[2009.09505] Interstrip Capacitances of the Readout Board used in Large Triple-GEM Detectors for the CMS Muon Upgrade

<?xml version="1.0" encoding="UTF-8"?> <!DOCTYPE html PUBLIC "-//W3C//DTD XHTML 1.0 Transitional//EN" "http://www.w3.org/TR/xhtml1/DTD/xhtml1-transitional.dtd"> <html xmlns="http://www.w3.org/1999/xhtml" lang="en" xml:lang="en"> <head> <title>[2009.09505] Interstrip Capacitances of the Readout Board used in Large Triple-GEM Detectors for the CMS Muon Upgrade</title> <meta name="viewport" content="width=device-width, initial-scale=1"> <link rel="apple-touch-icon" sizes="180x180" href="/static/browse/0.3.4/images/icons/apple-touch-icon.png"> <link rel="icon" type="image/png" sizes="32x32" href="/static/browse/0.3.4/images/icons/favicon-32x32.png"> <link rel="icon" type="image/png" sizes="16x16" href="/static/browse/0.3.4/images/icons/favicon-16x16.png"> <link rel="manifest" href="/static/browse/0.3.4/images/icons/site.webmanifest"> <link rel="mask-icon" href="/static/browse/0.3.4/images/icons/safari-pinned-tab.svg" color="#5bbad5"> <meta name="msapplication-TileColor" content="#da532c"> <meta name="theme-color" content="#ffffff"> <link rel="stylesheet" type="text/css" media="screen" href="/static/browse/0.3.4/css/arXiv.css?v=20240822" /> <link rel="stylesheet" type="text/css" media="print" href="/static/browse/0.3.4/css/arXiv-print.css?v=20200611" /> <link rel="stylesheet" type="text/css" media="screen" href="/static/browse/0.3.4/css/browse_search.css" /> <script language="javascript" src="/static/browse/0.3.4/js/accordion.js" /></script> <link rel="canonical" href="https://arxiv.org/abs/2009.09505"/> <meta name="description" content="Abstract page for arXiv paper 2009.09505: Interstrip Capacitances of the Readout Board used in Large Triple-GEM Detectors for the CMS Muon Upgrade"><meta property="og:type" content="website" /> <meta property="og:site_name" content="arXiv.org" /> <meta property="og:title" content="Interstrip Capacitances of the Readout Board used in Large Triple-GEM Detectors for the CMS Muon Upgrade" /> <meta property="og:url" content="https://arxiv.org/abs/2009.09505v1" /> <meta property="og:image" content="/static/browse/0.3.4/images/arxiv-logo-fb.png" /> <meta property="og:image:secure_url" content="/static/browse/0.3.4/images/arxiv-logo-fb.png" /> <meta property="og:image:width" content="1200" /> <meta property="og:image:height" content="700" /> <meta property="og:image:alt" content="arXiv logo"/> <meta property="og:description" content="We present analytical calculations, Finite Element Analysis modeling, and physical measurements of the interstrip capacitances for different potential strip geometries and dimensions of the readout boards for the GE2/1 triple-Gas Electron Multiplier detector in the CMS muon system upgrade. The main goal of the study is to find configurations that minimize the interstrip capacitances and consequently maximize the signal-to-noise ratio for the detector. We find agreement at the 1.5--4.8% level between the two methods of calculations and on the average at the 17% level between calculations and measurements. A configuration with halved strip lengths and doubled strip widths results in a measured 27--29% reduction over the original configuration while leaving the total number of strips unchanged. We have now adopted this design modification for all eight module types of the GE2/1 detector and will produce the final detector with this new strip design."/> <meta name="twitter:site" content="@arxiv"/> <meta name="twitter:card" content="summary"/> <meta name="twitter:title" content="Interstrip Capacitances of the Readout Board used in Large..."/> <meta name="twitter:description" content="We present analytical calculations, Finite Element Analysis modeling, and physical measurements of the interstrip capacitances for different potential strip geometries and dimensions of the..."/> <meta name="twitter:image" content="https://static.arxiv.org/icons/twitter/arxiv-logo-twitter-square.png"/> <meta name="twitter:image:alt" content="arXiv logo"/> <link rel="stylesheet" media="screen" type="text/css" href="/static/browse/0.3.4/css/tooltip.css"/><link rel="stylesheet" media="screen" type="text/css" href="https://static.arxiv.org/js/bibex-dev/bibex.css?20200709"/> <script src="/static/browse/0.3.4/js/mathjaxToggle.min.js" type="text/javascript"></script> <script src="//code.jquery.com/jquery-latest.min.js" type="text/javascript"></script> <script src="//cdn.jsdelivr.net/npm/js-cookie@2/src/js.cookie.min.js" type="text/javascript"></script> <script src="//cdn.jsdelivr.net/npm/dompurify@2.3.5/dist/purify.min.js"></script> <script src="/static/browse/0.3.4/js/toggle-labs.js?20241022" type="text/javascript"></script> <script src="/static/browse/0.3.4/js/cite.js" type="text/javascript"></script><meta name="citation_title" content="Interstrip Capacitances of the Readout