We briefly review the latest evidence for non-baryonic dark matter in the Universe, including cosmological constants. We also review the most recent estimates for SUSY dark matter particle interaction with matter. We then provide a critique of the current search for the dark matter with various detectors and describe one very promising method using powerful background discrimination in liquid xenon.

Topics
Cosmological constant, Dark matter, Chemical elements
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© 1998 American Institute of Physics.
1998
American Institute of Physics
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