1 Introduction

Let us consider the following second-order linear homogeneous differential equation (see for details [1] and [2]):

z 2 ω (z)+bz ω (z)+ [ c z 2 u 2 + ( 1 b ) u ] ω(z)=0(u,b,cC).
(1.1)

The function ω u , b , c (z), which is called the generalized Bessel function of the first kind of order u, it is defined as a particular solution of (1.1). The function ω u , b , c (z) has the familiar representation as

ω u , b , c (z)= n = 0 ( c ) n n ! Γ ( u + n + b + 1 2 ) ( z 2 ) 2 n + u (zC).
(1.2)

Here Γ stands for the Euler gamma function. The series (1.2) permits the study of Bessel, modified Bessel, and spherical Bessel function altogether. It is worth mentioning that, in particular:

  1. (1)

    For b=c=1 in (1.2), we obtain the familiar Bessel function of the first kind of order u defined by

    J u (z)= n = 0 ( 1 ) n n ! Γ ( u + n + 1 ) ( z 2 ) 2 n + u (zC).
    (1.3)
  2. (2)

    For b=1 and c=1 in (1.2), we obtain the modified Bessel function of the first kind of order u defined by

    I u (z)= n = 0 1 n ! Γ ( u + n + 1 ) ( z 2 ) 2 n + u (zC).
    (1.4)
  3. (3)

    For b=2 and c=1 in (1.2), the function ω u , b , c (z) reduces to 2 π j u (z) where j u is the spherical Bessel function of the first kind of order u, defined by

    j u (z)= π 2 n = 0 ( 1 ) n n ! Γ ( u + n + 3 2 ) ( z 2 ) 2 n + u (zC).
    (1.5)

In [3], the author considered the function φ u , b , c (z) defined, in terms of the generalized Bessel function ω u , b , c (z). From (1.2), it is clear that ω(0)=0. Therefore, it follows from (1.2)

ω u , b , c (z)= [ 2 u Γ ( u + b + 1 2 ) ] 1 z u n = 0 ( c 4 ) n n ! Γ ( u + n + b + 1 2 ) z 2 n ,zC.
(1.6)

Let us set

φ u , b , c (z)= n = 0 b n z n ,

where

b n = ( c 4 ) n n ! Γ ( u + n + b + 1 2 ) .

Hence, (1.6) becomes

ω u , b , c (z)= [ 2 u Γ ( u + b + 1 2 ) ] 1 z u φ u , b , c ( z 2 ) .
(1.7)

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

ω u , b , c ( z ) = [ 2 u Γ ( u + b + 1 2 ) ] 1 z u φ u , b , c ( z 2 ) , ( λ ) μ : = Γ ( λ + μ ) Γ ( λ ) = { 1 ( μ = 0 ; λ C { 0 } ) , λ ( λ + 1 ) ( λ + n 1 ) ( μ = n N ; λ C ) ,
(1.8)

where it is being understood conventionally that ( 0 ) 0 =1. Therefore, we obtain the following series representation for the function φ u , b , c (z) given by (1.6):

φ u , b , c (z)=z+ n = 1 ( c ) n z n + 1 4 n ( κ ) n n ! (zC),
(1.9)

where κ=u+ b + 1 2 Z 0 , N={1,2,} and Z 0 ={0,1,2,}, and therefore

φ u , b , c (z)=z+ n = 2 ( c / 4 ) n 1 z n ( κ ) n 1 ( n 1 ) ! ( κ : = u + b + 1 2 Z 0 ) ,
(1.10)

where N:={1,2,3,} and Z 0 :={0,1,2,}. The function φ u , b , c is called the generalized and ‘normalized’ Bessel function of the first kind of order u. We note that by the ratio test, the radius of convergence of the series φ u , b , c (z) is infinity. Moreover, the function φ u , b , c is analytic in ℂ and satisfies the differential equation 4 z 2 φ (z)+4κz φ (z)+czφ(z)=0. For convenience, we write φ κ , c (z)= φ u , b , c (z). Let A denote the class of functions of the form

f(z)=z+ n = 2 a n z n ,
(1.11)