Board used in Large Triple-GEM Detectors for the CMS Muon Upgrade" /><meta name="citation_author" content="Abbas, M." /><meta name="citation_author" content="Abbrescia, M." /><meta name="citation_author" content="Abdalla, H." /><meta name="citation_author" content="Abdelalim, A." /><meta name="citation_author" content="AbuZeid, S." /><meta name="citation_author" content="Agapitos, A." /><meta name="citation_author" content="Ahmad, A." /><meta name="citation_author" content="Ahmed, A." /><meta name="citation_author" content="Ahmed, W." /><meta name="citation_author" content="Aim猫, C." /><meta name="citation_author" content="Aruta, C." /><meta name="citation_author" content="Asghar, I." /><meta name="citation_author" content="Aspell, P." /><meta name="citation_author" content="Avila, C." /><meta name="citation_author" content="Babbar, J." /><meta name="citation_author" content="Ban, Y." /><meta name="citation_author" content="Band, R." /><meta name="citation_author" content="Bansal, S." /><meta name="citation_author" content="Benussi, L." /><meta name="citation_author" content="Bhatnagar, V." /><meta name="citation_author" content="Bianco, M." /><meta name="citation_author" content="Bianco, S." /><meta name="citation_author" content="Black, K." /><meta name="citation_author" content="Borgonovi, L." /><meta name="citation_author" content="Bouhali, O." /><meta name="citation_author" content="Braghieri, A." /><meta name="citation_author" content="Braibant, S." /><meta name="citation_author" content="Butalla, S." /><meta name="citation_author" content="Calzaferri, S." /><meta name="citation_author" content="Caponero, M." /><meta name="citation_author" content="Cassese, F." /><meta name="citation_author" content="Cavallo, N." /><meta name="citation_author" content="Chauhan, S." /><meta name="citation_author" content="Colaleo, A." /><meta name="citation_author" content="Collins, J." /><meta name="citation_author" content="Garcia, A. 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C." /><meta name="citation_author" content="Yang, Y." /><meta name="citation_author" content="Yang, U." /><meta name="citation_author" content="Yongho, J." /><meta name="citation_author" content="Yoon, I." /><meta name="citation_author" content="You, Z." /><meta name="citation_author" content="Yu, I." /><meta name="citation_author" content="Zaleski, S." /><meta name="citation_doi" content="10.1088/1748-0221/15/12/P12019" /><meta name="citation_date" content="2020/09/20" /><meta name="citation_online_date" content="2020/09/20" /><meta name="citation_pdf_url" content="http://arxiv.org/pdf/2009.09505" /><meta name="citation_arxiv_id" content="2009.09505" /><meta name="citation_abstract" content="We present analytical calculations, Finite Element Analysis modeling, and physical measurements of the interstrip capacitances for different potential strip geometries and dimensions of the readout boards for the GE2/1 triple-Gas Electron Multiplier detector in the CMS muon system upgrade. The main goal of the study is to find configurations that minimize the interstrip capacitances and consequently maximize the signal-to-noise ratio for the detector. We find agreement at the 1.5--4.8% level between the two methods of calculations and on the average at the 17% level between calculations and measurements. A configuration with halved strip lengths and doubled strip widths results in a measured 27--29% reduction over the original configuration while leaving the total number of strips unchanged. We have now adopted this design modification for all eight module types of the GE2/1 detector and will produce the final detector with this new strip design." /> </head> <body class="with-cu-identity"> <div class="flex-wrap-footer"> <header> <a href="#content" class="is-sr-only">Skip to main content</a>  <div class="columns is-vcentered is-hidden-mobile" id="cu-identity"> <div class="column" id="cu-logo"> <a href="https://www.cornell.edu/"><img src="/static/browse/0.3.4/images/icons/cu/cornell-reduced-white-SMALL.svg" alt="Cornell University" /></a> </div><div class="column" id="support-ack"> <span id="support-ack-url">We gratefully acknowledge support from the Simons Foundation, <a href="https://info.arxiv.org/about/ourmembers.html">member institutions</a>, and all contributors.