• Open Access

High gradient experiments with X-band cryogenic copper accelerating cavities

A. D. Cahill, J. B. Rosenzweig, V. A. Dolgashev, S. G. Tantawi, and S. Weathersby
Phys. Rev. Accel. Beams 21, 102002 – Published 23 October 2018

Abstract

Vacuum radio-frequency (rf) breakdown is one of the major factors that limit operating accelerating gradients in rf particle accelerators. The occurrence of rf breakdowns was shown to be probabilistic, and can be characterized by a breakdown rate. Experiments with hard copper cavities showed that harder materials can reach larger accelerating gradients for the same breakdown rate. We study the effect of cavity material on rf breakdowns with short X-band standing wave accelerating structures. Here we report results from tests of a structure at cryogenic temperatures. At gradients greater than 150MV/m we observed a degradation in the intrinsic cavity quality factor, Q0. This decrease in Q0 is consistent with rf power being absorbed by field emission currents, and is accounted for in the determination of accelerating gradients. The structure was conditioned up to an accelerating gradient of 250MV/m at 45 K with 108 rf pulses and a breakdown rate of 2×104/pulse/m. For this breakdown rate, the cryogenic structure has the largest reported accelerating gradient. This improved performance over room temperatures structures supports the hypothesis that breakdown rate can be reduced by immobilizing crystal defects and decreasing thermally induced stresses.

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  • Received 14 December 2017

DOI:https://doi.org/10.1103/PhysRevAccelBeams.21.102002

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)

  1. Research Areas
Accelerators & Beams

Authors & Affiliations

A. D. Cahill* and J. B. Rosenzweig

  • UCLA Los Angeles, California 90095, USA

V. A. Dolgashev, S. G. Tantawi, and S. Weathersby

  • SLAC Menlo Park, California 94025, USA

  • *acahill@physics.ucla.edu

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Vol. 21, Iss. 10 — October 2018

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