which are analytic in the open unit disk U={zU:|z|<1}. Let S be the subclass of A consisting of univalent functions in U with the normalized condition f(0)=0= f (0)1. A function fA is said to be starlike of order η if it satisfies ( z f ( z ) f ( z ) )>η (zU) for some η (0η<1) and we denote the class of functions which are starlike of order η in U as S ( η ) . Also, a function fA is said to be convex of order η if it satisfies (1+ z f ( z ) f ( z ) )>η (zU) for some η (0η<1) and we denote by C ( η ) the class of all convex functions of order η in U. It follows by the Alexander relation that fC(η)z f S (η). The classes S ( η ) and C(η) were introduced by Robertson [4] (see also Srivastava and Owa [5]). Let fA and g S (η). Then f is said to be close to convex of order γ and type η if and only if ( z f ( z ) g ( z ) )>γ (zU) where 0γ<1 and 0η<1. The classes K(γ,η) were introduced by Libera [6] (see also Noor and Al-Kharsani [7], Silverman [8] and Shanmugam and Ramachandran [9]). Furthermore, we denote by k-UCV and k-ST (0k<), two interesting subclasses of S consisting, respectively, of functions which are k-uniformly convex and k-starlike in U defined for 0k< by

k-UCV:= { f S : ( 1 + z f ( z ) f ( z ) ) > k | z f ( z ) f ( z ) | ( z U ) }

and

k-ST:= { f S : ( z f ( z ) f ( z ) ) > k | z f ( z ) f ( z ) 1 | ( z U ) } .

The class k-UCV was introduced by Kanas and Wiśniowska in [10], where its geometric definition and connections with the conic domains were considered. The class k-ST was investigated in [11]. In fact, it is related to the class k-UCV by means of the well-known Alexander equivalence between the usual classes of convex and starlike functions (see also the work of Kanas and Srivastava [12] for further developments involving each of the classes k-UCV and k-ST). In particular, when k=1, we obtain k-UCVUCV and k-ST=SP, where UCV and SP are the familiar classes of uniformly convex functions and parabolic starlike functions in U, respectively. We remark here that the classes k-UCVUCV and k-ST=SP are related to the domain bounded by conical sections. Motivated by works of Kanas and Wiśniowska [10] and [11], Al-Kharsani and Al-Hajiry [13] introduced the classes k-uniformly convex functions and k-starlike functions of order η (0η<1) as below:

k-UCV(η):= { f S : ( 1 + z f ( z ) f ( z ) η ) > k | z f ( z ) f ( z ) | ( z U ) }
(1.12)

and

k-ST(η):= { f S : ( z f ( z ) f ( z ) η ) > k | z f ( z ) f ( z ) 1 | ( z U ) } .
(1.13)

In the case when k=0 the inequalities (1.12) and (1.13) reduce to the well-known classes of starlike and convex functions of order η, respectively. Further, as mentioned earlier, for the special choices of η=0 and k=1 the class k-UCV(η) reduces to the class of uniformly convex functions introduced by Goodman [14] and the class k-UCV(η) reduces to the class of parabolic starlike functions studied extensively by Rønning [15] (see also the work of Ma and Minda [16]). If f and g are analytic in U, then we say that the function f is subordinate to g, if there exists a Schwarz function w(z), analytic in U with w(0)=0 and |w(z)|<1 (zU), such that f(z)=g(w(z)) (zU). We denote this subordination by fg or f(z)g(z) (zU). In view of the earlier works studied by Kanas and Kanas et al. [1012, 1722], Sim et al. [23] and Al-Kharsani [24] defined the domain Ω k , η for 0k< as

Ω k , η = { u + i v : ( u η ) 2 > k 2 ( u 1 ) 2 + k 2 v 2 } .

Note that, for 0<k<1,

Ω k , η = { u + i v : ( u + k 2 η 1 k 2 k ( 1 η 1 k 2 ) ) 2 ( v 1 η 1 k 2 ) 2 > 1 } ,

for k>1,

Ω k , η = { u + i v : ( u + k 2 η k 2 1 k ( 1 η k 2 1 ) ) 2 + ( v 1 η k 2 1 ) 2 < 1 } .

