Direct Dark Matter Searches with CDMS and XENON

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

appears in the proceedings of the 36th COSPAR Scientific Assembly in Beijing, July 2006

Scientific paper

10.1016/j.asr.2007.02.071

The Cryogenic Dark Matter Search (CDMS) and XENON experiments aim to directly detect dark matter in the form of weakly interacting massive particles (WIMPs) via their elastic scattering on the target nuclei. The experiments use different techniques to suppress background event rates to the minimum, and at the same time, to achieve a high WIMP detection rate. The operation of cryogenic Ge and Si crystals of the CDMS-II experiment in the Soudan mine yielded the most stringent spin-independent WIMP-nucleon cross-section (~10^{-43} cm^2) at a WIMP mass of 60 GeV/c^2. The two-phase xenon detector of the XENON10 experiment is currently taking data in the Gran Sasso underground lab and promising preliminary results were recently reported. Both experiments are expected to increase their WIMP sensitivity by a one order of magnitude in the scheduled science runs for 2007.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Direct Dark Matter Searches with CDMS and XENON does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Direct Dark Matter Searches with CDMS and XENON, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Direct Dark Matter Searches with CDMS and XENON will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-163399

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.