Radiative Losses in Plasma Accelerators
arXiv:0705.4521 · doi:10.1134/S1063776106110173
Abstract
We investigate the dynamics of a relativistic electron in a strongly nonlinear plasma wave in terms of classical mechanics by taking into account the action of the radiative reaction force. The two limiting cases are considered. In the first case where the energy of the accelerated electrons is low, the electron makes many betatron oscillations during the acceleration. In the second case where the energy of the accelerated electrons is high, the betatron oscillation period is longer than the electron residence time in the accelerating phase. We show that the force of radiative friction can severely limit the rate of electron acceleration in a plasma accelerator.
17 pages, 5 figures
Cited by in corpus (4)
- Radiation Emission by Extreme Relativistic Electrons and Pair Production by Hard Photons in a Strong Plasma Wakefield
- On radiative damping in plasma-based accelerators
- Radiation reaction-dominated regime of wakefield acceleration
- Modeling of three-dimensional betatron oscillation and radiation reaction in plasma accelerators