1 Introduction

In 1903, the Swedish mathematician Mittag-Leffler [1, 2] introduced the function

E α (z)= n = 0 z n Γ ( α n + 1 ) ( α C ; Re ( α ) > 0 ) .
(1.1)

A generalization of (1.1) was given by Wiman [3] in 1905 in the form

E α , β (z)= n = 0 z n Γ ( α n + β ) ( α , β C ; Re ( α ) > 0 , Re ( β ) > 0 ) .
(1.2)

In 1971, in connection with the solution of certain singular integral equations, a further interesting and useful generalization of (1.2) was introduced by Prabhakar [4] in the form

(1.3)

where ( γ ) n is the Pochhammer symbol defined by

( γ ) 0 =1; ( γ ) n =γ(γ+1)(γ+n1)= Γ ( γ + n ) Γ ( γ ) ;γ0.
(1.4)

A generalization of (1.3) is given by Shukla and Prajapati [5] in the following form:

E α , β γ , q (z)= n = 0 ( γ ) q n z n Γ ( α n + β ) n ! ,
(1.5)

where (α,β,γC; Re(α)>0, Re(β)>0, Re(γ)>0, q(0,1)N).

The above generalization studied by Shukla and Prajapati is shown in a series of papers [58]. A generalization of Mittag-Leffler functions defined by (1.3) and (1.5) is introduced and studied by Srivastava and Tomovski [9] in the form

E α , β γ , κ (z)= n = 0 ( γ ) n κ z n Γ ( α n + β ) n ! ,
(1.6)

where α,β,γ,κC; Re(α)=Re(κ)1>0, Re(β)>0, Re(γ)>0, Re(κ)>0 and the Pochhammer symbol for λ,μC is defined by

( λ ) μ = Γ ( λ + μ ) Γ ( λ ) ={ 1 ( μ = 0 , λ C { 0 } ) ; λ ( λ + 1 ) ( λ + n 1 ) , μ = n N ; λ C .
(1.7)

The object of this paper is to derive the Laplace and Mellin transforms of the following integral operator associated with the generalized Mittag-Leffler function, defined by Shukla and Prajapati [6] as well as Srivastava and Tomovski [9], in the next sections:

( E α , β , ω ; 0 + γ , q f ) (x)= 0 x ( x t ) β 1 E α , β γ , q [ w ( x t ) α ] f(t)dt,
(1.8)

where α,β,γC; Re(α)>0, Re(β)>0, Re(γ)>0; q(0,1)N.

Shukla and Prajapati [6] have shown that the Mellin-Barnes integral for the function defined by (1.5) is given by

E α , β γ , q (z)= 1 2 π i Γ ( γ ) i i Γ ( ξ ) Γ ( γ + q ξ ) Γ ( α ξ + β ) ( z ) ξ dξ.
(1.9)

As γ0, then by virtue of the limit formula,

lim γ 0 E α , β γ (z)= 1 Γ ( β )
(1.10)

reduces to the familiar Reimann-Liouville fractional integral

( I 0 + α f ) (x)= 1 Γ ( α ) 0 x ( x t ) α 1 f(t)dt ( α C , Re ( α ) > 0 ) .
(1.11)

In the following, we will use the representation of a high transcendental function in terms of the so-called H-function defined as [10]

H p , q m , n [ z ( a 1 , A 1 ) , , ( a p , A p ) ( b 1 , B 1 ) , , ( b q , B q ) ] = 1 2 π i L θ(ξ) z ξ dξ,
(1.12)

where

θ(ξ)= [ j = 1 m Γ ( b j + B j ξ ) ] [ j = 1 n Γ ( 1 a j A j ξ ) ] [ j = m + 1 q Γ ( 1 b j B j ξ ) ] [ j = n + 1 p Γ ( a j + A j ξ ) ] ,
(1.13)

and an empty product is always interpreted as unity; m,n,p,q N 0 with 0np, 1mq, A i , B j R + , a i , b j R or ℂ (i=1,,p; j=1,,q) such that

A i ( b j +k) B j ( a i l1)(k,l N 0 ;i=1,,n;j=1,,m).
(1.14)

The contour L is the path of integration in the complex ξ-plane running from γi to γ+i for some real number γ.

2 Mellin transform of the operator (1.8)

Theorem 2.1 It is shown here that

M { ( E α , β , ω ; 0 + γ , q f ) ( x ) ; s } = 1 Γ ( γ ) Γ ( 1 s ) H 1 , 2 2 , 1 [ w t α ( 1 γ , q ) ( 0 , 1 ) , ( 1 s β , α ) ] M { t β f ( t ) ; s } ,
(2.1)

where (Re(α)>0, Re(β)>0, Re(γ)>0); q(0,1)N, Re(1sβ)>0and H 1 , 2 2 , 1 ()is the H-function defined by (1.12).

Proof

Mellin transform is defined as

M { f ( x ) ; s } = 0 x s 1 f(x)dx.

Therefore, we have

M { ( E α , β , ω ; 0 + γ , q f ) ( x ) ; s } = 0 x s 1 0 x ( x t ) β 1 E α , β γ , q [ ω ( x t ) α ] f(t)dtdx.

