Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
9828036 | New Astronomy Reviews | 2005 | 4 Pages |
Abstract
In planned large dark matter experiments, a small population of nuclear recoils due to dark matter interactions will be difficult to distinguish from a possible residual background of neutron interactions or a low energy alpha background from U/Th in the containing vessel. Simulations are presented which demonstrate this ambiguity for small signals with Poisson fluctuations, and which show the feasibility of resolving this ambiguity in the case of spin-independent weak interactions by comparing signals from two or more target elements with a large difference in A2. Examples are shown for liquid Xe/Ar and gas mixture targets.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
Peter F. Smith,