<?xml version="1.0" encoding="UTF-8"?><?xml-stylesheet type="text/xsl" href="static/style.xsl"?><OAI-PMH xmlns="http://www.openarchives.org/OAI/2.0/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/ http://www.openarchives.org/OAI/2.0/OAI-PMH.xsd"><responseDate>2026-04-19T16:17:51Z</responseDate><request verb="GetRecord" identifier="oai:www.recercat.cat:2445/140643" metadataPrefix="oai_dc">https://recercat.cat/oai/request</request><GetRecord><record><header><identifier>oai:recercat.cat:2445/140643</identifier><datestamp>2025-12-05T16:43:35Z</datestamp><setSpec>com_2072_1057</setSpec><setSpec>col_2072_478823</setSpec><setSpec>col_2072_478917</setSpec></header><metadata><oai_dc:dc xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:doc="http://www.lyncode.com/xoai" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
   <dc:title>Search for Strange-Pentaquark Production in e+e− Annihilation at √s=10.58 GeVc</dc:title>
   <dc:creator>Graugés Pous, Eugeni</dc:creator>
   <dc:creator>BABAR Collaboration</dc:creator>
   <dc:subject>Física de partícules</dc:subject>
   <dc:subject>Experiments</dc:subject>
   <dc:subject>Particle physics</dc:subject>
   <dc:subject>Experiments</dc:subject>
   <dc:description>We search for strange-pentaquark states that have been previously reported by other experiments the Θ ( 1540 ) + , Ξ 5 ( 1860 ) −− , and Ξ 5 ( 1860 ) 0  in 123     fb − 1 of data recorded with the BABAR detector at the PEP-II e + e − storage ring. We find no evidence for these states and set 95% confidence level upper limits on the number of Θ ( 1540 ) + and Ξ 5 ( 1860 ) −− pentaquarks produced per e + e − annihilation into q ¯ q and per Υ ( 4 S ) decay. For q ¯ q events the Θ ( 1540 ) + [ Ξ 5 ( 1860 ) −− ] limit is about 8 [4] times lower than the rates measured for ordinary baryons of similar mass.</dc:description>
   <dc:date>2019-09-20T11:22:50Z</dc:date>
   <dc:date>2019-09-20T11:22:50Z</dc:date>
   <dc:date>2005-07-21</dc:date>
   <dc:date>2019-09-20T11:22:50Z</dc:date>
   <dc:type>info:eu-repo/semantics/article</dc:type>
   <dc:type>info:eu-repo/semantics/publishedVersion</dc:type>
   <dc:identifier>0031-9007</dc:identifier>
   <dc:identifier>https://hdl.handle.net/2445/140643</dc:identifier>
   <dc:identifier>539087</dc:identifier>
   <dc:language>eng</dc:language>
   <dc:relation>Reproducció del document publicat a: https://doi.org/10.1103/PhysRevLett.95.042002</dc:relation>
   <dc:relation>Physical Review Letters, 2005, vol. 95, num. 4, p. 042002</dc:relation>
   <dc:relation>https://doi.org/10.1103/PhysRevLett.95.042002</dc:relation>
   <dc:rights>(c) American Physical Society, 2005</dc:rights>
   <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
   <dc:format>7 p.</dc:format>
   <dc:format>application/pdf</dc:format>
   <dc:publisher>American Physical Society</dc:publisher>
   <dc:source>Articles publicats en revistes (Física Quàntica i Astrofísica)</dc:source>
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