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MOYBB3 |
Progress in Nb3Sn SRF Cavities at Cornell University |
37 |
SUPLS08 |
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- R.D. Porter, H. Hu, M. Liepe, N.A. Stilin, Z. Sun, M.J. Tao
Cornell University (CLASSE), Cornell Laboratory for Accelerator-Based Sciences and Education, Ithaca, New York, USA
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Niobium-3 Tin (NbSn) is the most promising alternative material for next-generation SRF cavities. The material can obtain high quality factors (> 1010) at 4.2 K and could theoretically support ~ 96 MV/m operation of a TESLA elliptical style cavity. Current Nb3Sn cavities made at Cornell University achieve high quality factors but are limited to about 17 MV/m in CW operation due to the presence of a surface defect. Here we examine recent results on studying the quench mechanism and propose that surface roughness is a major limiter for accelerating gradients. Furthermore, we discuss recent work on reducing the surface roughness including chemical polishing, modification of material growth, and tin electroplating.
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DOI • |
reference for this paper
※ https://doi.org/10.18429/JACoW-NAPAC2019-MOYBB3
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About • |
paper received ※ 02 September 2019 paper accepted ※ 12 September 2019 issue date ※ 08 October 2019 |
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