Over the last decade much attention was given in increasing the quality factor of superconducting radio frequency cavities by impurity doping. Prior to the era of doping, the final cavity processing technique to achieve the high accelerating gradient includes the "in-situ" low temperature baking of SRF cavities at temperature ∼ 120 • C for several hours. Here, we present the results of a series of measurements on 1.3 GHz TESLA shape single-cell cavities with successive low temperature baking at 120 • C up to 96 hours. The experimental data were analyzed with available theory of superconductivity to elucidate the effect of the duration of low temperature baking on the superconducting properties of cavity materials as well as the rf performance. In addition, the rf loss related to the trapping of residual magnetic field refereed as flux trapping sensitivity was measured with respect to the duration of 120 • C bake.
We present the cost-effective production of superconducting
radio frequency (SRF) cavities made of medium grain (MG) niobium
(Nb) discs directly sliced from forged and annealed billet. This
production method provides clean surface conditions and reliable
mechanical characteristics with sub-millimeter average grain size
resulting in stable SRF cavity production. We propose to apply this
material to particle accelerator in the science and industrial
applications. The science applications require high field
gradients(≥ 30 MV/m) particularly in pulsed mode. The
industrial applications require high Q
0 values with moderate
gradients (∼ 20 MV/m) in CW mode operation. This paper
describes the MG Nb disc production recently demonstrated and
discusses future prospects for application in advanced particle
accelerators in the science and industrial applications.
We have successfully fabricated two 1.5 GHz single cell from forged ingot of residual resistivity ratio ~100.• Both cavities are processed with bulk EP, followed by 650 C/10 hrs annealing. • The rf performance of one of the cavity tested to this date is limited ~14 MV/m. Multipacting barrier was predicted at this gradient and it may be the likely the cause of quench.Oscillating superleak transducer (OST) sensors were used during rf measurements to detect the quench location and data are under review.
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