## Wavenumber | <<< | >>> |

Definition: the phase delay per unit length, or that quantity divided by 2π

German: Wellenzahl

Formula symbol: *k*, ν

Units: 1/m, 1/cm

Unfortunately, there are different definitions of the *wavenumber* of light in the literature.
In physics, the definition

is common, where λ is the wavelength in the medium (not the vacuum wavelength). That wavenumber is the magnitude of the wave vector, and is the phase delay per unit length during propagation of a plane wave.

The other definition

(with units of cm^{−1}) is widely used in the field of spectroscopy and therefore called the *spectroscopic wavenumber*.
The former quantity can be called *angular wavenumber* (in analogy with *angular frequency*) to avoid confusion, but that term is not very common.

For light in a medium, the wavenumber is the vacuum wavenumber times the refractive index. Spectroscopic wavenumbers are usually considered in vacuum.

The wavenumber is related to the phase change per unit length of a plane wave in a homogeneous medium. For focused beams, the phase change per unit length is modified with respect to that for a plane wave. For Gaussian beams, for example, this modification is the Gouy phase shift. For propagation of guided waves in waveguides, the imaginary part of the propagation constant γ (called β) is the relevant quantity.

See also: wave vector, propagation constant, refractive index

and other articles in the category general optics

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