<?xml version="1.0" encoding="UTF-8"?><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>2026-10-19T01:36:15Z</responseDate><request verb="GetRecord" identifier="oai:ebyu-rdlopen.rawdatalibrary.net:ebyu/15854" metadataPrefix="oai_dc">https://ebyu-rdlopen.rawdatalibrary.net/oai/request</request><GetRecord><record><header><identifier>oai:ebyu-rdlopen.rawdatalibrary.net:ebyu/15854</identifier><datestamp>2026-10-18T20:30:42Z</datestamp><setSpec>openaire</setSpec><setSpec>driver</setSpec><setSpec>com_ebyu_10000</setSpec><setSpec>col_ebyu_10001</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" 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 a W' or Techni-ρ decaying into WZ in pp collisions at √s=7TeV</dc:title><dc:creator>Chatrchyan, S.</dc:creator><dc:creator>Khachatryan, V.</dc:creator><dc:creator>Sirunyan, A.M.</dc:creator><dc:creator>Tumasyan, A.</dc:creator><dc:creator>Adam, W.</dc:creator><dc:creator>Aguilo, E.</dc:creator><dc:creator>Bergauer, T.</dc:creator><dc:creator>Dragicevic, M.</dc:creator><dc:creator>Erö, J.</dc:creator><dc:creator>Fabjan, C.</dc:creator><dc:creator>Friedl, M.</dc:creator><dc:creator>Frühwirth, R.</dc:creator><dc:creator>Ghete, V.M.</dc:creator><dc:creator>Hammer, J.</dc:creator><dc:creator>Hörmann, N.</dc:creator><dc:creator>Hrubec, J.</dc:creator><dc:creator>Jeitler, M.</dc:creator><dc:creator>Kiesenhofer, W.</dc:creator><dc:creator>Knünz, V.</dc:creator><dc:creator>Krammer, M.</dc:creator><dc:creator>Liko, D.</dc:creator><dc:creator>Mikulec, I.</dc:creator><dc:creator>Pernicka, M.</dc:creator><dc:creator>Rahbaran, B.</dc:creator><dc:creator>Rohringer, C.</dc:creator><dc:creator>Rohringer, H.</dc:creator><dc:creator>Schöfbeck, R.</dc:creator><dc:creator>Strauss, J.</dc:creator><dc:creator>Taurok, A.</dc:creator><dc:creator>Waltenberger, W.</dc:creator><dc:creator>Walzel, G.</dc:creator><dc:creator>Widl, E.</dc:creator><dc:creator>Wulz, C.-E.</dc:creator><dc:creator>Mossolov, V.</dc:creator><dc:creator>Shumeiko, N.</dc:creator><dc:creator>Suarez Gonzalez, J.</dc:creator><dc:creator>Bansal, S.</dc:creator><dc:creator>Cornelis, T.</dc:creator><dc:creator>De Wolf, E.A.</dc:creator><dc:creator>Janssen, X.</dc:creator><dc:creator>Luyckx, S.</dc:creator><dc:creator>Mucibello, L.</dc:creator><dc:creator>Ochesanu, S.</dc:creator><dc:creator>Roland, B.</dc:creator><dc:creator>Rougny, R.</dc:creator><dc:creator>Selvaggi, M.</dc:creator><dc:creator>Staykova, Z.</dc:creator><dc:creator>Van Haevermaet, H.</dc:creator><dc:creator>Van Mechelen, P.</dc:creator><dc:creator>Van Remortel, N.</dc:creator><dc:subject>Colliding beam accelerators</dc:subject><dc:subject>Confidence levels</dc:subject><dc:subject>Data sample</dc:subject><dc:subject>Exotic particles</dc:subject><dc:subject>Final state</dc:subject><dc:subject>Integrated luminosity</dc:subject><dc:subject>Production cross section</dc:subject><dc:subject>Standard model</dc:subject><dc:subject>Technicolour</dc:subject><dc:subject>Upper Bound</dc:subject><dc:subject>W bosons</dc:subject><dc:subject>Bosons</dc:subject><dc:description>A search is performed in pp collisions at √s=7TeV for exotic particles decaying via WZ to final states with electrons and muons. The data sample corresponds to an integrated luminosity of approximately 5fb -1. No significant excess is observed in the data above the expected standard model background. Upper bounds at 95% confidence level are set on the production cross section of the W′ boson described by the sequential standard model and on the W′ WZ coupling. W ′ bosons with masses below 1143 GeV are excluded. Limits are also set in the context of low-scale technicolor models, under a range of assumptions concerning the model parameters. © 2012 CERN.</dc:description><dc:publisher>American Physical Society</dc:publisher><dc:date>2012</dc:date><dc:type>Article</dc:type><dc:identifier>https://rdlopen.rawdatalibrary.net/r/ebyu/15854</dc:identifier><dc:identifier>https://doi.org/10.1103/physrevlett.109.141801</dc:identifier><dc:identifier>0031-9007</dc:identifier><dc:language>en</dc:language><dc:relation>Physical Review Letters</dc:relation><dc:rights>info:eu-repo/semantics/openAccess</dc:rights><dc:type>info:eu-repo/semantics/article</dc:type><dc:identifier>https://ebyu-rdlopen.rawdatalibrary.net/tr/items/ebyu/15854</dc:identifier></oai_dc:dc></metadata></record></GetRecord></OAI-PMH>