• Open Access

Development of a prototype superconducting radio-frequency cavity for conduction-cooled accelerators

G. Ciovati, J. Anderson, S. Balachandran, G. Cheng, B. Coriton, E. Daly, P. Dhakal, A. Gurevich, F. Hannon, K. Harding, L. Holland, F. Marhauser, K. McLaughlin, D. Packard, T. Powers, U. Pudasaini, J. Rathke, R. Rimmer, T. Schultheiss, H. Vennekate, and D. Vollmer
Phys. Rev. Accel. Beams 26, 044701 – Published 17 April 2023

Abstract

The higher efficiency of superconducting radio-frequency (SRF) cavities compared to normal-conducting ones enables the development of high-energy continuous-wave linear accelerators (linacs). Recent progress in the development of high-quality Nb3Sn film coatings along with the availability of cryocoolers with high cooling capacity at 4 K makes it feasible to operate SRF cavities cooled by thermal conduction at relevant accelerating gradients for use in accelerators. A possible use of conduction-cooled SRF linacs is for environmental applications, requiring electron beams with energy of 1–10 MeV and 1 MW of power. We have designed a 915 MHz SRF linac for such an application and developed a prototype single-cell cavity to prove the proposed design by operating it with cryocoolers at the accelerating gradient required for 1 MeV energy gain. The cavity has a 3μm thick Nb3Sn film on the inner surface, deposited on a 4mm thick bulk Nb substrate and a bulk 7mm thick Cu outer shell with three Cu attachment tabs. The cavity was tested up to a peak surface magnetic field of 53 mT in liquid He at 4.3 K. A horizontal test cryostat was designed and built to test the cavity cooled with three Gifford-McMahon cryocoolers. The rf tests of the conduction-cooled cavity, performed at General Atomics, achieved a peak surface magnetic field of 50 mT and stable operation was possible with up to 18.5 W of rf heat load. The peak frequency shift due to microphonics was 23 Hz. These results represent the highest peak surface magnetic field achieved in a conduction-cooled SRF cavity to date and meet the requirements for a 1 MeV energy gain.

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  • Received 7 February 2023
  • Accepted 28 March 2023

DOI:https://doi.org/10.1103/PhysRevAccelBeams.26.044701

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

G. Ciovati1,2,*, J. Anderson3, S. Balachandran1, G. Cheng1, B. Coriton3,†, E. Daly1, P. Dhakal1, A. Gurevich2, F. Hannon1,‡, K. Harding1, L. Holland3, F. Marhauser1,§, K. McLaughlin3, D. Packard3, T. Powers1, U. Pudasaini1, J. Rathke4, R. Rimmer1, T. Schultheiss5, H. Vennekate1, and D. Vollmer3

  • 1Thomas Jefferson National Accelerator Facility, Newport News, Virginia 23606, USA
  • 2Center for Accelerator Science, Department of Physics, Old Dominion University, Norfolk, Virginia 23529, USA
  • 3General Atomics, San Diego, California 92121, USA
  • 4TECHSOURCE, Inc., Los Alamos, New Mexico 87544, USA
  • 5TJS Technologies LLC, Commack, New York 11725, USA

  • *gciovati@jlab.org
  • Present address: ITER, 13067 Saint Paul-lez-Durance, France.
  • Present address: Phasespace Tech, 23734 Bjärred, Sweden.
  • §Present address: SCK CEN, 2400 Mol, Belgium.

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Vol. 26, Iss. 4 — April 2023

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