Four-frequency

From Wikipedia, the free encyclopedia

The four-frequency of a photon is defined by

N^a = \left( \nu, \nu \mathbf{n} \right)

where ν is the photon's frequency and \mathbf{n} is a unit vector in the direction of the photon's motion. The four-frequency is always a null vector. Closely related to the four-frequency is the wave four-vector defined by

K^a=\left(\frac{\omega}{c}, \mathbf{k}\right)

where ω = 2πν, c is the speed of light and \mathbf{k}=\frac{2 \pi}{\lambda}\mathbf{n} and λ is the wavelength of the photon. The wave four-vector is more often used in practice than the four-frequency, but the two vectors are related (using c = νλ) by

K^a=\frac{2 \pi}{c}N^a
This relativity-related article is a stub. You can help Wikipedia by expanding it.