<?xml version="1.0" encoding="UTF-8"?><rdf:RDF xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:dcq="http://purl.org/dc/terms/"><records count="1" morepages="false" start="1" end="1"><record rownumber="1"><dc:product_type>Journal Article</dc:product_type><dc:title>Search for charged excited states of dark matter with KamLAND-Zen</dc:title><dc:creator>Abe, S; Eizuka, M; Futagi, S; Gando, A; Gando, Y; Goto, S; Hachiya, T; Hata, K; Hosokawa, K; Ichimura, K; Ieki, S; Ikeda, H; Inoue, K; Ishidoshiro, K; Kamei, Y; Kawada, N; Kishimoto, Y; Koga, M; Kurasawa, M; Mitsui, T; Miyake, H; Morita, D; Nakahata, T; Nakajima, R; Nakamura, K; Nakamura, R; Nakamura, R; Nakane, J; Ozaki, H; Sakai, T; Shimizu, I; Shirai, J; Shiraishi, K; Shoji, R; Suzuki, A; Takeuchi, A; Tamae, K; Watanabe, H; Watanabe, K; Obara, S; Yoshida, S; Umehara, S; Fushimi, K; Kotera, K; Urano, Y; Ichikawa, A; Berger, BE; Fujikawa, BK; Learned, JG; Maricic, J; Axani, SN; Fu, Z; Smolsky, J; Winslow, LA; Efremenko, Y; Karwowski, HJ; Markoff, DM; Tornow, W; Dell'Oro, S; O'Donnell, T; Detwiler, JA; Enomoto, S; Decowski, MP; Weerman, KM; Grant, C; Li, A; Song, H</dc:creator><dc:corporate_author/><dc:editor/><dc:description>Particle dark matter could belong to a multiplet that includes an electrically charged state. WIMP dark matter (χ0) accompanied by a negatively charged excited state (χ−) with a small mass difference (e.g. &lt; 20 MeV) can form a bound-state with a nucleus such as xenon. This bound-state formation is rare and the released energy is O(1−10) MeV depending on the nucleus, making large liquid scintillator detectors suitable for detection. We searched for bound-state formation events with xenon in two experimental phases of the KamLAND-Zen experiment, a xenon-doped liquid scintillator detector. No statistically significant events were observed. For a benchmark parameter set of WIMP mass mχ0=1 TeV and mass difference Δm=17 MeV, we set the most stringent upper limits on the recombination cross section times velocity 〈σv〉 and the decay-width of χ− to 9.2×10−30cm3/s and 8.7×10−14 GeV, respectively at 90% confidence level.</dc:description><dc:publisher>Elsevier</dc:publisher><dc:date>2024-08-01</dc:date><dc:nsf_par_id>10530373</dc:nsf_par_id><dc:journal_name>Physics Letters B</dc:journal_name><dc:journal_volume>855</dc:journal_volume><dc:journal_issue>C</dc:journal_issue><dc:page_range_or_elocation>138846</dc:page_range_or_elocation><dc:issn>0370-2693</dc:issn><dc:isbn/><dc:doi>https://doi.org/10.1016/j.physletb.2024.138846</dc:doi><dcq:identifierAwardId>2110720; 2310130</dcq:identifierAwardId><dc:subject/><dc:version_number/><dc:location/><dc:rights/><dc:institution/><dc:sponsoring_org>National Science Foundation</dc:sponsoring_org></record></records></rdf:RDF>