Dipòsit Digital de la Universitat de Barcelona: Zenith angle distributions at Super-Kamiokande and SNO and the solution of the solar neutrino problem

<!DOCTYPE html> <html> <head> <title>Dipòsit Digital de la Universitat de Barcelona: Zenith angle distributions at Super-Kamiokande and SNO and the solution of the solar neutrino problem</title> <base href="https://diposit.ub.edu" /> <meta http-equiv="Content-Type" content="text/html; charset=UTF-8" /> <meta name="Generator" content="DSpace 5.8" /> <meta name="viewport" content="width=device-width, initial-scale=1.0"> <link rel="shortcut icon" href="/dspace/favicon.ico" type="image/x-icon"/> <link rel="stylesheet" href="/dspace/static/css/jquery-ui-1.10.3.custom/redmond/jquery-ui-1.10.3.custom.css" type="text/css" /> <link rel="stylesheet" href="/dspace/static/css/bootstrap/bootstrap.min.css" type="text/css" /> <link rel="stylesheet" href="/dspace/static/css/bootstrap/bootstrap-theme.min.css" type="text/css" /> <link rel="stylesheet" href="/dspace/static/css/bootstrap/dspace-theme.css" type="text/css" /> <link rel="search" type="application/opensearchdescription+xml" href="/dspace/open-search/description.xml" title="DSpace"/> <link rel="schema.DCTERMS" href="http://purl.org/dc/terms/" /> <link rel="schema.DC" href="http://purl.org/dc/elements/1.1/" /> <meta name="DC.creator" content="Gonz谩lez Garc铆a, Ma. Concepci贸n" xml:lang="cat" /> <meta name="DC.creator" content="Pe帽a Garay, Carlos" xml:lang="cat" /> <meta name="DC.creator" content="Smirnov, Alexei Yu" xml:lang="cat" /> <meta name="DCTERMS.dateAccepted" content="2010-05-06T12:33:47Z" scheme="DCTERMS.W3CDTF" /> <meta name="DCTERMS.available" content="2010-05-06T12:33:47Z" scheme="DCTERMS.W3CDTF" /> <meta name="DCTERMS.issued" content="2001" xml:lang="cat" scheme="DCTERMS.W3CDTF" /> <meta name="DC.identifier" content="0556-2821" xml:lang="cat" /> <meta name="DC.identifier" content="https://hdl.handle.net/2445/12510" scheme="DCTERMS.URI" /> <meta name="DCTERMS.abstract" content="We have performed a detailed study of the zenith angle dependence of the regeneration factor and distributions of events at SNO and SK for different solutions of the solar neutrino problem. In particular, we discuss the oscillatory behavior and the synchronization effect in the distribution for the LMA solution, the parametric peak for the LOW solution, etc. A physical interpretation of the effects is given. We suggest a new binning of events which emphasizes the distinctive features of the zenith angle distributions for the different solutions. We also find the correlations between the integrated day-night asymmetry and the rates of events in different zenith angle bins. The study of these correlations strengthens the identification power of the analysis." xml:lang="eng" /> <meta name="DCTERMS.extent" content="18 p." xml:lang="cat" /> <meta name="DC.format" content="application/pdf" xml:lang="eng" /> <meta name="DC.language" content="eng" xml:lang="eng" scheme="DCTERMS.RFC1766" /> <meta name="DC.publisher" content="The American Physical Society" xml:lang="eng" /> <meta name="DCTERMS.isFormatOf" content="Reproducci贸 digital del document publicat en format paper, proporcionada per PROLA i http://dx.doi.org/10.1103/PhysRevD.63.113004" xml:lang="cat" /> <meta name="DCTERMS.isPartOf" content="Physical Review D, 2001, vol. 63, n煤m. 11, p. 113004-1-113004-18" xml:lang="cat" /> <meta name="DC.relation" content="http://dx.doi.org/10.1103/PhysRevD.63.113004" scheme="DCTERMS.URI" /> <meta name="DC.rights" content="(c) The American Physical Society, 2001" xml:lang="eng" /> <meta name="DC.source" content="Articles publicats en revistes (F铆sica Qu脿ntica i Astrof铆sica)" /> <meta name="DC.subject" content="Neutrins solars" xml:lang="cat" /> <meta name="DC.subject" content="Part铆cules (F铆sica nuclear)" xml:lang="cat" /> <meta name="DC.subject" content="Astrof铆sica