The explicit form of the extremal function that maps U onto the conic domain Ω k , η is given by

Q k , η (z)= { 1 + ( 1 2 η ) z 1 z k = 0 , 1 + 2 ( 1 η ) π 2 log 2 ( 1 + z 1 z ) , k = 1 , 1 + 2 ( 1 η ) 1 k 2 sinh 2 ( A ( k ) arctanh z ) , 0 < k < 1 , ( 1 η ) k 2 1 sin 2 ( π 2 κ ( t ) F ( z t , t ) ) + k 2 η k 2 1 , k > 1 ,

where A(k)= 2 π arccosk, F(ω,t) is the Legendre elliptic integral of the first kind

F(ω,t)= 0 ω d x 1 x 2 1 t 2 x 2 ,κ(t)=F(1,t)

and t(0,1) is chosen such that k=cosh π κ ( t ) 4 κ ( t ) . In view of the definition of subordination and the extremal function Q k , η (z),

fk-ST(η) z f ( z ) f ( z ) Q k , η (z)
(1.14)

and

fk-UCV(η)1+ z f ( z ) f ( z ) Q k , η (z).
(1.15)

Therefore,

( p ( z ) ) > ( Q k , η ( z ) ) > k + η k + 1 .
(1.16)

Define UCC(k,η,β) as the family of functions fA such that

z f ( z ) g ( z ) Q k , η (z)for some g(z)k-ST(β)(0β<1).
(1.17)

Similarly, we define UQC(k,η,β) as the family of functions fA such that

( z f ( z ) ) g ( z ) Q k , η (z)for some g(z)k-UCV(β)(0β<1).
(1.18)

We note that UCC(0,η,β) is the class of close to convex univalent functions of order η and type β and UQC(0,η,β) is the class of quasi-convex univalent functions of order η and type β. For fA given by (1.11) and g(z) given by g(z)=z+ n = 1 b n + 1 z n + 1 , the Hadamard product (or convolution) of f(z) and g(z) is given by

(fg)(z)=z+ n = 1 a n + 1 b n + 1 z n + 1 =(gf)(z)(zU).

Note that fgA. For α j C (j=1,2,,q) and β j C Z 0 (j=1,2,,s), the generalized hypergeometric function F s q ( α 1 , α 2 ,, α q ; β 1 , β 2 ,, β s ;z) is defined by the following infinite series (see the work of [25] and [26] for details):

F s q ( α 1 , α 2 ,, α q ; β 1 , β 2 ,, β s ;z)= n = 0 ( α 1 ) n ( α q ) n z n ( β 1 ) n ( β s ) n n !

(qs+1; q,s N 0 =N{0}). Dziok and Srivastava [27] (also see [28]) considered the linear operator

H( α 1 , α 2 ,, α q ; β 1 , β 2 ,, β s ):AA

defined by the Hadamard product

H( α 1 , α 2 ,, α q ; β 1 , β 2 ,, β s )f(z)= z q F s ( α 1 , α 2 ,, α q ; β 1 , β 2 ,, β s ;z)f(z)
(1.19)

(qs+1; q,s N 0 =N{0}, zU). If fA is given by (1.11), then we have

H( α 1 , α 2 ,, α q ; β 1 , β 2 ,, β s )f(z)=z+ n = 1 ( α 1 ) n ( α q ) n ( β 1 ) n ( β s ) n 1 n ! a n + 1 z n + 1 (zU).

Now, by using the above idea of Dziok and Srivastava [27], Deniz [2] introduced the B κ c -operator as follows:

B κ c f(z)= φ κ , c f(z)=z+ n = 1 ( c ) n a n + 1 z n + 1 4 n ( κ ) n n ! .
(1.20)

It easy to verify from the definition (1.20) that

z [ B κ + 1 c f ( z ) ] =κ B κ c f(z)(κ1) B κ + 1 c f(z),
(1.21)

where κ=u+ b + 1 2 Z 0 . In fact, the function B κ c given by (1.20) is an elementary transformation of the generalized hypergeometric function. That is, it is easy to see that B κ c f(z)= z 0 F 1 (κ; c 4 z)f(z) and also φ κ , c ( c 4 z)= z 0 F 1 (κ;z). In special cases of the B κ c -operator we obtain the following operators related to the Bessel function:

