Stable Operation of a Free-Electron Laser Driven by a Plasma Accelerator

  • M. Galletti*
  • , D. Alesini
  • , M. P. Anania
  • , S. Arjmand
  • , M. Behtouei
  • , M. Bellaveglia
  • , A. Biagioni
  • , B. Buonomo
  • , F. Cardelli
  • , M. Carpanese
  • , E. Chiadroni
  • , A. Cianchi
  • , G. Costa
  • , A. Del Dotto
  • , M. Del Giorno
  • , F. Dipace
  • , A. Doria
  • , F. Filippi
  • , G. Franzini
  • , L. Giannessi
  • A. Giribono, P. Iovine, V. Lollo, A. Mostacci, F. Nguyen, M. Opromolla, L. Pellegrino, A. Petralia, V. Petrillo, L. Piersanti, G. Di Pirro, R. Pompili, S. Romeo, A. R. Rossi, A. Selce, V. Shpakov, A. Stella, C. Vaccarezza, F. Villa, A. Zigler, M. Ferrario
*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

25 Scopus citations

Abstract

The breakthrough provided by plasma-based accelerators enabled unprecedented accelerating fields by boosting electron beams to gigaelectronvolt energies within a few centimeters [1-4]. This, in turn, allows the realization of ultracompact light sources based on free-electron lasers (FELs) [5], as demonstrated by two pioneering experiments that reported the observation of self-amplified spontaneous emission (SASE) driven by plasma-accelerated beams [6,7]. However, the lack of stability and reproducibility due to the intrinsic nature of the SASE process (whose amplification starts from the shot noise of the electron beam) may hinder their effective implementation for user purposes. Here, we report a proof-of-principle experiment using plasma-accelerated beams to generate stable and reproducible FEL light seeded by an external laser. FEL radiation is emitted in the infrared range, showing the typical exponential growth of its energy over six consecutive undulators. Compared to SASE, the seeded FEL pulses have energies 2 orders of magnitude larger and stability that is 3 times higher.

Original languageEnglish
Article number234801
JournalPhysical Review Letters
Volume129
Issue number23
DOIs
StatePublished - 2 Dec 2022

Bibliographical note

Publisher Copyright:
© 2022 American Physical Society.

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