<?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>2026-10-18T23:15:01Z</responseDate><request verb="GetRecord" identifier="oai:ebyu-rdlopen.rawdatalibrary.net:ebyu/12092" metadataPrefix="oai_dc">https://ebyu-rdlopen.rawdatalibrary.net/oai/request</request><GetRecord><record><header><identifier>oai:ebyu-rdlopen.rawdatalibrary.net:ebyu/12092</identifier><datestamp>2026-10-18T20:27:02Z</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 electroweak production of charginos and neutralinos at s=13TeV in final states containing hadronic decays of WW, WZ, or WH and missing transverse momentum</dc:title><dc:creator>Tumasyan, A.</dc:creator><dc:creator>Adam, W.</dc:creator><dc:creator>Andrejkovic, J.W.</dc:creator><dc:creator>Bergauer, T.</dc:creator><dc:creator>Chatterjee, S.</dc:creator><dc:creator>Damanakis, K.</dc:creator><dc:creator>Dragicevic, M.</dc:creator><dc:creator>Escalante Del Valle, A.</dc:creator><dc:creator>Frühwirth, R.</dc:creator><dc:creator>Jeitler, M.</dc:creator><dc:creator>Krammer, N.</dc:creator><dc:creator>Lechner, L.</dc:creator><dc:creator>Liko, D.</dc:creator><dc:creator>Mikulec, I.</dc:creator><dc:creator>Paulitsch, P.</dc:creator><dc:creator>Pitters, F.M.</dc:creator><dc:creator>Schieck, J.</dc:creator><dc:creator>Schöfbeck, R.</dc:creator><dc:creator>Schwarz, D.</dc:creator><dc:creator>Templ, S.</dc:creator><dc:creator>Waltenberger, W.</dc:creator><dc:creator>Wulz, C.-E.</dc:creator><dc:creator>Darwish, M.R.</dc:creator><dc:creator>De Wolf, E.A.</dc:creator><dc:creator>Janssen, T.</dc:creator><dc:creator>Kello, T.</dc:creator><dc:creator>Lelek, A.</dc:creator><dc:creator>Rejeb Sfar, H.</dc:creator><dc:creator>Van Mechelen, P.</dc:creator><dc:creator>Van Putte, S.</dc:creator><dc:creator>Van Remortel, N.</dc:creator><dc:creator>Bols, E.S.</dc:creator><dc:creator>D'Hondt, J.</dc:creator><dc:creator>Delcourt, M.</dc:creator><dc:creator>El Faham, H.</dc:creator><dc:creator>Lowette, S.</dc:creator><dc:creator>Moortgat, S.</dc:creator><dc:creator>Morton, A.</dc:creator><dc:creator>Müller, D.</dc:creator><dc:creator>Sahasransu, A.R.</dc:creator><dc:creator>Tavernier, S.</dc:creator><dc:creator>Van Doninck, W.</dc:creator><dc:creator>Vannerom, D.</dc:creator><dc:creator>Beghin, D.</dc:creator><dc:creator>Bilin, B.</dc:creator><dc:creator>Clerbaux, B.</dc:creator><dc:creator>De Lentdecker, G.</dc:creator><dc:creator>Favart, L.</dc:creator><dc:creator>Kalsi, A.K.</dc:creator><dc:creator>Lee, K.</dc:creator><dc:subject>CMS</dc:subject><dc:subject>Electroweakino</dc:subject><dc:subject>Gaugino</dc:subject><dc:subject>Supersymmetry</dc:subject><dc:description>This Letter presents a search for direct production of charginos and neutralinos via electroweak interactions. The results are based on data from proton-proton collisions at a center-of-mass energy of 13 TeV collected with the CMS detector at the LHC, corresponding to an integrated luminosity of 137 fb−1. The search considers final states with large missing transverse momentum and pairs of hadronically decaying bosons WW, WZ, and WH, where H is the Higgs boson. These bosons are identified using novel algorithms. No significant excess of events is observed relative to the expectations from the standard model. Limits at the 95% confidence level are placed on the cross section for production of mass-degenerate wino-like supersymmetric particles χ˜1                         ± and χ˜2                         0, and mass-degenerate higgsino-like supersymmetric particles χ˜1                         ±, χ˜2                         0, and χ˜3                         0. In the limit of a nearly-massless lightest supersymmetric particle χ˜1                         0, wino-like particles with masses up to 870 and 960 GeV are excluded in the cases of χ˜2                         0→Zχ˜1                         0 and χ˜2                         0→Hχ˜1                         0, respectively, and higgsino-like particles are excluded between 300 and 650 GeV. © 2022 The Author(s)</dc:description><dc:publisher>Elsevier B.V.</dc:publisher><dc:date>2023</dc:date><dc:type>Article</dc:type><dc:identifier>https://rdlopen.rawdatalibrary.net/r/ebyu/12092</dc:identifier><dc:identifier>https://doi.org/10.1016/j.physletb.2022.137460</dc:identifier><dc:identifier>0370-2693</dc:identifier><dc:language>en</dc:language><dc:relation>Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics</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/12092</dc:identifier></oai_dc:dc></metadata></record></GetRecord></OAI-PMH>