2c2 : = X2(n).

Similarly the coefficient κ2+ 3κ + 1 + c/2 of n2 in the above expression is nonnegative, since κ > N (c). Therefore using that n2 ≥ 2n − 1, we obtain

X2(n) ≥ n

16 (2n − 1) κ2+ 3κ + 1 + c/2 +16n −2 − 5κ − κ2+ (κ + 1) c/2 + 32κ + 8cκ + c2+ 16

+ 2c2

= n

 16n κ2+ κ + c + (κ + 1) c/2 + −16κ2− 16κ − 8c + 8cκ + c2

 + 2c2 := X3(n).

Now, we observe that κ2+κ+c+(κ + 1) c/2 is also nonnegative, because κ > N (c). Therefore for n ≥ 2, we have

X3(n) ≥ n16κ2+ 16κ + 40c + 24cκ + c2 + 2c2:= X4(n).

Since κ > N (c), we have 16κ2+ 16κ + 40c + 24cκ + c2> 0 . Thus we obtain for n ≥ 2

X4(n) ≥ 32κ2+ 32κ + 80c + 48cκ + 4c2 := X5(n) > 0.

Thus, we have proved a chain of inequalities

U2(n) ≥ X1(n) ≥ X2(n) ≥ X3(n) ≥ X4(n) ≥ X5(n) > 0,

which implies Kn−Kn+1> 0. Consequently this shows that the sequence {Kn}n≥2 is strictly decreasing.

Next, we show that the sequence {nGn− (n + 1)Gn+1}n≥1is decreasing.

For convenience we denote Pn= nGn− (n + 1)Gn+1for n ≥ 1. Therefore we find that

Pn− Pn+1 = nGn− 2 (n + 1) Gn+1+ (n + 2) Gn+2

= Gn

 V2(n)

16n (n + 1) (κ + n − 1) (κ + n)



(15)

where V2(n) = n

 16n4+ 32κn3+ n2 16κ2+ 16κ − 16 + 8c +n 16κ2− 16κ + 16c + 8κc + 16κc + 8c + c2



+8cκ+2c2. Our aim is to show that V2(n) > 0. First we observe that n4 ≥ 4n3− 6n2+ 4n − 1 holds. By using this inequality we obtain

V2(n) ≥ = n

32n3(κ + 2) + n2 16κ2+ 16κ − 112 + 8c +n 16κ2− 16κ + 16c + 8κc + 64

+16κc + 8c + c2− 16

+8cκ+2c2 : = Y1(n).

Clearly, the coefficient of n3in κ+2 the above expression is nonnegative, since κ > N (c). Therefore using that n3 ≥ 3n2− 3n + 1, we obtain

Y1(n) ≥ n

n2 16κ2+ 112κ + 80 + 8c

+n 16κ2− 112κ + 16c + 8κc − 128 +16κc + 8c + 32κ + c2+ 48

+ 8cκ + 2c2 : = Y2(n).

Similarly the coefficient of n2 in the above expression is nonnegative, since κ > N (c). Therefore using that n2 ≥ 2n − 1, we obtain

Y2(n) ≥ n

 n 48κ2+ 112κ + 32c + 8κc + 32

−16κ2− 80κ + 16κc + c2− 32



+ 8cκ + 2c2 := Y3(n).

Now, we observe that 48κ2+ 112κ + 32c + 8κc + 32 is also nonnegative, because κ > N (c). Therefore for n ≥ 1 we can deduce easily that

Y3(n) ≥ n 32 κ2+ κc + c + 1 + c2 + 8κc + c2:=Y4(n).

Since κ > N (c) we have 32 κ2+ κc + c + 1 + c2> 0 for n ≥ 1. Thus we get

Y4(n) ≥ 32 κ2+ κc + c + 1 + 3c2 := Y5(n) > 0.

Consequently we have proved a chain of inequalities

V2(n) ≥ Y1(n) ≥ Y2(n) ≥ Y3(n) ≥ Y4(n) ≥ Y5(n) > 0.

This implies that the sequence {Pn}n≥1 is strictly decreasing.

Since the sequences {Kn} and {Pn} are strictly decreasing, {nAn− (n + 1)An+1}n≥1

is also strictly decreasing.

Consequently using Lemma 1.1 ϕν,a,b,c∈ S.

(16)

References

[1] ´A. Baricz, Geometric properties of generalized Bessel functions, Publ. Math.

Debrecen 73(1-2) (2008), 155-178.

[2] ´A. Baricz and S. Ponnusamy, Starlikeness and convexity of generalized Bessel functions, Integr. Transforms Spec. Funct. 21 (2010), 641-653.

[3] ´A. Baricz, M. C¸ a˘glar and E. Deniz, Starlikeness of Bessel functions and their derivatives, Math. Ineq. Appl. 19(2) (2016), 439–449.

[4] ´A. Baricz, E. Deniz and N. Ya˘gmur, Close-to-convexity of normalized Dini func- tions, Math. Narch. 289 (2016), 1721-1726.

[5] ´A. Baricz. S. Ponnusamy and S. Singh, Modified Dini functions: monotonicity patterns and functional inequalities, Acta Math. Hungrica 149 (2016), 120-142.

[6] E. Deniz, H. Orhan and H. M. Srivastava, Some sufficient conditions for univa- lence of certain families of integral operators involving generalized Bessel func- tions, Taiwanese J. Math. 15(2) (2011), 883-917.

[7] E. Deniz, S¸. G¨oren and M. C¸ a˘glar, Starlikeness and convexity of the general- ized Dini functions, AIP Conference Proceedings 1833(020004) (2017), doi:

10.1063/1.4981652.

[8] L. Fejer, Untersuchungen ¨uber Potenzreihen mit mehrfach monotoner Koeffizien- tenfolg e, Acta Litterarum ac Scientiarum 8 (1936), 89–115.

[9] T. H. MacGregor, A class of univalent functions, Proc. Amer. Math. Society, 15 (1964), 311-317.

[10] S. Owa, M. Nunokawa, H. Saitoh and H. M. Srivastava, Close-to-convexity, starlikeness, and convexity of certain analytic functions, Appl. Math. Lett. 15 (2002), 63-69.

[11] G. N. Watson, A treatise on the theory of Bessel functions, Second edition, Cam- bridge University Press, Cambridge, London and New York, 1944.

Erhan Deniz

Department of Mathematics, Kafkas University, Kars 36100, Turkey.

E-mail: edeniz36@gmail.com S¸eyma G¨oren

Department of Mathematics, Kafkas University, Kars 36100, Turkey.

E-mail: seyma mat36@hotmail.com

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