</span> <a href="https://info.arxiv.org/about/donate.html" class="btn-header-donate">Donate</a> </div> </div> <div id="header" class="is-hidden-mobile"> <a aria-hidden="true" tabindex="-1" href="/IgnoreMe"></a> 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href="https://arxiv.org/search/physics?searchtype=author&query=Abbas,+M" rel="nofollow">M. Abbas</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Abbrescia,+M" rel="nofollow">M. Abbrescia</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Abdalla,+H" rel="nofollow">H. Abdalla</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Abdelalim,+A" rel="nofollow">A. Abdelalim</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=AbuZeid,+S" rel="nofollow">S. AbuZeid</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Agapitos,+A" rel="nofollow">A. Agapitos</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Ahmad,+A" rel="nofollow">A. Ahmad</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Ahmed,+A" rel="nofollow">A. Ahmed</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Ahmed,+W" rel="nofollow">W. Ahmed</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Aim%C3%A8,+C" rel="nofollow">C. Aim猫</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Aruta,+C" rel="nofollow">C. Aruta</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Asghar,+I" rel="nofollow">I. Asghar</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Aspell,+P" rel="nofollow">P. Aspell</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Avila,+C" rel="nofollow">C. Avila</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Babbar,+J" rel="nofollow">J. Babbar</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Ban,+Y" rel="nofollow">Y. Ban</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Band,+R" rel="nofollow">R. Band</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Bansal,+S" rel="nofollow">S. Bansal</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Benussi,+L" rel="nofollow">L. Benussi</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Bhatnagar,+V" rel="nofollow">V. Bhatnagar</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Bianco,+M" rel="nofollow">M. Bianco</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Bianco,+S" rel="nofollow">S. Bianco</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Black,+K" rel="nofollow">K. Black</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Borgonovi,+L" rel="nofollow">L. Borgonovi</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Bouhali,+O" rel="nofollow">O. Bouhali</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Braghieri,+A" rel="nofollow">A. Braghieri</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Braibant,+S" rel="nofollow">S. Braibant</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Butalla,+S" rel="nofollow">S. 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Tuuva</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Tytgat,+M" rel="nofollow">M. Tytgat</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Vanegas,+I+V+N" rel="nofollow">I. Vai N. Vanegas</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Venditti,+R" rel="nofollow">R. Venditti</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Verwilligen,+P" rel="nofollow">P. Verwilligen</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Vetens,+W" rel="nofollow">W. Vetens</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Virdi,+A" rel="nofollow">A. Virdi</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Vitulo,+P" rel="nofollow">P. Vitulo</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Wajid,+A" rel="nofollow">A. Wajid</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Wang,+D" rel="nofollow">D. Wang</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Wang,+K" rel="nofollow">K. Wang</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Watson,+I" rel="nofollow">I.J. Watson</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Weatherwax,+J" rel="nofollow">J. Weatherwax</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Wickramage,+N" rel="nofollow">N. Wickramage</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Wickramarathna,+D" rel="nofollow">D.D.C. Wickramarathna</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Yang,+Y" rel="nofollow">Y. Yang</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Yang,+U" rel="nofollow">U. Yang</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Yongho,+J" rel="nofollow">J. Yongho</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Yoon,+I" rel="nofollow">I. Yoon</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=You,+Z" rel="nofollow">Z. You</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Yu,+I" rel="nofollow">I. Yu</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Zaleski,+S" rel="nofollow">S. Zaleski</a> (on behalf of the CMS Muon Group) </div> <a href="javascript:toggleAuthorList('long-author-list','et al. (81 additional authors not shown)');" title="Show Entire Author List" id="toggle"> et al. (81 additional authors not shown)</a> <noscript> You must enable JavaScript to view entire author list.