Frequency dependence of trapped flux sensitivity in SRF cavities
In this letter, we present the frequency dependence of the vortex surface resistance of bulk niobium accelerating cavities as a function of different state-of-the-art surface treatments. Higher flux surface resistance per amount of trapped magnetic field—sensitivity—is observed for higher frequencie...
Gespeichert in:
Veröffentlicht in: | Applied physics letters 2018-02, Vol.112 (7) |
---|---|
Hauptverfasser: | , , , , , , , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | |
---|---|
container_issue | 7 |
container_start_page | |
container_title | Applied physics letters |
container_volume | 112 |
creator | Checchin, M. Martinello, M. Grassellino, A. Aderhold, S. Chandrasekaran, S. K. Melnychuk, O. S. Posen, S. Romanenko, A. Sergatskov, D. A. |
description | In this letter, we present the frequency dependence of the vortex surface resistance of bulk niobium accelerating cavities as a function of different state-of-the-art surface treatments. Higher flux surface resistance per amount of trapped magnetic field—sensitivity—is observed for higher frequencies, in agreement with our theoretical model. Higher sensitivity is observed for N-doped cavities, which possess an intermediate value of the electron mean-free-path, compared to 120 °C and EP/BCP cavities. Experimental results from our study showed that the sensitivity has a non-monotonic trend as a function of the mean-free-path, including frequencies other than 1.3 GHz, and that the vortex response to the rf field can be tuned from the pinning regime to flux-flow regime by manipulating the frequency and/or the mean-free-path of the resonator, as reported in our previous studies. The frequency dependence of the trapped flux sensitivity to the amplitude of the accelerating gradient is also highlighted. |
doi_str_mv | 10.1063/1.5016525 |
format | Article |
fullrecord | <record><control><sourceid>proquest_osti_</sourceid><recordid>TN_cdi_proquest_journals_2115807750</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2115807750</sourcerecordid><originalsourceid>FETCH-LOGICAL-c389t-8aea88ae4535c89427bdc362128baaddf854bc4fac55a7ae1eecda5fa3e1dbda3</originalsourceid><addsrcrecordid>eNqd0E1LAzEQBuAgCtbqwX8Q9KSwNdlsdtObUqwKBcGPc8gmE0zRZE3SYv-9KS1495Jk4GFm8iJ0TsmEkpbd0AkntOU1P0AjSrquYpSKQzQihLCqnXJ6jE5SWpaS14yN0O08wvcKvN5gAwN4U56Ag8U5qmEAg-3n6gcn8Mllt3Z5g53Hry9zrFWpHKRTdGTVZ4Kz_T1G7_P7t9ljtXh-eJrdLSrNxDRXQoES5Wg441pMm7rrjWZtTWvRK2WMFbzpdWOV5lx1CiiANopbxYCa3ig2Rhe7viFlJ5N2GfSHDt6DzpI2jLQtKehyh4YYyq9Slsuwir7sJWtKuSiB8K262ikdQ0oRrByi-1JxIymR2xQllfsUi73e2e1ElV3w_8PrEP-gHIxlv_WxgI0</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2115807750</pqid></control><display><type>article</type><title>Frequency dependence of trapped flux sensitivity in SRF cavities</title><source>AIP Journals Complete</source><source>Alma/SFX Local Collection</source><creator>Checchin, M. ; Martinello, M. ; Grassellino, A. ; Aderhold, S. ; Chandrasekaran, S. K. ; Melnychuk, O. S. ; Posen, S. ; Romanenko, A. ; Sergatskov, D. A.</creator><creatorcontrib>Checchin, M. ; Martinello, M. ; Grassellino, A. ; Aderhold, S. ; Chandrasekaran, S. K. ; Melnychuk, O. S. ; Posen, S. ; Romanenko, A. ; Sergatskov, D. A. ; Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)</creatorcontrib><description>In this letter, we present the frequency dependence of the vortex surface resistance of bulk niobium accelerating cavities as a function of different state-of-the-art surface treatments. Higher flux surface resistance per amount of trapped magnetic field—sensitivity—is observed for higher frequencies, in agreement with our theoretical model. Higher sensitivity is observed for N-doped cavities, which possess an intermediate value of the electron mean-free-path, compared to 120 °C and EP/BCP cavities. Experimental results from our study showed that the sensitivity has a non-monotonic trend as a function of the mean-free-path, including frequencies other than 1.3 GHz, and that the vortex response to the rf field can be tuned from the pinning regime to flux-flow regime by manipulating the frequency and/or the mean-free-path of the resonator, as reported in our previous studies. The frequency dependence of the trapped flux sensitivity to the amplitude of the accelerating gradient is also highlighted.</description><identifier>ISSN: 0003-6951</identifier><identifier>EISSN: 1077-3118</identifier><identifier>DOI: 10.1063/1.5016525</identifier><identifier>CODEN: APPLAB</identifier><language>eng</language><publisher>Melville: American Institute of Physics</publisher><subject>Applied physics ; CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS ; Computational fluid dynamics ; Dependence ; Flux ; Flux pinning ; Holes ; Niobium ; PARTICLE ACCELERATORS ; Sensitivity ; Surface resistance</subject><ispartof>Applied physics letters, 2018-02, Vol.112 (7)</ispartof><rights>Author(s)</rights><rights>2018 Author(s). All article content, except where otherwise noted, is licensed under a Creative Commons Attribution (CC BY) license (http://creativecommons.org/licenses/by/4.0/).