Inelastic dark matter

David Smith and Neal Weiner
Phys. Rev. D 64, 043502 – Published 12 July 2001
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Abstract

Many observations suggest that much of the matter of the universe is nonbaryonic. Recently, the DAMA NaI dark matter direct detection experiment reported an annual modulation in their event rate consistent with a WIMP relic. However, the Cryogenic Dark Matter Search (CDMS) Ge experiment excludes most of the region preferred by DAMA. We demonstrate that if the dark matter can only scatter by making a transition to a slightly heavier state (Δm100keV), the experiments are no longer in conflict. Moreover, differences in the energy spectrum of nuclear recoil events could distinguish such a scenario from the standard WIMP scenario. Finally, we discuss the sneutrino as a candidate for inelastic dark matter in supersymmetric theories.

  • Received 15 February 2001

DOI:https://doi.org/10.1103/PhysRevD.64.043502

©2001 American Physical Society

Authors & Affiliations

David Smith

  • Department of Physics, University of California, Berkeley, California 94720
  • Theoretical Physics Group, Ernest Orlando Lawrence Berkeley National Laboratory, University of California, Berkeley, California 94720

Neal Weiner

  • Department of Physics, University of Washington, Seattle, Washington 98195

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Vol. 64, Iss. 4 — 15 August 2001

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