Physics Letters B (Aug 2024)

Search for charged excited states of dark matter with KamLAND-Zen

  • S. Abe,
  • M. Eizuka,
  • S. Futagi,
  • A. Gando,
  • Y. Gando,
  • S. Goto,
  • T. Hachiya,
  • K. Hata,
  • K. Hosokawa,
  • K. Ichimura,
  • S. Ieki,
  • H. Ikeda,
  • K. Inoue,
  • K. Ishidoshiro,
  • Y. Kamei,
  • N. Kawada,
  • Y. Kishimoto,
  • M. Koga,
  • M. Kurasawa,
  • T. Mitsui,
  • H. Miyake,
  • D. Morita,
  • T. Nakahata,
  • R. Nakajima,
  • K. Nakamura,
  • R. Nakamura,
  • R. Nakamura,
  • J. Nakane,
  • H. Ozaki,
  • T. Sakai,
  • I. Shimizu,
  • J. Shirai,
  • K. Shiraishi,
  • R. Shoji,
  • A. Suzuki,
  • A. Takeuchi,
  • K. Tamae,
  • H. Watanabe,
  • K. Watanabe,
  • S. Obara,
  • S. Yoshida,
  • S. Umehara,
  • K. Fushimi,
  • K. Kotera,
  • Y. Urano,
  • A. Ichikawa,
  • B.E. Berger,
  • B.K. Fujikawa,
  • J.G. Learned,
  • J. Maricic,
  • S.N. Axani,
  • Z. Fu,
  • J. Smolsky,
  • L.A. Winslow,
  • Y. Efremenko,
  • H.J. Karwowski,
  • D.M. Markoff,
  • W. Tornow,
  • S. Dell'Oro,
  • T. O'Donnell,
  • J.A. Detwiler,
  • S. Enomoto,
  • M.P. Decowski,
  • K.M. Weerman,
  • C. Grant,
  • A. Li,
  • H. Song

Journal volume & issue
Vol. 855
p. 138846

Abstract

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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. < 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 9.2×10−30 cm3/s and 8.7×10−14 GeV, respectively at 90% confidence level.

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