PIRSA:09060041

Dark Matter Search with CDMS and SuperCDMS

Rau, W. (2009). Dark Matter Search with CDMS and SuperCDMS. Perimeter Institute. https://pirsa.org/09060041

Rau, Wolfgang. Dark Matter Search with CDMS and SuperCDMS. Perimeter Institute, Jun. 12, 2009, https://pirsa.org/09060041 

          @misc{ pirsa_PIRSA:09060041,
            doi = {10.48660/09060041},
            url = {https://pirsa.org/09060041},
            author = {Rau, Wolfgang},
            keywords = {Particle Physics, Cosmology},
            language = {en},
            title = {Dark Matter Search with CDMS and SuperCDMS},
            publisher = {Perimeter Institute},
            year = {2009},
            month = {jun},
            note = {PIRSA:09060041 see, \url{https://pirsa.org}}
          }

Wolfgang Rau

Queen's University

Talk number
PIRSA:09060041
Collection
Talk Type
Subject
Abstract
The Cryogenic Dark Matter Search (CDMS) experiment employs cryogenic ionization detectors to search for nuclear recoils induced by Weakly Interacting assive dark matter particles (WIMPs). A fast readout of the thermal energy deposition and the simultaneous measurement of an ionization signal provide an excellent handle for rejection of electron recoil background events from environmental radiation. This unique technology together with passive and active shielding makes CDMS the only background free experiment in the field. The recently published data based on the full complement of 30 individual detector modules operated in the Soudan Underground Laboratory in Minnesota give the best sensitivity for spin-independent WIMP-nucleon scattering for the most interesting mass range above about 40 GeV/c². The experiment is in a transition to the next phase, SuperCDMS, with increased total target mass and larger individual detector modules with improved sensor technology. SuperCDMS plans to install a total of 100-200 kg of cryogenic germanium detectors in the new SNOLAB facility near Sudbury ON, which, as the deepest large underground laboratory, provides the best conditions for direct dark matter search experiments.