</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c389t-8aea88ae4535c89427bdc362128baaddf854bc4fac55a7ae1eecda5fa3e1dbda3</citedby><cites>FETCH-LOGICAL-c389t-8aea88ae4535c89427bdc362128baaddf854bc4fac55a7ae1eecda5fa3e1dbda3</cites><orcidid>0000-0001-8468-3328 ; 0000-0002-2089-8685 ; 0000-0003-1979-8721 ; 0000000220898685 ; 0000000319798721 ; 0000000184683328</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://pubs.aip.org/apl/article-lookup/doi/10.1063/1.5016525$$EHTML$$P50$$Gscitation$$Hfree_for_read</linktohtml><link.rule.ids>230,314,780,784,794,885,4512,27924,27925,76384</link.rule.ids><backlink>$$Uhttps://www.osti.gov/servlets/purl/1430660$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Checchin, M.</creatorcontrib><creatorcontrib>Martinello, M.</creatorcontrib><creatorcontrib>Grassellino, A.</creatorcontrib><creatorcontrib>Aderhold, S.</creatorcontrib><creatorcontrib>Chandrasekaran, S. K.</creatorcontrib><creatorcontrib>Melnychuk, O. S.</creatorcontrib><creatorcontrib>Posen, S.</creatorcontrib><creatorcontrib>Romanenko, A.</creatorcontrib><creatorcontrib>Sergatskov, D. A.</creatorcontrib><creatorcontrib>Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)</creatorcontrib><title>Frequency dependence of trapped flux sensitivity in SRF cavities</title><title>Applied physics letters</title><description>In this letter, we present the frequency dependence of the vortex surface resistance of bulk niobium accelerating cavities as a function of different state-of-the-art surface treatments. Higher flux surface resistance per amount of trapped magnetic field—sensitivity—is observed for higher frequencies, in agreement with our theoretical model. Higher sensitivity is observed for N-doped cavities, which possess an intermediate value of the electron mean-free-path, compared to 120 °C and EP/BCP cavities. Experimental results from our study showed that the sensitivity has a non-monotonic trend as a function of the mean-free-path, including frequencies other than 1.3 GHz, and that the vortex response to the rf field can be tuned from the pinning regime to flux-flow regime by manipulating the frequency and/or the mean-free-path of the resonator, as reported in our previous studies. The frequency dependence of the trapped flux sensitivity to the amplitude of the accelerating gradient is also highlighted.</description><subject>Applied physics</subject><subject>CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS</subject><subject>Computational fluid dynamics</subject><subject>Dependence</subject><subject>Flux</subject><subject>Flux pinning</subject><subject>Holes</subject><subject>Niobium</subject><subject>PARTICLE ACCELERATORS</subject><subject>Sensitivity</subject><subject>Surface resistance</subject><issn>0003-6951</issn><issn>1077-3118</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2018</creationdate><recordtype>article</recordtype><recordid>eNqd0E1LAzEQBuAgCtbqwX8Q9KSwNdlsdtObUqwKBcGPc8gmE0zRZE3SYv-9KS1495Jk4GFm8iJ0TsmEkpbd0AkntOU1P0AjSrquYpSKQzQihLCqnXJ6jE5SWpaS14yN0O08wvcKvN5gAwN4U56Ag8U5qmEAg-3n6gcn8Mllt3Z5g53Hry9zrFWpHKRTdGTVZ4Kz_T1G7_P7t9ljtXh-eJrdLSrNxDRXQoES5Wg441pMm7rrjWZtTWvRK2WMFbzpdWOV5lx1CiiANopbxYCa3ig2Rhe7viFlJ5N2GfSHDt6DzpI2jLQtKehyh4YYyq9Slsuwir7sJWtKuSiB8K262ikdQ0oRrByi-1JxIymR2xQllfsUi73e2e1ElV3w_8PrEP-gHIxlv_WxgI0</recordid><startdate>20180212</startdate><enddate>20180212</enddate><creator>Checchin, M.</creator><creator>Martinello, M.</creator><creator>Grassellino, A.</creator><creator>Aderhold, S.</creator><creator>Chandrasekaran, S. K.</creator><creator>Melnychuk, O. S.</creator><creator>Posen, S.</creator><creator>Romanenko, A.</creator><creator>Sergatskov, D. A.</creator><general>American Institute of Physics</general><general>American Institute of Physics (AIP)</general><scope>AJDQP</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>OIOZB</scope><scope>OTOTI</scope><orcidid>https://orcid.org/0000-0001-8468-3328</orcidid><orcidid>https://orcid.org/0000-0002-2089-8685</orcidid><orcidid>https://orcid.org/0000-0003-1979-8721</orcidid><orcidid>https://orcid.org/0000000220898685</orcidid><orcidid>https://orcid.org/0000000319798721</orcidid><orcidid>https://orcid.org/0000000184683328</orcidid></search><sort><creationdate>20180212</creationdate><title>Frequency dependence of trapped flux sensitivity in SRF cavities</title><author>Checchin, M. ; Martinello, M. ; Grassellino, A. ; Aderhold, S. ; Chandrasekaran, S. K. ; Melnychuk, O. S. ; Posen, S. ; Romanenko, A. ; Sergatskov, D. A.