Status of the Search for Supersymmetric Dark Matter

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dc.creatorCline, David B.
dc.date2003-06-05
dc.date.accessioned2026-07-07T02:08:43Z
dc.date.available2026-07-07T02:08:43Z
dc.descriptionWe assume the supersymmetric model for dark matter in the universe and our galaxy, and direct methods to distinguish these kinds of dark matter are described. We then focus on the current and future experiment search for SUSY-WIMPS. Theoretical models suggest that a new generation of at least one ton detectors may be required to observe this form of dark matter. We concentrate on Liquid Xenon detectors because they can be scaled to large mass.
dc.description10 pages, 8 figures, invited talk at the SUGRA 20 Meeting, Boston, MA 2003
dc.identifierhttps://arxiv.org/abs/astro-ph/0306124
dc.identifierhttp://arxiv.org/abs/astro-ph/0306124
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6163
dc.subjectAstrophysics
dc.titleStatus of the Search for Supersymmetric Dark Matter
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