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A Search for Charged Excitation of Dark Matter with the KamLAND-Zen Detector
There are many theories where a dark matter particle is part of a multiplet with an electrically charged state. If WIMP dark matter (\(\chi^{0}\)) is accompanied by a charged excited state (\(\chi^{-}\)) separated by a small mass difference, it can form a stable bound state with a nucleus. In supers...
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Published in: | arXiv.org 2021-01 |
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Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Format: | Article |
Language: | English |
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Online Access: | Get full text |
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Summary: | There are many theories where a dark matter particle is part of a multiplet with an electrically charged state. If WIMP dark matter (\(\chi^{0}\)) is accompanied by a charged excited state (\(\chi^{-}\)) separated by a small mass difference, it can form a stable bound state with a nucleus. In supersymmetric models, the \(\chi^{0}\) and the \(\chi^{-}\) could be the neutralino and a charged slepton, such as the neutralino-stau degenerate model. The formation binding process is expected to result in an energy deposition of {\it O}(1--10 MeV), making it suitable for detection in large liquid scintillator detectors. We describe new constraints on the bound state formation with a xenon nucleus using the KamLAND-Zen 400 Phase-II dataset. In order to enlarge the searchable parameter space, all xenon isotopes in the detector were used. For a benchmark parameter set of \(m_{\chi^{0}} = 100\) GeV and \(\Delta m = 10\) MeV, this study sets the most stringent upper limits on the recombination cross section \(\langle\sigma v\rangle\) and the decay-width of \(\chi^{-}\) of \(2.0 \times 10^{-31}\) \({\rm cm^3/s}\) and \(1.1 \times 10^{-18}\) GeV, respectively (90\% confidence level). |
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ISSN: | 2331-8422 |