For a particle of rest mass and velocity , the relativistic energy and momentum are
For a photon of wavelength travelling along ,
Here is Planck constant and is the speed of light.
Let and be the incident and scattered photon energies. The stationary electron initially has energy . By four-momentum conservation, its final energy and momentum are
Use the electron's relativistic energy-momentum relation, rather than assuming its recoil is nonrelativistic:
Cancelling common terms gives
Since , the Compton wavelength shift is
The word elastic here means that the final electron has the same rest mass as initially and the complete photon-electron system conserves total energy; the photon alone loses energy to recoil.
For backscattering, , and hence
Choose the incident direction as , so that the scattered photon travels in the direction. An observer moving with velocity meets that photon head-on. The Lorentz transformation of four-momentum gives the observed energy
This is the approaching-observer relativistic Doppler effect. Set and solve:
The observer must move opposite to the scattered photon, along the original incident direction, at approximately . Moving with the scattered photon would redshift it instead.

Articles by others on the same topic (0)

There are currently no matching articles.