  1. (1)

    Choosing b=c=1 in (1.20) or (1.21), we obtain the operator J u :AA related with Bessel function, defined by

    J u f ( z ) = φ u , 1 , 1 ( z ) f ( z ) = [ 2 u Γ ( u + 1 ) z 1 u 2 J u ( z ) ] f ( z ) = z + n = 1 ( 1 ) n a n + 1 z n + 1 4 n ( u + 1 ) n n !
    (1.22)

and its recursive relation

z [ J u + 1 f ( z ) ] =(u+1) J u f(z)u J u + 1 f(z).
  1. (2)

    Choosing b=1 and c=1 in (1.20) or (1.21), we obtain the operator I u :AA related with the modified Bessel function, defined by

    I u f ( z ) = φ u , 1 , 1 ( z ) f ( z ) = [ 2 u Γ ( u + 1 ) z 1 u 2 I u ( z ) ] f ( z ) = z + n = 1 a n + 1 z n + 1 4 n ( u + 1 ) n n !
    (1.23)

and its recursive relation

z [ I u + 1 f ( z ) ] =(u+1) I u f(z)u I u + 1 f(z).
  1. (3)

    Choosing b=2 and c=1 in (1.20) or (1.21), we obtain the operator S u :AA related with the spherical Bessel function, defined by

    S u f(z)= [ π 1 2 2 u + 1 2 Γ ( u + 3 2 ) z 1 u 2 J u ( z ) ] f(z)=z+ n = 1 ( 1 ) n a n + 1 z n + 1 4 n ( u + 3 2 ) n n !
    (1.24)

and its recursive relation

z [ S u + 1 f ( z ) ] = ( u + 3 2 ) S u f(z) ( u + 1 2 ) S u + 1 f(z).

Finally we recall the generalized Bernardi-Libera-Livingston integral operator, which is defined by

L γ (f)= L γ ( f ( z ) ) = γ + 1 z γ 0 z t γ 1 f(t)dt,γ>1.

2 Preliminaries

In proving our main results, we need the following lemmas.

Lemma 2.1 [29]

Let h be convex univalent in U with h(0)=1 and (νh(z)+μ)>0 (ν,μC). If p is analytic in U with p(0)=1 then

p(z)+ z p ( z ) ν p ( z ) + μ h(z)(zU)p(z)h(z)(zU).
(2.1)

Lemma 2.2 [30]

Let h be convex in the open unit disk U and let E0. Suppose B(z) (zU) is analytic in U with (B(z))>0. If g(z) is analytic in U and h(0)=g(0). Then

E z 2 g (z)+B(z)g(z)h(z)g(z)h(z).
(2.2)

3 Main results

We study certain inclusion relationships for some subclasses of k-starlike functions, k-uniformly convex functions, and quasi-convex functions involving the Bessel equation. We reiterate that these classes of k-starlike functions and k-uniformly convex functions are related to domains bounded by conical sections.

Theorem 3.1 Let c1, and h be convex univalent in U with h(0)=1 and (h(z))>0. If a function fA satisfies the condition

1 1 η [ z ( B κ c f ( z ) ) B κ c f ( z ) η ] h(z)(0η<1;zU),
(3.1)

then

1 1 η [ z ( B κ + 1 c f ( z ) ) B κ + 1 c f ( z ) η ] h(z)(0η<1;zU).
(3.2)

Proof Let

p(z)= 1 1 η [ z ( B κ + 1 c f ( z ) ) B κ + 1 c f ( z ) η ] (zU),
(3.3)

where p is an analytic function in U with p(0)=1. By using (1.21), we get

(1η)p(z)+η=κ z B κ c f ( z ) B κ + 1 c f ( z ) (κ1).

Differentiating logarithmically with respect to z and multiplying by z, we obtain

p(z)+ z p ( z ) ( 1 η ) p ( z ) + η + κ 1 = 1 1 η [ z B κ c f ( z ) B κ + 1 c f ( z ) η ] .