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c389t-8aea88ae4535c89427bdc362128baaddf854bc4fac55a7ae1eecda5fa3e1dbda3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2018</creationdate><topic>Applied physics</topic><topic>CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS</topic><topic>Computational fluid dynamics</topic><topic>Dependence</topic><topic>Flux</topic><topic>Flux pinning</topic><topic>Holes</topic><topic>Niobium</topic><topic>PARTICLE ACCELERATORS</topic><topic>Sensitivity</topic><topic>Surface resistance</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Checchin, M.</creatorcontrib><creatorcontrib>Martinello, M.</creatorcontrib><creatorcontrib>Grassellino, A.</creatorcontrib><creatorcontrib>Aderhold, S.</creatorcontrib><creatorcontrib>Chandrasekaran, S. K.</creatorcontrib><creatorcontrib>Melnychuk, O. S.</creatorcontrib><creatorcontrib>Posen, S.</creatorcontrib><creatorcontrib>Romanenko, A.</creatorcontrib><creatorcontrib>Sergatskov, D. A.</creatorcontrib><creatorcontrib>Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)</creatorcontrib><collection>AIP Open Access Journals</collection><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>OSTI.GOV - Hybrid</collection><collection>OSTI.GOV</collection><jtitle>Applied physics letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Checchin, M.</au><au>Martinello, M.</au><au>Grassellino, A.</au><au>Aderhold, S.</au><au>Chandrasekaran, S. K.</au><au>Melnychuk, O. S.</au><au>Posen, S.</au><au>Romanenko, A.</au><au>Sergatskov, D. A.</au><aucorp>Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Frequency dependence of trapped flux sensitivity in SRF cavities</atitle><jtitle>Applied physics letters</jtitle><date>2018-02-12</date><risdate>2018</risdate><volume>112</volume><issue>7</issue><issn>0003-6951</issn><eissn>1077-3118</eissn><coden>APPLAB</coden><abstract>In this letter, we present the frequency dependence of the vortex surface resistance of bulk niobium accelerating cavities as a function of different state-of-the-art surface treatments. Higher flux surface resistance per amount of trapped magnetic field—sensitivity—is observed for higher frequencies, in agreement with our theoretical model. Higher sensitivity is observed for N-doped cavities, which possess an intermediate value of the electron mean-free-path, compared to 120 °C and EP/BCP cavities. Experimental results from our study showed that the sensitivity has a non-monotonic trend as a function of the mean-free-path, including frequencies other than 1.3 GHz, and that the vortex response to the rf field can be tuned from the pinning regime to flux-flow regime by manipulating the frequency and/or the mean-free-path of the resonator, as reported in our previous studies. The frequency dependence of the trapped flux sensitivity to the amplitude of the accelerating gradient is also highlighted.</abstract><cop>Melville</cop><pub>American Institute of Physics</pub><doi>10.1063/1.5016525</doi><tpages>4</tpages><orcidid>https://orcid.org/0000-0001-8468-3328</orcidid><orcidid>https://orcid.org/0000-0002-2089-8685</orcidid><orcidid>https://orcid.org/0000-0003-1979-8721</orcidid><orcidid>https://orcid.org/0000000220898685</orcidid><orcidid>https://orcid.org/0000000319798721</orcidid><orcidid>https://orcid.org/0000000184683328</orcidid><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | ISSN: 0003-6951 |
ispartof | Applied physics letters, 2018-02, Vol.112 (7) |
issn | 0003-6951 1077-3118 |
language | eng |
recordid | cdi_proquest_journals_2115807750 |
source | AIP Journals Complete; Alma/SFX Local Collection |
subjects | Applied physics CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS Computational fluid dynamics Dependence Flux Flux pinning Holes Niobium PARTICLE ACCELERATORS Sensitivity Surface resistance |
title | Frequency dependence of trapped flux sensitivity in SRF cavities |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-21T08%3A17%3A40IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_osti_&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Frequency%20dependence%20of%20trapped%20flux%20sensitivity%20in%20SRF%20cavities&rft.jtitle=Applied%20physics%20letters&rft.au=Checchin,%20M.&rft.aucorp=Fermi%20National%20Accelerator%20Lab.%20(FNAL),%20Batavia,%20IL%20(United%20States)&rft.date=2018-02-12&rft.volume=112&rft.issue=7&rft.issn=0003-6951&rft.eissn=1077-3118&rft.coden=APPLAB&rft_id=info:doi/10.1063/1.5016525&rft_dat=%3Cproquest_osti_%3E2115807750%3C/proquest_osti_%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2115807750&rft_id=info:pmid/&rfr_iscdi=true |