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It is easy to notice that

k

n

(

|

t

|

, y

)

and

l

n

(

|

t

|

, y

)

are infinitely differentiable

and rapidly decreasing functions

t

R

n

, i.e. they belong to the space

S

(

R

n

)

[7]. These functions are also spherically symmetric, so while

calculating the inverse Fourier transform it is possible to pass to the

spherical coordinates in the space

R

n

. Let us denote

|

x

|

=

r

,

|

t

|

=

ρ, σ

n

1

as an area of the unit sphere in the space

R

n

.

For any spherically symmetric

function

h

n

(

|

t

|

) =

h

n

(

ρ

)

∈ S

(

R

n

)

we have

H

n

(

|

x

|

) =

H

n

(

r

) =

F

1

t

[

h

n

] (

x

) =

1

(2

π

)

n

Z

R

n

h

n

(

|

t

|

)

e

i

h

x,t

i

dt

=

=

σ

n

1

(2

π

)

n

Z

0

h

n

(

ρ

)

ρ

n

2

π

Z

0

e

irρ

cos

θ

sin

n

2

θdθ

=

=

1

(2

π

)

n

2

r

n

2

1

Z

0

h

n

(

ρ

)

ρ

n

2

J

n

2

1

(

)

dρ,

where

J

n

2

1

(

)

is the Bessel function of the first kind of order

ν

=

n/

2

1

[7, 8]. The above formula is valid and it is easy to be checked.

By differentiating the above equation and by considering the formula

of the theory of Bessel functions [4]

νJ

ν

(

)

J

0

ν

(

) =

J

ν

+1

(

)

,

we obtain the recurrence formula

H

n

+2

(

r

) =

1

2

πr

∂r

H

n

(

r

)

.

For this formula it is necessary to know the kernels

K

n

(

x, y

)

and

L

n

(

x, y

)

only for

n

= 1

and

n

= 2

.

Since the Fourier transform moves the space

S

(

R

n

)

into itself,

the kernels

K

n

(

x, y

) =

K

n

(

|

x

|

, y

)

and

L

n

(

x, y

) =

L

n

(

|

x

|

, y

)

when

y

(0

, a

)

, are spherically symmetric functions of

x

in the space

S

(

R

n

)

.

Therefore, the convolution (1) exists for any tempered distribution

ϕ

(

x

)

∈ S

0

(

R

n

)

,

ψ

(

x

)

∈ S

0

(

R

n

)

, and can be written as

ϕ

(

x

)

K

n

(

x, y

) +

ψ

(

x

)

L

n

(

x, y

) =

= (

ϕ

(

t

)

, K

n

(

x

t, y

)) + (

ψ

(

t

)

, L

n

(

x

t, y

))

.

When

ϕ

(

x

)

and

ψ

(

x

)

are normal functions of polynomial growth,

convolution (1) can be written as a sum of integrals

Z

R

n

ϕ

(

t

)

K

n

(

x

t, y

)

dt

+

Z

R

n

ψ

(

t

)

L

n

(

x

t, y

)

dt .

6

ISSN 1812-3368. Herald of the BMSTU. Series “Natural Sciences”. 2015. No. 1