Smith–Purcell effect
The Smith–Purcell effect was the precursor of the free-electron laser. It was studied by Steve Smith, a graduate student under the guidance of Edward Purcell. In their experiment, they sent an energetic beam of electrons very closely parallel to the surface of a ruled optical diffraction grating, and thereby generated visible light. Smith showed there was negligible effect on the trajectory of the inducing electrons. Essentially, this is a form of Cherenkov radiation where the phase velocity of the light has been altered by the periodic grating. However, unlike Cherenkov radiation, there is no minimum or threshold particle velocity.
Smith–Purcell radiation is particularly attractive for applications involving non-destructive beam diagnostics and especially as a viable THz radiation source, which has further broad-range uses in diverse and high-impact fields like materials sciences, biotechnology, security and communications, manufacturing and medicine. Operating at THz frequencies also allows for potentially large accelerating gradients to be realised. This, paired with plasma-wakefield acceleration methods under development and linear accelerator technology, could pave the way to next-generation, compact, less prone to RF breakdown, high energy output linacs.
Background
Charged particles usually radiate/generate radiation via two different mechanisms:- Acceleration or change of direction of motion: e.g. Bremsstrahlung radiation, synchrotron radiation.
- Polarisation: A moving charge has a dynamic Coulomb field. For a conducting/polarisable material, the interaction between this field and the charges in the material/ medium could generate radiation. This includes Cherenkov and transition radiation, where the particle moves within the medium which generates the radiation, but also diffraction radiation, where particles move in the vicinity of the target material, generating for example, optical diffraction radiation and Smith–Purcell radiation.
Dispersion relation
When a charged particle travels above a periodic grating, a current is induced on the surface of the grating. This induced current then emits radiation at the discontinuities of the grating due to the scattering of the Coulomb field of the induced charges at the grating boundaries. The dispersion relation for the Smith–Purcell effect is given as follows:where the wavelength is observed at an angle to the direction of the electron beam for the order reflection mode, and is the grating period and is the relative electron velocity. This relation can be derived through considering energy and momentum conservation laws.