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BiBTeX citation export for MOPAB392: Alternative RF Tuning Methods Performed on Spoke Cavities for ESS and MYRRHA Projects

@inproceedings{duchesne:ipac2021-mopab392,
  author       = {P. Duchesne and S. Blivet and G. Olivier and G. Olry and T. Pépin-Donat},
  title        = {{Alternative RF Tuning Methods Performed on Spoke Cavities for ESS and MYRRHA Projects}},
  booktitle    = {Proc. IPAC'21},
  pages        = {1196--1199},
  eid          = {MOPAB392},
  language     = {english},
  keywords     = {cavity, operation, target, simulation, experiment},
  venue        = {Campinas, SP, Brazil},
  series       = {International Particle Accelerator Conference},
  number       = {12},
  publisher    = {JACoW Publishing, Geneva, Switzerland},
  month        = {08},
  year         = {2021},
  issn         = {2673-5490},
  isbn         = {978-3-95450-214-1},
  doi          = {10.18429/JACoW-IPAC2021-MOPAB392},
  url          = {https://jacow.org/ipac2021/papers/mopab392.pdf},
  note         = {https://doi.org/10.18429/JACoW-IPAC2021-MOPAB392},
  abstract     = {{In order to obtain the target frequency in operation, the resonant frequency of superconducting radiofrequency cavities is controlled and adjusted from the manufacturing to the end of preparation phase. Reaching this right frequency can be challenging due to the narrow frequency range defined by the tuning sensitivity of the cavity and the capability of the tuner. Mechanical deformation until plasticity is attained is of great interest to tune SRF cavities when large frequency shift is needed. But once a cavity is dressed with its helium tank, the only accessible part is its beam pipe, reducing the mechanical action to a push/pull action. This limited possibility has hence to be skilfully associated with chemical etching. An original mechanical tuning of Spoke dressed cavities consists in increasing the pressure inside the helium tank to induce a permanent deformation of the cavity walls. The frequency shift induced by nonlinear deformation is numerically evaluated in order to determine the pressure increments. Both methods were successfully performed on the cavities of the ESS accelerator and of the Myrrha project.}},
}