The proof of the theorem follows now by an application of Lemma 2.1. □

Theorem 3.2 Let fA. If B κ c f(z)k-ST(η), then B κ + 1 c f(z)k-ST(η).

Proof Let

s(z)= z ( B κ + 1 c f ( z ) ) B κ + 1 c f ( z ) .

From (1.21), we can write

κ B κ c f ( z ) B κ + 1 c f ( z ) =s(z)+κ1.

Taking logarithmic differentiation and multiplying by z, we get

z ( B κ c f ( z ) ) B κ c f ( z ) =s(z)+ z s ( z ) s ( z ) + κ 1 Q k , η (z).

Since Q k , η (z) is convex univalent in U and

( Q k , η ( z ) ) > k + η k + 1 ,

the proof of the theorem follows by Theorem 3.1 and condition (1.14). □

Theorem 3.3 Let fA. If B κ c f(z)k-UCV(η), then B κ + 1 c f(z)k-UCV(η).

Proof By virtue of (1.12), (1.13), and Theorem 3.2, we obtain

B κ c f ( z ) k - UCV ( η ) z ( B κ c f ( z ) ) k - ST ( η ) B κ c z f ( z ) k - ST ( η ) B κ + 1 c z f ( z ) k - ST ( η ) B κ + 1 c f ( z ) k - UCV ( η )

and hence the proof is complete. □

Theorem 3.4 Let fA. If B κ c f(z)UCC(k,η,β), then B κ + 1 c f(z)UCC(k,η,β).

Proof Since

B κ c f ( z ) UCC ( k , η , β ) , z ( B κ c f ( z ) ) k ( z ) Q k , η ( z ) for some  k ( z ) k - ST ( β ) .

For g(z) such that B κ c g(z)=k(z) we have

z ( B κ c f ( z ) ) B κ c g ( z ) Q k , η (z).
(3.4)

Letting

h(z)= z ( B κ + 1 c f ( z ) ) B κ + 1 c g ( z ) andH(z)= z ( B κ + 1 c g ( z ) ) B κ + 1 c g ( z ) .

We observe that h(z) and H(z) are analytic in U and h(0)=H(0)=1.

Now, by Theorem 3.2,

B κ + 1 c g(z)k-ST(β)and ( H ( z ) ) > k + β k + 1 .

Also note that

z ( B κ + 1 c f ( z ) ) = ( B κ + 1 c g ( z ) ) h(z).
(3.5)

Differentiating both sides of (3.5), we obtain

z ( z ( B κ + 1 c f ( z ) ) ) B κ + 1 c g ( z ) =z ( B κ + 1 c g ( z ) ) B κ + 1 c g ( z ) h(z)+z h (z)=H(z)h(z)+z h (z).
(3.6)

Now using the identity (1.21), we obtain

z ( B κ c f ( z ) ) B κ c g ( z ) = B κ c ( z f ( z ) ) B κ c g ( z ) = z ( B κ + 1 c z f ( z ) ) + ( κ 1 ) B κ + 1 c ( z f ( z ) ) z ( B κ + 1 c g ( z ) ) + ( κ 1 ) B κ + 1 c g ( z ) = z ( B κ + 1 c z f ( z ) ) B κ + 1 c g ( z ) + ( κ 1 ) B κ + 1 c ( z f ( z ) ) B κ + 1 c g ( z ) z ( B κ + 1 c g ( z ) ) B κ + 1 c g ( z ) + κ 1 = h ( z ) + z h ( z ) H ( z ) + κ 1 .
(3.7)

From (3.4), (3.6), and the above equation, we conclude that

h(z)+ z h ( z ) H ( z ) + κ 1 Q k , η (z).

On letting E=0 and B(z)= 1 H ( z ) + κ 1 , we obtain

( B ( z ) ) = ( H ( z ) + κ 1 ) | H ( z ) + κ 1 | 2 >0

and the above inequality satisfies the conditions required by Lemma 2.2. Hence

h(z) Q k , η (z)

and so the proof is complete. □

Using a similar argument to Theorem 3.4, we can prove the following theorem.

Theorem 3.5 Let fA. If B κ c f(z)UQC(k,η,β), then B κ + 1 c f(z)UQC(k,η,β).

