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Study of Nb-Cu 1.3 GHz SRF cavity resonators for future particle accelerators
Niobium-coated superconducting radio-frequency cavities have a number of advantages over cavities made from bulk niobium. Cavities coated with high-power impulse magnetron sputtering are tested at CERN in order to optimize the coating and study the Q-slope that limits the performance. To accurately...
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Lenguaje: | eng |
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2017
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Acceso en línea: | http://cds.cern.ch/record/2280159 |
_version_ | 1780955517193027584 |
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author | Amelin, Kirill |
author_facet | Amelin, Kirill |
author_sort | Amelin, Kirill |
collection | CERN |
description | Niobium-coated superconducting radio-frequency cavities have a number of advantages over cavities made from bulk niobium. Cavities coated with high-power impulse magnetron sputtering are tested at CERN in order to optimize the coating and study the Q-slope that limits the performance. To accurately measure the quality factor as a function of accelerating field, it is important to have good matching between an input antenna and a cavity impedance. To improve the matching, a variable coupler that changes the length of the antenna can be used. We have shown that the Q-factor of the input antenna can be changed between $10^7-10^{11}$ by moving the antenna, which should allow to achieve critical coupling with a cavity. This technology could be used in future measurements, so that reflections are always minimized. |
id | cern-2280159 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2017 |
record_format | invenio |
spelling | cern-22801592019-09-30T06:29:59Zhttp://cds.cern.ch/record/2280159engAmelin, KirillStudy of Nb-Cu 1.3 GHz SRF cavity resonators for future particle acceleratorsEngineeringNiobium-coated superconducting radio-frequency cavities have a number of advantages over cavities made from bulk niobium. Cavities coated with high-power impulse magnetron sputtering are tested at CERN in order to optimize the coating and study the Q-slope that limits the performance. To accurately measure the quality factor as a function of accelerating field, it is important to have good matching between an input antenna and a cavity impedance. To improve the matching, a variable coupler that changes the length of the antenna can be used. We have shown that the Q-factor of the input antenna can be changed between $10^7-10^{11}$ by moving the antenna, which should allow to achieve critical coupling with a cavity. This technology could be used in future measurements, so that reflections are always minimized. CERN-STUDENTS-Note-2017-079oai:cds.cern.ch:22801592017-08-18 |
spellingShingle | Engineering Amelin, Kirill Study of Nb-Cu 1.3 GHz SRF cavity resonators for future particle accelerators |
title | Study of Nb-Cu 1.3 GHz SRF cavity resonators for future particle accelerators |
title_full | Study of Nb-Cu 1.3 GHz SRF cavity resonators for future particle accelerators |
title_fullStr | Study of Nb-Cu 1.3 GHz SRF cavity resonators for future particle accelerators |
title_full_unstemmed | Study of Nb-Cu 1.3 GHz SRF cavity resonators for future particle accelerators |
title_short | Study of Nb-Cu 1.3 GHz SRF cavity resonators for future particle accelerators |
title_sort | study of nb-cu 1.3 ghz srf cavity resonators for future particle accelerators |
topic | Engineering |
url | http://cds.cern.ch/record/2280159 |
work_keys_str_mv | AT amelinkirill studyofnbcu13ghzsrfcavityresonatorsforfutureparticleaccelerators |