</noscript></div> <div id="download-button-info" hidden>View a PDF of the paper titled Interstrip Capacitances of the Readout Board used in Large Triple-GEM Detectors for the CMS Muon Upgrade, by M. Abbas and 179 other authors</div> <a class="mobile-submission-download" href="/pdf/2009.09505">View PDF</a> <blockquote class="abstract mathjax"> <span class="descriptor">Abstract:</span>We present analytical calculations, Finite Element Analysis modeling, and physical measurements of the interstrip capacitances for different potential strip geometries and dimensions of the readout boards for the GE2/1 triple-Gas Electron Multiplier detector in the CMS muon system upgrade. The main goal of the study is to find configurations that minimize the interstrip capacitances and consequently maximize the signal-to-noise ratio for the detector. We find agreement at the 1.5--4.8% level between the two methods of calculations and on the average at the 17% level between calculations and measurements. A configuration with halved strip lengths and doubled strip widths results in a measured 27--29% reduction over the original configuration while leaving the total number of strips unchanged. We have now adopted this design modification for all eight module types of the GE2/1 detector and will produce the final detector with this new strip design. </blockquote>  <div class="metatable"> <table summary="Additional metadata"> <tr> <td class="tablecell label">Comments:</td> <td class="tablecell comments mathjax">22 pages, 14 figures</td> </tr> <tr> <td class="tablecell label">Subjects:</td> <td class="tablecell subjects"> <span class="primary-subject">Instrumentation and Detectors (physics.ins-det)</span>; High Energy Physics - Experiment (hep-ex)</td> </tr><tr> <td class="tablecell label">Cite as:</td> <td class="tablecell arxivid"><span class="arxivid"><a href="https://arxiv.org/abs/2009.09505">arXiv:2009.09505</a> [physics.ins-det]</span></td> </tr> <tr> <td class="tablecell label"> </td> <td class="tablecell arxividv">(or <span class="arxivid"> <a href="https://arxiv.org/abs/2009.09505v1">arXiv:2009.09505v1</a> [physics.ins-det]</span> for this version) </td> </tr> <tr> <td class="tablecell label"> </td> <td class="tablecell arxivdoi"> <a href="https://doi.org/10.48550/arXiv.2009.09505" id="arxiv-doi-link">https://doi.org/10.48550/arXiv.2009.09505</a><div class="button-and-tooltip"> <button class="more-info" aria-describedby="more-info-desc-1"> <svg height="15" role="presentation" xmlns="http://www.w3.org/2000/svg" viewBox="0 0 512 512"><path fill="currentColor" d="M256 8C119.043 8 8 119.083 8 256c0 136.997 111.043 248 248 248s248-111.003 248-248C504 119.083 392.957 8 256 8zm0 110c23.196 0 42 18.804 42 42s-18.804 42-42 42-42-18.804-42-42 18.804-42 42-42zm56 254c0 6.627-5.373 12-12 12h-88c-6.627 0-12-5.373-12-12v-24c0-6.627 5.373-12 12-12h12v-64h-12c-6.627 0-12-5.373-12-12v-24c0-6.627 5.373-12 12-12h64c6.627 0 12 5.373 12 12v100h12c6.627 0 12 5.373 12 12v24z" class=""></path></svg> <span class="visually-hidden">Focus to learn more</span> </button>  <div role="tooltip" id="more-info-desc-1"> <span class="left-corner"></span> arXiv-issued DOI via DataCite</div> </div> </td> </tr> <tr> <td class="tablecell label">Journal reference:</td> <td class="tablecell jref">2020 JINST 15 P12019</td> </tr> <tr> <td class="tablecell label"> <abbr title="Digital Object Identifier">Related DOI</abbr>: </td> <td class="tablecell doi"><a href="https://doi.org/10.1088/1748-0221/15/12/P12019" data-doi="10.1088/1748-0221/15/12/P12019" class="link-https link-external" rel="external noopener nofollow">https://doi.org/10.1088/1748-0221/15/12/P12019</a>  <div class="button-and-tooltip"> <button class="more-info" aria-describedby="more-info-desc-1"> <svg height="15" role="presentation" xmlns="http://www.w3.org/2000/svg" viewBox="0 0 512 512"><path fill="currentColor" d="M256 8C119.043 8 8 119.083 8 256c0 136.997 111.043 248 248 248s248-111.003 248-248C504 119.083 392.957 8 256 8zm0 110c23.196 0 42 18.804 42 42s-18.804 42-42 42-42-18.804-42-42 18.804-42 42-42zm56 254c0 6.627-5.373 12-12 12h-88c-6.627 0-12-5.373-12-12v-24c0-6.627 5.373-12 12-12h12v-64h-12c-6.627 0-12-5.373-12-12v-24c0-6.627 5.373-12 12-12h64c6.627 0 12 5.373 12 12v100h12c6.627 0 12 5.373 12 12v24z" class=""></path></svg> <span class="visually-hidden">Focus to learn more</span> </button>  <div role="tooltip" id="more-info-desc-1"> <span class="left-corner"></span> DOI(s) linking to related resources </div> </div> </td> </tr> </table> </div> </div> </div> <div class="submission-history"> <h2>Submission history</h2> From: Stephen Butalla [<a href="/show-email/dcee8b1f/2009.09505" rel="nofollow">view email</a>] <br/> <strong>[v1]</strong> Sun, 20 Sep 2020 19:18:06 UTC (27,838 KB)<br/> </div> </div>  <div class="extra-services"> <div class="full-text"> <a name="other"></a> <span class="descriptor">Full-text links:</span> <h2>Access Paper:</h2> <ul> <div id="download-button-info" hidden> View a PDF of the paper titled Interstrip Capacitances of the Readout Board used in Large Triple-GEM Detectors for the CMS Muon Upgrade, by M. 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[2009.09505] Interstrip Capacitances of the Readout Board used in Large Triple-GEM Detectors for the CMS Muon Upgrade