Now we examine the closure properties of the integral operator L γ .

Theorem 3.6 Let γ> k + η k + 1 . If B κ c k-ST(η) so is L γ ( B κ c ).

Proof From the definition of L γ (f) and the linearity of the operator B κ c we have

z ( B κ c L γ ( f ) ) =(γ+1) B κ c f(z)γ B κ c L γ (f).
(3.8)

Substituting z ( B κ c L γ ( f ( z ) ) ) B κ c v L γ ( f ( z ) ) =p(z) in (3.8) we may write

p(z)=(γ+1) B κ c f ( z ) B κ c L γ ( f ( z ) ) γ.
(3.9)

On differentiating (3.9) we get

z ( B κ c ( f ( z ) ) ) B κ c ( f ( z ) ) = z ( B κ c L γ f ( z ) ) B κ c L γ ( f ( z ) ) + z p ( z ) p ( z ) + γ =p(z)+ z p ( z ) p ( z ) + γ .

By Lemma 2.1, we have p(z)Q(k,η), since (Q(k,η)+γ)>0. This completes the proof of Theorem 3.6. □

By a similar argument we can prove Theorem 3.7 as below.

Theorem 3.7 Let γ> k + η k + 1 . If B κ c k-UCV(η) so is L γ ( B κ c ).

Theorem 3.8 Let γ> k + η k + 1 . If B κ c UCC(k,η,β) so is L γ ( B κ c ).

Proof By definition, there exists a function

K(z)= B κ c g(z)k-ST(η),

so that

z ( B κ c ( f ( z ) ) ) B κ c ( g ( z ) ) Q k , η (z)(zU).
(3.10)

Now from (3.8) we have

z ( B κ c f ) B κ c ( g ( z ) ) = z ( B κ c L γ ( z f ) ) + γ B κ c L γ ( z f ( z ) ) z ( B κ c L γ ( g ( z ) ) ) + γ B κ c L γ ( g ( z ) ) = z ( B κ c ( z f ( z ) ) ) B κ c L γ ( g ( z ) ) + γ B κ c ( z f ( z ) ) B κ c L γ ( g ( z ) ) z ( B κ c L γ ( g ( z ) ) ) B κ c L γ ( g ( z ) ) + γ .
(3.11)

Since B κ c gk-ST(η), by Theorem 3.6, we have L γ ( B κ c g)k-ST(η). Taking z ( B κ c L γ ( g ( z ) ) ) B κ c L γ ( g ) =H(z), we note that (H(z))> k + η k + 1 . Now for h(z)= z ( B κ c L γ ( f ( z ) ) ) B κ c L γ ( g ( z ) ) we obtain

z ( B κ c L γ ( f ( z ) ) ) =h(z) B κ c L γ ( g ( z ) ) .
(3.12)

Differentiating both sides of (3.12) yields

z ( B κ c ( z L γ ( f ) ) ) B κ c L γ ( g ) = z h ( z ) + h ( z ) z ( B κ c L γ ( g ) ) B κ c L γ ( g ) = z h ( z ) + H ( z ) h ( z ) .
(3.13)

Therefore from (3.11) and (3.13) we obtain

z ( B κ c f ( z ) ) B κ c g = z h ( z ) + H ( z ) h ( z ) + γ h ( z ) H ( z ) + γ .
(3.14)

This in conjunction with (3.10) leads to

h(z)+ z h ( z ) H ( z ) + γ Q(k,η)(z).
(3.15)

Let us take B(z)= 1 H ( z ) + γ in (3.15) and observe that (B(z))>0 as γ> k + η k + 1 . Now for A=0 and B as described we conclude the proof since the required conditions of Lemma 2.2 are satisfied. □

A similar argument yields the following.

Theorem 3.9 Let γ> k + η k + 1 . If B κ c UQC(k,η,β) so is L γ ( B κ c ).

4 Concluding remarks

As observed earlier when B κ c was defined, all the results discussed can easily be stated for the convolution operators J u f(z), I u f(z), and S u f(z), which are defined by (1.22), (1.23), and (1.24), respectively. However, we leave those results to the interested readers.