The function is defined through the equation
|
(1)
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where is a Bessel
function of the first kind, so
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(2)
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where is the real
part.
The function is implemented in the Wolfram Language as KelvinBer[nu, z].
The function has the series expansion
|
(3)
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where is the gamma
function (Abramowitz and Stegun 1972, p. 379), which can be written in closed
form as
|
(4)
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where is a modified
Bessel function of the first kind.
The special case ,
commonly denoted
,
corresponds to
|
(5)
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where is the zeroth order Bessel
function of the first kind. The function
has the series expansion
|
(6)
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which can be written in closed form as
|
(7)
| |||
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(8)
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