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Related papers: Constraints on Light WIMPs from SuperCDMS

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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…

Cosmology and Nongalactic Astrophysics · Physics 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

We report a first search for weakly interacting massive particles (WIMPs) using the background rejection capabilities of SuperCDMS. An exposure of 577 kg-days was analyzed for WIMPs with mass < 30 GeV/c2, with the signal region blinded.…

The CDMS low ionization threshold experiment (CDMSlite) uses cryogenic germanium detectors operated at a relatively high bias voltage to amplify the phonon signal in the search for weakly interacting massive particles (WIMPs). Results are…

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…

Instrumentation and Methods for Astrophysics · Physics 2019-08-13 T. Bruch

WIMP-nucleon cross sections in the range 10^{-46} - 10^{-44} cm^2 may be probed by a ton-scale experiment with low energy thresholds and excellent discrimination of backgrounds. Because CDMS ZIP detectors are the most proven means of…

Astrophysics · Physics 2012-08-27 SuperCDMS Collaboration

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)…

High Energy Physics - Experiment · Physics 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…

We report results from a reanalysis of data from the Cryogenic Dark Matter Search (CDMS II) experiment at the Soudan Underground Laboratory. Data taken between October 2006 and September 2008 using eight germanium detectors are reanalyzed…

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…

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…

Astrophysics · Physics 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…

Astrophysics · Physics 2019-08-13 T. Bruch

We report on the results of a search for a Weakly Interacting Massive Particle (WIMP) signal in low-energy data of the Cryogenic Dark Matter Search (CDMS~II) experiment using a maximum likelihood analysis. A background model is constructed…

Bosonic superweakly interacting massive particles (super-WIMPs) are a candidate for warm dark matter. With the absorption of such a boson by a xenon atom these dark matter candidates would deposit an energy equivalent to their rest mass in…

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…

Astrophysics · Physics 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…

Astrophysics · Physics 2008-11-26 Kaixuan Ni , Laura Baudis

Experiments seeking to detect rare event interactions such as dark matter or coherent elastic neutrino nucleus scattering are striving for large mass detectors with very low detection threshold. Using Neganov-Luke phonon amplification…

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…

Cosmology and Nongalactic Astrophysics · Physics 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

We study the accuracy with which the WIMP mass could be determined by a superCDMS-like direct detection experiment, given optimistic assumptions about the detector set-up and WIMP properties. We consider WIMPs with an interaction…

High Energy Physics - Phenomenology · Physics 2008-11-26 Anne M Green

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…

Astrophysics · Physics 2007-05-23 Samuel Leclercq
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