Microbunching Instability Based Synchrotron Radiation Sources

TL;DR

This paper proposes a novel magnetic device using permanent magnets to amplify microbunching at EUX and XUV wavelengths, enabling high-power, ultra-short radiation pulses with moderate beam parameters.

Contribution

Introduction of a new magnetic device design that amplifies microbunching in the EUX and XUV range using permanent magnets and specific focusing and dispersive elements.

Findings

Simulations show effective microbunching amplification at targeted wavelengths.

Device can produce high-power, ultra-short radiation pulses.

Performance demonstrated across different beam energies.

Abstract

Although microbunching-instability (MBI) based synchrotron-radiation facilities do not exist yet, the prominent presence of this space-charge driven instability in the high-brightness accelerator facilities promotes the ongoing worldwide effort to mastering it. Thereby not only the possible countermeasures but also the applications of MBI are in focus of the research. So far, the observed microbunching wavelengths are in IR or optical regime. Shifting the microbunching towards shorter wavelengths seems to require either very high-bunch peak currents or extremely small emittances. These extreme characteristics are difficult to generate and hard to preserve. This letter proposes a novel magnetic device which allows to amplify the initial shot noise at wavelengths in EUX and XUV range with moderate peak current and emittance. It consists of permanent magnets. The specific combination of focusing channels, dispersive chicanes and single focusing elements in this device allows for optimal amplification of microbunching by the longitudinal-space charge-impedance. Extensive simulation studies for different beam energies show the performance of the proposed device, which fed for example with an energy recovery linac can provide ultra-short coherent-high power-radiation pulses with a high repetition rate.