Interchanging the order of integration, which is permissible under the conditions given in Theorem 2.1, we find that

(2.2)

If we consider x=t+u in the r.h.s. of (2.2), we get

M { ( E α , β , ω ; 0 + γ , q f ) ( x ) ; s } = 0 f(t)dt t ( t + u ) s 1 u β 1 E α , β γ , q [ ω u α ] du.
(2.3)

To evaluate the u-integral, we express the Mittag-Leffler function in terms of its Mellin-Barnes contour integral by means of the formula (1.9), then the above expression transforms into the form

M { ( E α , β , ω ; 0 + γ , q f ) ( x ) ; s } = 0 f ( t ) d t 1 2 π i Γ ( γ ) i i Γ ( ξ ) Γ ( γ + q ξ ) Γ ( α ξ + β ) ( ω ) ξ 0 ( t + u ) s 1 u β + α ξ 1 d u d ξ .
(2.4)

If the u-integral is evaluated with the help of the formula

0 x ν 1 ( x + a ) ρ dx= Γ ( ν ) Γ ( ρ ν ) Γ ( ρ ) ;Re(ρ)>Re(ν)>0,
(2.5)

then after some simplification, it is seen that the right-hand side of above equation (2.4) simplifies to

(2.6)

which, on being interpreted by the definition of H-function (1.12), yields the desired result. □

For q=1, Theorem 2.1 reduces to the following corollary.

Corollary 2.1 The following result holds:

M { ( E α , β , ω ; 0 + γ f ) ( x ) ; s } = 1 Γ ( γ ) Γ ( 1 s ) H 1 , 2 2 , 1 [ w t α ( 1 γ , 1 ) ( 0 , 1 ) , ( 1 s β , α ) ] M { t β f ( t ) ; s } ,
(2.7)

where (Re(α)>0, Re(β)>0, Re(γ)>0); Re(1sβ)>0and H 1 , 2 2 , 1 ()is the H-function defined by (1.12).

Theorem 2.2 It is shown here that

M { ( E α , β , ω ; 0 + γ , κ f ) ( x ) ; s } = 1 Γ ( γ ) Γ ( 1 s ) H 1 , 2 2 , 1 [ w t α ( 1 γ , κ ) ( 0 , 1 ) , ( 1 s β , α ) ] M { t β f ( t ) ; s } ,
(2.8)

whereRe(α)=Re(κ)1>0, Re(β)>0, Re(γ)>0, Re(κ)>0, Re(1sβ)>0and H 1 , 2 2 , 1 ()is the H-function defined by (1.12).

3 Laplace transform of the operator (1.8)

Theorem 3.1 The following result holds:

L { ( E α , β , ω ; 0 + γ , q f ) ( x ) ; p } = 1 Γ ( γ ) p 1 β ψ 0 [ ( γ , q ) ; ω / p α ; ] F(p),
(3.1)

where (Re(α),Re(β),Re(γ)>0); Re(p)> | ω | 1 / Re ( α ) andF(p)is the Laplace transform off(t)defined by

L { f ( t ) ; p } =F(p)= 0 e p t f(t)dt,
(3.2)

whereRe(p)>0and the integral is convergent.

Proof By virtue of the definitions (1.8) and (3.2), it follows that

L { ( E α , β , ω ; 0 + γ , q f ) ( x ) ; p } = 0 e p x 0 x ( x t ) β 1 E α , β γ , q [ ω ( x t ) α ] f(t)dtdx.

Interchanging the order of integration, which is permissible under the conditions given in Theorem 3.1, we find that

L { ( E α , β , ω ; 0 + γ , q f ) ( x ) ; p } = 0 f(t)dt t e p x ( x t ) β 1 E α , β γ , q [ ω ( x t ) α ] dx.

If we consider x=t+u, we obtain

L { ( E α , β , ω ; 0 + γ , q f ) ( x ) ; p } = 0 e p t f(t)dt 0 e p u u β 1 E α , β γ , q [ ω u α ] du.

On making use of the series definition (1.5), the above expression becomes

and F(p) is the Laplace transform of f(t). □

For q=1, Theorem 3.1 reduces to the following corollary.

Corollary 3.1 The following result holds:

Ł { ( E α , β , ω ; 0 + γ f ) ( x ) ; p } = p β ( 1 a p α ) γ F(p),
(3.3)

where (Re(α)>0, Re(β)>0, Re(γ)>0); Re(p)>0and the integral operator is the one discussed by Prabhakar[4]defined by (1.10).

Theorem 3.2 The following result holds:

L { ( E α , β , ω ; 0 + γ , κ f ) ( x ) ; p } = 1 Γ ( γ ) p 1 β ψ 0 [ ( γ , κ ) ; ω / p α ; ] F(p),
(3.4)

whereRe(α)=Re(κ)1>0, Re(β)>0, Re(γ)>0, Re(κ)>0; Re(p)> | ω | 1 / Re ( α ) andF(p)is the Laplace transform off(t)defined by (3.2).