nuclear" xml:lang="cat" /> <meta name="DC.subject" content="Sistema solar" xml:lang="cat" /> <meta name="DC.subject" content="Solar neutrinos" xml:lang="eng" /> <meta name="DC.subject" content="Particles (Nuclear physics)" xml:lang="eng" /> <meta name="DC.subject" content="Nuclear astrophysics" xml:lang="eng" /> <meta name="DC.subject" content="Solar system" xml:lang="eng" /> <meta name="DC.title" content="Zenith angle distributions at Super-Kamiokande and SNO and the solution of the solar neutrino problem" xml:lang="eng" /> <meta name="DC.type" content="info:eu-repo/semantics/article" xml:lang="eng" /> <meta name="DC.type" content="info:eu-repo/semantics/publishedVersion" /> <meta name="DC.identifier" content="551553" xml:lang="cat" /> <meta name="DC.rights" content="info:eu-repo/semantics/openAccess" /> <meta name="citation_keywords" content="info:eu-repo/semantics/article; info:eu-repo/semantics/publishedVersion" /> <meta name="citation_title" content="Zenith angle distributions at Super-Kamiokande and SNO and the solution of the solar neutrino problem" /> <meta name="citation_issn" content="0556-2821" /> <meta name="citation_publisher" content="The American Physical Society" /> <meta name="citation_language" content="eng" /> <meta name="citation_author" content="Gonz谩lez Garc铆a, Ma. Concepci贸n" /> <meta name="citation_author" content="Pe帽a Garay, Carlos" /> <meta name="citation_author" content="Smirnov, Alexei Yu" /> <meta name="citation_pdf_url" content="https://diposit.ub.edu/dspace/bitstream/2445/12510/1/551553.pdf" /> <meta name="citation_date" content="2001" /> <meta name="citation_abstract_html_url" content="https://diposit.ub.edu/dspace/handle/2445/12510" /> <script type='text/javascript' src="/dspace/static/js/jquery/jquery-1.10.2.min.js"></script> <script type='text/javascript' src='/dspace/static/js/jquery/jquery-ui-1.10.3.custom.min.js'></script> <script type='text/javascript' src='/dspace/static/js/bootstrap/bootstrap.min.js'></script> <script type='text/javascript' src='/dspace/static/js/holder.js'></script> <script type="text/javascript" src="/dspace/utils.js"></script> <script type="text/javascript" src="/dspace/static/js/choice-support.js"> </script>  <script async src="https://www.googletagmanager.com/gtag/js?id=G-TTP469ZDVB"></script> <script> window.dataLayer = window.dataLayer || []; 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Concepci贸n</a><br /><a class="author"href="/dspace/browse?type=author&value=Pe%C3%B1a+Garay%2C+Carlos">Pe帽a Garay, Carlos</a><br /><a class="author"href="/dspace/browse?type=author&value=Smirnov%2C+Alexei+Yu">Smirnov, Alexei Yu</a></td></tr> <tr><td class="metadataFieldLabel">Keywords: </td><td class="metadataFieldValue">Neutrins solars<br />Part铆cules (F铆sica nuclear)<br />Astrof铆sica nuclear<br />Sistema solar<br />Solar neutrinos<br />Particles (Nuclear physics)<br />Nuclear astrophysics<br />Solar system</td></tr> <tr><td class="metadataFieldLabel">Issue Date: </td><td class="metadataFieldValue">2001</td></tr> <tr><td class="metadataFieldLabel">Publisher: </td><td class="metadataFieldValue">The American Physical Society</td></tr> <tr><td class="metadataFieldLabel">Abstract: </td><td class="metadataFieldValue">We have performed a detailed study of the zenith angle dependence of the regeneration factor and distributions of events at SNO and SK for different solutions of the solar neutrino problem. In particular, we discuss the oscillatory behavior and the synchronization effect in the distribution for the LMA solution, the parametric peak for the LOW solution, etc. A physical interpretation of the effects is given. We suggest a new binning of events which emphasizes the distinctive features of the zenith angle distributions for the different solutions. We also find the correlations between the integrated day-night asymmetry and the rates of events in different zenith angle bins. The study of these correlations strengthens the identification power of the analysis.