Sommerfeld identity

Result used in the theory of propagation of waves

The Sommerfeld identity is a mathematical identity, due Arnold Sommerfeld, used in the theory of propagation of waves,

e i k R R = 0 I 0 ( λ r ) e μ | z | λ d λ μ {\displaystyle {\frac {e^{ikR}}{R}}=\int \limits _{0}^{\infty }I_{0}(\lambda r)e^{-\mu \left|z\right|}{\frac {\lambda d\lambda }{\mu }}}

where

μ = λ 2 k 2 {\displaystyle \mu ={\sqrt {\lambda ^{2}-k^{2}}}}

is to be taken with positive real part, to ensure the convergence of the integral and its vanishing in the limit z ± {\displaystyle z\rightarrow \pm \infty } and

R 2 = r 2 + z 2 {\displaystyle R^{2}=r^{2}+z^{2}} .

Here, R {\displaystyle R} is the distance from the origin while r {\displaystyle r} is the distance from the central axis of a cylinder as in the ( r , ϕ , z ) {\displaystyle (r,\phi ,z)} cylindrical coordinate system. Here the notation for Bessel functions follows the German convention, to be consistent with the original notation used by Sommerfeld. The function I 0 ( z ) {\displaystyle I_{0}(z)} is the zeroth-order Bessel function of the first kind, better known by the notation I 0 ( z ) = J 0 ( i z ) {\displaystyle I_{0}(z)=J_{0}(iz)} in English literature. This identity is known as the Sommerfeld identity.[1]

In alternative notation, the Sommerfeld identity can be more easily seen as an expansion of a spherical wave in terms of cylindrically-symmetric waves:[2]

e i k 0 r r = i 0 d k ρ k ρ k z J 0 ( k ρ ρ ) e i k z | z | {\displaystyle {\frac {e^{ik_{0}r}}{r}}=i\int \limits _{0}^{\infty }{dk_{\rho }{\frac {k_{\rho }}{k_{z}}}J_{0}(k_{\rho }\rho )e^{ik_{z}\left|z\right|}}}

Where

k z = ( k 0 2 k ρ 2 ) 1 / 2 {\displaystyle k_{z}=(k_{0}^{2}-k_{\rho }^{2})^{1/2}}

The notation used here is different form that above: r {\displaystyle r} is now the distance from the origin and ρ {\displaystyle \rho } is the radial distance in a cylindrical coordinate system defined as ( ρ , ϕ , z ) {\displaystyle (\rho ,\phi ,z)} . The physical interpretation is that a spherical wave can be expanded into a summation of cylindrical waves in ρ {\displaystyle \rho } direction, multiplied by a two-sided plane wave in the z {\displaystyle z} direction; see the Jacobi-Anger expansion. The summation has to be taken over all the wavenumbers k ρ {\displaystyle k_{\rho }} .

The Sommerfeld identity is closely related to the two-dimensional Fourier transform with cylindrical symmetry, i.e., the Hankel transform. It is found by transforming the spherical wave along the in-plane coordinates ( x {\displaystyle x} , y {\displaystyle y} , or ρ {\displaystyle \rho } , ϕ {\displaystyle \phi } ) but not transforming along the height coordinate z {\displaystyle z} . [3]

Notes

  1. ^ Sommerfeld 1964, p. 242.
  2. ^ Chew 1990, p. 66.
  3. ^ Chew 1990, p. 65-66.

References

  • Sommerfeld, Arnold (1964). Partial Differential Equations in Physics. New York: Academic Press. ISBN 9780126546583.
  • Chew, Weng Cho (1990). Waves and Fields in Inhomogeneous Media. New York: Van Nostrand Reinhold. ISBN 9780780347496.
  • v
  • t
  • e