Four-frequency

The four-frequency of a massless particle, such as a photon, is a four-vector defined by

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

where ν {\displaystyle \nu } is the photon's frequency and n ^ {\displaystyle {\hat {\mathbf {n} }}} is a unit vector in the direction of the photon's motion. The four-frequency of a photon is always a future-pointing and null vector. An observer moving with four-velocity V b {\displaystyle V^{b}} will observe a frequency

1 c η ( N a , V b ) = 1 c η a b N a V b {\displaystyle {\frac {1}{c}}\eta \left(N^{a},V^{b}\right)={\frac {1}{c}}\eta _{ab}N^{a}V^{b}}

Where η {\displaystyle \eta } is the Minkowski inner-product (+−−−) with covariant components η a b {\displaystyle \eta _{ab}} .

Closely related to the four-frequency is the four-wavevector defined by

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

where ω = 2 π ν {\displaystyle \omega =2\pi \nu } , c {\displaystyle c} is the speed of light and k = 2 π λ n ^ {\textstyle \mathbf {k} ={\frac {2\pi }{\lambda }}{\hat {\mathbf {n} }}} and λ {\displaystyle \lambda } is the wavelength of the photon. The four-wavevector is more often used in practice than the four-frequency, but the two vectors are related (using c = ν λ {\displaystyle c=\nu \lambda } ) by

K a = 2 π c N a {\displaystyle K^{a}={\frac {2\pi }{c}}N^{a}}

See also

  • Four-vector
  • Wave vector

References

  • Woodhouse, N.M.J. (2003). Special Relativity. London: Springer-Verlag. ISBN 1-85233-426-6.


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