Kelvin Functions

Kelvin defined the Kelvin functions bei and ber according to

ber_nu(x)+ibei_nu(x)=J_nu(xe^(3pii/4))
(1)
=e^(nupii)J_nu(xe^(-pii/4)),
(2)
=e^(nupii/2)I_nu(xe^(pii/4))
(3)
=e^(3nupii/2)I_nu(xe^(-3pii/4)),
(4)

where J_nu(x) is a Bessel function of the first kind and I_nu(x) is a modified Bessel function of the first kind. These functions satisfy the Kelvin differential equation.

Similarly, the functions kei and ker by

 ker_nu(x)+ikei_nu(x)=e^(-nupii/2)K_nu(xe^(pii/4)),
(5)

where K_nu(x) is a modified Bessel function of the second kind. For the special case nu=0,

J_0(isqrt(i)x)=J_0(1/2sqrt(2)(i-1)x)
(6)
=ber(x)+ibei(x).
(7)

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