• Open Access

Ka-band linearizer structure studies for a compact light source

A. Castilla, R. Apsimon, G. Burt, X. Wu, A. Latina, X. Liu, I. Syratchev, W. Wuensch, B. Spataro, and A. W. Cross
Phys. Rev. Accel. Beams 25, 112001 – Published 9 November 2022

Abstract

The CompactLight design for a next-generation x-ray free-electron laser utilizes a C-band injector. This requires that the harmonic system used to linearize the beam’s phase space must operate at X-band rf or higher. We investigate the optimum frequency for the harmonic system in the range of frequencies from 12 to 48 GHz. We describe the reasoning behind selecting 36 GHz (Ka-band) as our working harmonic frequency. The full linearizer system design including the power source, pulse compressor, and linearizing structure, along with options, is considered and presented. These designs are compared in terms of rf and beam dynamics performance. Two potential MW-level rf sources are discussed; a multibeam klystron and a gyro-klystron, while a klystron-based upconverter with an X-band driver is briefly discussed as an alternative path if even higher peak powers are needed. To further increase peak power, novel options for pulse compressors at Ka-band are discussed. Traveling and standing wave solutions for the structure are presented.

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  • Received 29 April 2022
  • Accepted 31 October 2022

DOI:https://doi.org/10.1103/PhysRevAccelBeams.25.112001

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Accelerators & Beams

Authors & Affiliations

A. Castilla*, R. Apsimon, and G. Burt

  • Engineering Department, Lancaster University, Lancaster LA1 4YW, United Kingdom
  • Cockcroft Institute, Daresbury Laboratory, Warrington WA4 4AD, United Kingdom

X. Wu, A. Latina, X. Liu, I. Syratchev, and W. Wuensch

  • CERN, CH-1211 Geneva, Switzerland

B. Spataro

  • INFN-LNF, Via Enrico Fermi 40, 00044 Frascati, Rome, Italy

A. W. Cross

  • Strathclyde University, Glasgow G4 0NG, United Kingdom

  • *Also at CERN
  • g.burt@lancs.ac.uk

Article Text

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Issue

Vol. 25, Iss. 11 — November 2022

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