Inelastic dark matter at DAMA, CDMS and future experiments

David Smith, Neal Weiner

    Research output: Contribution to journalArticle

    Abstract

    The DAMA annual modulation signature, interpreted as evidence for a spin-independent WIMP coupling, seems in conflict with null results from CDMS. However, in models of "inelastic dark matter", the experiments are compatible. Inelastic dark matter can arise in supersymmetric theories as the real component of a sneutrino mixed with a singlet scalar. In contrast with ordinary sneutrino dark matter, such particles can satisfy all experimental constraints while giving the appropriate relic abundance. We discuss the modifications to the signal seen at DAMA, in particular noting the strong suppression of low energy events in both modulated and unmodulated components. We discuss future experiments, with emphasis on distinguishing inelastic dark matter from ordinary dark matter, and stressing the significance of experiments with heavy target nuclei, such as xenon and tungsten.

    Original languageEnglish (US)
    Pages (from-to)197-200
    Number of pages4
    JournalNuclear Physics B - Proceedings Supplements
    Volume124
    DOIs
    StatePublished - Jul 2003

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    dark matter
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    ASJC Scopus subject areas

    • Nuclear and High Energy Physics

    Cite this

    Inelastic dark matter at DAMA, CDMS and future experiments. / Smith, David; Weiner, Neal.

    In: Nuclear Physics B - Proceedings Supplements, Vol. 124, 07.2003, p. 197-200.

    Research output: Contribution to journalArticle

    Smith, David ; Weiner, Neal. / Inelastic dark matter at DAMA, CDMS and future experiments. In: Nuclear Physics B - Proceedings Supplements. 2003 ; Vol. 124. pp. 197-200.
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