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The Cryogenic Dark Matter Search (CDMS) employs low-temperature Ge and Si detectors to search for Weakly Interacting Massive Particles (WIMPs) via their elastic-scattering interactions with nuclei while discriminating against interactions…

天体物理学 · 物理学 2012-08-27 CDMS Collaboration

The Cryogenic Dark Matter Search (CDMS) is an experiment to detect weakly interacting massive particles (WIMPs) based on their interactions with Ge and Si nuclei. We report the results of an analysis of data from the first two runs of CDMS…

天体物理学 · 物理学 2012-08-27 CDMS Collaboration

The Cryogenic Dark Matter Search experiment (CDMS) employs low-temperature Ge and Si detectors to detect WIMPs via their elastic scattering interaction with the target nuclei. The current analysis of 397.8 kg-days Ge exposure resulted in…

天体物理学 · 物理学 2019-08-13 T. Bruch

Using improved Ge and Si detectors, better neutron shielding, and increased counting time, the Cryogenic Dark Matter Search (CDMS) experiment has obtained stricter limits on the cross section of weakly interacting massive particles (WIMPs)…

高能物理 - 实验 · 物理学 2012-08-27 CDMS Collaboration

The Cryogenic Dark Matter search experiment (CDMS) employs low-temperature Ge and Si detectors to detect WIMPs via their elastic scattering of target nuclei. The last analysis with an germanium exposure of 397.8 kg-days resulted in zero…

天体物理仪器与方法 · 物理学 2019-08-13 T. Bruch

The Cryogenic Dark Matter Search (CDMS-II) employs low-temperature Ge and Si detectors to seek Weakly Interacting Massive Particles (WIMPs) via their elastic scattering interactions with nuclei. Simultaneous measurements of both ionization…

天体物理学 · 物理学 2012-08-27 CDMS Collaboration

We are conducting an experiment to search for WIMPs, or weakly-interacting massive particles, in the galactic halo using terrestrial detectors. This generic class of hypothetical particles, whose properties are similar to those predicted by…

Astrophysical observations strongly suggest that non-luminous, nonbaryonic components, so called "Dark Matter", may constitute most of the matter in the Universe. The Cryogenic Dark Matter Search (CDMS) experiment is designed to detect Dark…

高能物理 - 实验 · 物理学 2019-08-13 Jonghee Yoo

We report the first results from a search for weakly interacting massive particles (WIMPs) in the Cryogenic Dark Matter Search (CDMS) experiment at the Soudan Underground Laboratory. Four Ge and two Si detectors were operated for 52.6 live…

天体物理学 · 物理学 2012-08-27 CDMS Collaboration

We report first results from the Cryogenic Dark Matter Search (CDMS II) experiment running with its full complement of 30 cryogenic particle detectors at the Soudan Underground Laboratory. This report is based on the analysis of data…

天体物理学 · 物理学 2012-08-27 CDMS Collaboration

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…

天体物理学 · 物理学 2008-11-26 Kaixuan Ni , Laura Baudis

We report results from a blind analysis of the final data taken with the Cryogenic Dark Matter Search experiment (CDMS II) at the Soudan Underground Laboratory, Minnesota, USA. A total raw exposure of 612 kg-days was analyzed for this work.…

宇宙学与河外天体物理 · 物理学 2014-11-20 The CDMS Collaboration , Z. Ahmed

We report new results from the Cryogenic Dark Matter Search (CDMS II) at the Soudan Underground Laboratory. Two towers, each consisting of six detectors, were operated for 74.5 live days, giving spectrum-weighted exposures of 34 kg-d for…

天体物理学 · 物理学 2012-08-27 CDMS Collaboration

We report the result of a blinded search for Weakly Interacting Massive Particles (WIMPs) using the majority of the SuperCDMS Soudan dataset. With an exposure of 1690 kg days, a single candidate event is observed, consistent with expected…

The Korea Invisible Mass Search(KIMS) experiment presents new limits on WIMP-nucleon cross section using the data from an exposure of 3409 kgd taken with low background CsI(Tl) crystals at Yangyang underground laboratory. The most stringent…

The CDMS II experiment uses Z-dependent Ionization Phonon (ZIP) detectors made of Germanium and Silicon to identify nuclear recoils from Weakly Interacting Massive Particles (WIMPs) with near complete event-by-event rejection of various…

天体物理学 · 物理学 2007-05-23 Samuel Leclercq

The Cryogenic Dark Matter Search experiment uses low-temperature solid-state detectors to seek Weakly Interacting Massive Particles (WIMPs) and has the world's best exclusion limit on the spin-independent WIMP-nucleon cross section. The…

高能物理 - 实验 · 物理学 2019-08-13 Oleg Kamaev

The EDELWEISS collaboration has performed a direct search for WIMP dark matter using a 320 g heat-and-ionization cryogenic Ge detector operated in a low-background environment in the Laboratoire Souterrain de Modane. No nuclear recoils are…

