The Cryogenic Dark Matter Search (CDMS) employs Ge and Si detectors to search for weakly interacting massive particles (WIMPs) via their elastic-scattering interactions with nuclei while discriminating against interactions of background particles. CDMS data, accounting for the neutron background, give limits on the spin-independent WIMP-nucleon elastic-scattering cross section that exclude unexplored parameter space above 10 GeV/c^2 WIMP mass and, at >75% C.L., the entire 3σ allowed region for the WIMP signal reported by the DAMA experiment
The Cryogenic Dark Matter Search (CDMS) has pioneered the use of ionization and athermal phonon sign...
The Cryogenic Dark Matter Search experiment uses germanium and silicon detectors cooled to cryogenic...
The Cryogenic Dark Matter Search (CDMS-II) experiment, at Soudan Underground Laboratory, used germa...
The Cryogenic Dark Matter Search (CDMS) employs Ge and Si detectors to search for weakly interacting...
The Cryogenic Dark Matter Search (CDMS) employs low-temperature Ge and Si detectors to search for we...
The Cryogenic Dark Matter Search (CDMS) seeks to directly detect the scattering of weakly interactin...
Using improved Ge and Si detectors, better neutron shielding, and increased counting time, the Cryog...
The Cryogenic Dark Matter Search (CDMS-II) employs low-temperature Ge and Si detectors to seek Weakl...
We are conducting an experiment to search for WIMPs, or weakly-interacting massive particles, in the...
The Cryogenic Dark Matter Search (CDMS-II) experiment, at Soudan Underground Laboratory, used germa...
The Cryogenic Dark Matter Search (CDMS-II) experiment, at Soudan Underground Laboratory, used germa...
The Cryogenic Dark Matter Search (CDMS) is an experiment to detect weakly interacting massive parti...
The Cryogenic Dark Matter Search (CDMS) is an experiment to detect weakly interacting massive parti...
The CDMS II experiment uses Z-dependent Ionization Phonon (ZIP) detectors made of Germanium and Sili...
Astrophysical observations indicate that dark matter constitutes most of the mass in our universe, b...
The Cryogenic Dark Matter Search (CDMS) has pioneered the use of ionization and athermal phonon sign...
The Cryogenic Dark Matter Search experiment uses germanium and silicon detectors cooled to cryogenic...
The Cryogenic Dark Matter Search (CDMS-II) experiment, at Soudan Underground Laboratory, used germa...
The Cryogenic Dark Matter Search (CDMS) employs Ge and Si detectors to search for weakly interacting...
The Cryogenic Dark Matter Search (CDMS) employs low-temperature Ge and Si detectors to search for we...
The Cryogenic Dark Matter Search (CDMS) seeks to directly detect the scattering of weakly interactin...
Using improved Ge and Si detectors, better neutron shielding, and increased counting time, the Cryog...
The Cryogenic Dark Matter Search (CDMS-II) employs low-temperature Ge and Si detectors to seek Weakl...
We are conducting an experiment to search for WIMPs, or weakly-interacting massive particles, in the...
The Cryogenic Dark Matter Search (CDMS-II) experiment, at Soudan Underground Laboratory, used germa...
The Cryogenic Dark Matter Search (CDMS-II) experiment, at Soudan Underground Laboratory, used germa...
The Cryogenic Dark Matter Search (CDMS) is an experiment to detect weakly interacting massive parti...
The Cryogenic Dark Matter Search (CDMS) is an experiment to detect weakly interacting massive parti...
The CDMS II experiment uses Z-dependent Ionization Phonon (ZIP) detectors made of Germanium and Sili...
Astrophysical observations indicate that dark matter constitutes most of the mass in our universe, b...
The Cryogenic Dark Matter Search (CDMS) has pioneered the use of ionization and athermal phonon sign...
The Cryogenic Dark Matter Search experiment uses germanium and silicon detectors cooled to cryogenic...
The Cryogenic Dark Matter Search (CDMS-II) experiment, at Soudan Underground Laboratory, used germa...