• Open Access

High field Q slope and the baking effect: Review of recent experimental results and new data on Nb heat treatments

G. Ciovati, G. Myneni, F. Stevie, P. Maheshwari, and D. Griffis
Phys. Rev. ST Accel. Beams 13, 022002 – Published 22 February 2010

Abstract

The performance of superconducting radio-frequency (SRF) cavities made of bulk Nb at high fields (peak surface magnetic field greater than about 90 mT) is characterized by exponentially increasing rf losses (high-field Q slope), in the absence of field emission, which are often mitigated by low-temperature (100140°C, 12–48 h) baking. In this contribution, recent experimental results and phenomenological models to explain this effect will be briefly reviewed. New experimental results on the high-field Q slope will be presented for cavities that had been heat treated in a vacuum furnace at high temperature without subsequent chemical etching. These studies are aimed at understanding the role of hydrogen on the high-field Q slope and at the passivation of the Nb surface during heat treatment. Improvement of the cavity performances, particularly of the cavities’ quality factor, have been obtained following the high-temperature heat treatments, while secondary ion mass spectroscopy surface analysis measurements on Nb samples treated with the cavities revealed significantly lower hydrogen concentration than for samples that followed standard cavity treatments.

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  • Received 25 November 2009

DOI:https://doi.org/10.1103/PhysRevSTAB.13.022002

This article is available under the terms of the Creative Commons Attribution 3.0 License. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI.

Authors & Affiliations

G. Ciovati1,*, G. Myneni1, F. Stevie2, P. Maheshwari2, and D. Griffis2

  • 1Thomas Jefferson National Accelerator Facility, Newport News, Virginia 23606, USA
  • 2North Carolina State University, Raleigh, North Carolina 27695, USA

  • *gciovati@jlab.org

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Vol. 13, Iss. 2 — February 2010

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