</td></tr> <tr><td class="metadataFieldLabel">Note: </td><td class="metadataFieldValue">Reproducci贸 digital del document publicat en format paper, proporcionada per PROLA i http://dx.doi.org/10.1103/PhysRevD.63.113004</td></tr> <tr><td class="metadataFieldLabel">It is part of: </td><td class="metadataFieldValue">Physical Review D, 2001, vol. 63, n煤m. 11, p. 113004-1-113004-18</td></tr> <tr><td class="metadataFieldLabel">URI: </td><td class="metadataFieldValue"><a href="https://hdl.handle.net/2445/12510">https://hdl.handle.net/2445/12510</a></td></tr> <tr><td class="metadataFieldLabel">Related resource: </td><td class="metadataFieldValue"><a href="http://dx.doi.org/10.1103/PhysRevD.63.113004">http://dx.doi.org/10.1103/PhysRevD.63.113004</a></td></tr> <tr><td class="metadataFieldLabel">ISSN: </td><td class="metadataFieldValue">0556-2821</td></tr> <tr><td class="metadataFieldLabel">Appears in Collections:</td><td class="metadataFieldValue"><a href="/dspace/handle/2445/7504">Articles publicats en revistes (F铆sica Qu脿ntica i Astrof铆sica)</a><br/></td></tr> </table><br/> <div class="panel panel-info"><div class="panel-heading">Files in This Item:</div> <table class="table panel-body"><tr><th id="t1" class="standard">File</th> <th id="t2" class="standard">Description</th> <th id="t3" class="standard">Size</th><th id="t4" class="standard">Format</th><th> </th></tr> <tr><td headers="t1" class="standard"><a target="_blank" href="/dspace/bitstream/2445/12510/1/551553.pdf">551553.pdf</a></td><td headers="t2" class="standard"></td><td headers="t3" class="standard">558.92 kB</td><td headers="t4" class="standard">Adobe PDF</td><td class="standard" align="center"><a class="btn btn-primary" target="_blank" href="/dspace/bitstream/2445/12510/1/551553.pdf">View/Open</a></td></tr></table> </div> <div class="container row"> <a class="btn btn-default" href="/dspace/handle/2445/12510?mode=full"> Show full item record </a> </div> <br/> <br/> <p class="submitFormHelp alert alert-info"> Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.   </p> <div class="addthis_sharing_toolbox"></div> </div> </main> <footer class="navbar navbar-inverse navbar-bottom" style='background:-webkit-linear-gradient(#6685a9,#406086);background:-o-linear-gradient(#6685a9,#406086);background:-moz-linear-gradient(#6685a9,#406086);background:linear-gradient(#6685a9,#406086);border-radius:0;border:0;width:100%'> <div id="designedby" class="container text-muted">  <div id="footer_feedback" class="pull-left"> <p class="text-muted"> <span style='color:white'>Coordination: </span> <a style='color:#000' onMouseOver="this.style.color='#fff'" onMouseOut="this.style.color='#000'" target='_blank' href='http://crai.ub.edu/en'> CRAI Universitat de Barcelona</a>       <a style='color:#000' onMouseOver="this.style.color='#fff'" onMouseOut="this.style.color='#000'" target="_blank" href='http://www.ub.edu/web/ub/en/menu_peu/avislegal/avis_legal.html'>Legal notice</a> </p> </div> <div id="footer_feedback" class="pull-right"> <p class="text-muted"> <span style='color:white'>Metadata subject to: </span> <a target='_blank' href='http://creativecommons.org/publicdomain/zero/1.0/'> <img src="/dspace/image/logoCC.png" alt="Logo CC" /> </a>      <span style='color:white'>Powered by: </span> <a style='color:#000' onMouseOver="this.style.color='#fff'" onMouseOut="this.style.color='#000'" target="_blank" href="http://dspace.org/">DSpace</a>      <a style='color:#000' onMouseOver="this.style.color='#fff'" onMouseOut="this.style.color='#000'" target="_blank" href="/dspace/feedback">Contact us</a> </p> </div>  </div> </footer> </body> </html>

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Dipòsit Digital de la Universitat de Barcelona: Zenith angle distributions at Super-Kamiokande and SNO and the solution of the solar neutrino problem