The SuperCDMS experiment is designed to directly detect weakly interacting massive particles (WIMPs) that may constitute the dark matter in our Galaxy. During its operation at the Soudan Underground Laboratory, germanium detectors were run…

宇宙学与河外天体物理 · 物理学 2018-01-24 SuperCDMS Collaboration , R. Agnese , A. J. Anderson , T. Aralis , T. Aramaki , I. J. Arnquist , W. Baker , D. Balakishiyeva , D. Barker , R. Basu Thakur , D. A. Bauer , T. Binder , M. A. Bowles , P. L. Brink , R. Bunker , B. Cabrera , D. O. Caldwell , R. Calkins , C. Cartaro , D. G. Cerdeno , Y. Chang , H. Chagani , Y. Chen , J. Cooley , B. Cornell , P. Cushman , M. Daal , P. C. F. Di Stefano , T. Doughty , L. Esteban , E. Fascione , E. Figueroa-Feliciano , M. Fritts , G. Gerbier , M. Ghaith , G. L. Godfrey , S. R. Golwala , J. Hall , H. R. Harris , Z. Hong , E. W. Hoppe , L. Hsu , M. E. Huber , V. Iyer , D. Jardin , A. Jastram , C. Jena , M. H. Kelsey , A. Kennedy , A. Kubik , N. A. Kurinsky , A. Leder , B. Loer , E. Lopez Asamar , P. Lukens , D. MacDonell , R. Mahapatra , V. Mandic , N. Mast , E. H. Miller , N. Mirabolfathi , R. A. Moffatt , B. Mohanty , J. D. Morales Mendoza , J. Nelson , J. L. Orrell , S. M. Oser , K. Page , W. A. Page , R. Partridge , M. Pepin , M. Penalver Martinez , A. Phipps , S. Poudel , M. Pyle , H. Qiu , W. Rau , P. Redl , A. Reisetter , T. Reynolds , A. Roberts , A. E. Robinson , H. E. Rogers , T. Saab , B. Sadoulet , J. Sander , K. Schneck , R. W. Schnee , S. Scorza , K. Senapati , B. Serfass , D. Speller , M. Stein , J. Street , H. A. Tanaka , D. Toback , R. Underwood , A. N. Villano , B. von Krosigk , B. Welliver , J. S. Wilson , M. J Wilson , D. H. Wright , S. Yellin , J. J. Yen , B. A. Young , X. Zhang , X. Zhao

The CDMS and EDELWEISS collaborations have combined the results of their direct searches for dark matter using cryogenic germanium detectors. The total data set represents 614 kg.d equivalent exposure. A straightforward method of…

宇宙学与河外天体物理 · 物理学 2015-03-19 CDMS , EDELWEISS Collaborations , : , Z. Ahmed , D. S. Akerib , E. Armengaud , S. Arrenberg , C. Augier , C. N. Bailey , D. Balakishiyeva , L. Baudis , D. A. Bauer , A. Benoît , L. Bergé , J. Blümer , P. L. Brink , A. Broniatowski , T. Bruch , V. Brudanin , R. Bunker , B. Cabrera , D. O. Caldwell , B. Censier , M. Chapellier , G. Chardin , F. Charlieux , J. Cooley , P. Coulter , G. A. Cox , P. Cushman , M. Daal , X. Defay , M. De Jesus , F. DeJongh , P. C. F. Di Stefano , Y. Dolgorouki , J. Domange , L. Dumoulin , M. R. Dragowsky , K. Eitel , S. Fallows , E. Figueroa-Feliciano , J. Filippini , D. Filosofov , N. Fourches , J. Fox , M. Fritts , J. Gascon , G. Gerbier , J. Gironnet , S. R. Golwala , M. Gros , J. Hall , R. Hennings-Yeomans , S. Henry , S. A. Hertel , S. Hervé , D. Holmgren , L. Hsu , M. E. Huber , A. Juillard , O. Kamaev , M. Kiveni , H. Kluck , M. Kos , V. Kozlov , H. Kraus , V. A. Kudryavtsev , S. W. Leman , S. Liu , P. Loaiza , R. Mahapatra , V. Mandic , S. Marnieros , C. Martinez , K. A. McCarthy , N. Mirabolfathi , D. Moore , P. Nadeau , X-F. Navick , H. Nelson , C. Nones , R. W. Ogburn , E. Olivieri , P. Pari , L. Pattavina , B. Paul , A. Phipps , M. Pyle , X. Qiu , W. Rau , A. Reisetter , Y. Ricci , M. Robinson , S. Rozov , T. Saab , B. Sadoulet , J. Sander , V. Sanglard , B. Schmidt , R. W. Schnee , S. Scorza , D. N. Seitz , S. Semikh , B. Serfass , K. M. Sundqvist , M. Tarka , A. S. Torrento-Coello , L. Vagneron , M. -A. Verdier , R. J. Walker , P. Wikus , E. Yakushev , S. Yellin , J. Yoo , B. A. Young , J. Zhang
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