Search for Axions with the CDMS Experiment (2009)
Ahmed, Z., Akerib, D. S., Arrenberg, S., Bailey, C. N., Balakishiyeva, D., Baudis, L., ...
We report on the first axion search results from the Cryogenic Dark Matter Search (CDMS) experiment at the Soudan Underground Laboratory. An energy threshold of 2 keV for electron-recoil events...
Analysis of the low-energy electron-recoil spectrum of the CDMS experiment (2009)
Ahmed, Z., Akerib, D. S., Arrenberg, S., Bailey, C. N., Balakishiyeva, D., Baudis, L., ...
We report on the analysis of the low-energy electron-recoil spectrum from the CDMS II experiment using data with an exposure of 443.2 kg-days. The analysis provides details on the observed counting...
D.S. Akerib · C.N. Bailey · P.P. Brusov · M.R. Dragowsky · D.R. Grant · R. Hennings-Yeomans · (2009)
Z. Ahmed, D. S. Akerib, M. J. Attisha, C. N. Bailey, L. Baudis, D. A. Bauer, ...
Abstract The Cryogenic Dark Matter Search experiment (CDMS) is using Phonon+ Ionization detectors to search for Dark Matter in the form of Weakly Interactive Massive Particles (WIMPs). We report the...
WIMP EXCLUSION RESULTS FROM THE CDMS EXPERIMENT (2009)
P. L. Brink, L. Baudis, B. Cabrera, J. P. Castle, C. Chang, T. Saab, ...
In early 2000 CDMS set the most competitive exclusion limit for scalarinteraction WIMPs at the Stanford Underground Facility (SUF). A new search (CDMS II) is now commencing at the Deep-site Soudan...
Deep Underground Science and Engineering Lab: Dark Matter Working Group 2007 White Paper (2009)
Akerib, D. S., Gaitskell, R. J.
This whitepaper is the result of discussions and presentations initiated at the DUSEL Town Meeting held in Washington in November 2007. The essential elements of this report are: - The quest to...
Ahmed, Z., Akerib, D. S., Arrenberg, S., Attisha, M. J., Bailey, C. N., Baudis, L., ...
We report results from the Cryogenic Dark Matter Search at the Soudan Underground Laboratory (CDMS II) featuring the full complement of 30 detectors. A blind analysis of data taken between October...
A Testing Strategy for the Mass Production of CDMS II Detectors (2008)
D. Driscoll, D. S. Akerib, D. Abrams, D. Bauer, P. L. Brink, B. Cabrera, ...
Abstract. The Cryogenic Dark Matter Search (CDMS) employs detectors which are capable of simultaneously measuring the ionization and phonon energies deposited by a particle collision. These detectors...
T. Saab, P. L. Brink, L. Baudis, B. Cabrera, J. P. Castle, C. Chang, ...
The CDMS II experiment deployed a set of 6 ZIP (Z-dependent Ionization and Phonon) detectors at the Stanford Underground Facility (SUF) shallow depth site in the fall of 2001. With a payload...
RESULTS AND STATUS OF THE CRYOGENIC DARK MATTER SEARCH (CDMS) (2008)
R. W. Schnee, D. S. Akerib, A. Bolodyzynya, T. A. Perera, P. D. Barnes, D. A. Bauer, ...
The Cryogenic Dark Matter Search experiment uses cooled germanium and silicon detectors for a direct search for weakly-interacting massive particles in our Galaxy. The novel detectors allow a high...
R. W. Schnee, R. Abusaidi, D. S. Akerib, D. A. Bauer, A. Bolozdynya, P. L. Brink, ...
J.P. Castle 8, R.M. Clarke 8, P. Colling 8, M.B. Crisler 2, A. Cummings 9 A. Da Silva
Hunting for WIMPs with the Cryogenic Dark Matter Search (2007)
Golwala Akerib Barnes, S. R. Golwala, D. S. Akerib, P. D. Barnes, D. A. Bauer, A. Bolozdynya, ...
. The Cryogenic Dark Matter Search #CDMS# is an experiment whose goal is to detect WIMPs via elastic-scattering interactions in detectors capable of nuclear-recoil discrimination. Recent advances in...
Center For, R. J. Gaitskell, P. D. Barnes, A. Dasilva, S. R. Golwala, J. Jochum, ...
this paper) , and a 100 g Si FLIP detector (which are discussed elsewhere in these (a)
A Testing Strategy for the Mass Production of CDMS II Detectors (2007)
D. Driscoll, D. S. Akerib, D. Abrams, D. Bauer, P. L. Brink, B. Cabrera, ...
, V. Mandic, P. Meunier
RESULTS AND STATUS OF THE CRYOGENIC DARK MATTER SEARCH (CDMS) (2007)
R. W. Schnee, D. S. Akerib, A. Bolodyzynya, T. A. Perera, P. D. Barnes, D. A. Bauer, ...
The Cryogenic Dark Matter Search experiment uses cooled germanium and silicon detectors for a direct search for weakly-interacting massive particles in our Galaxy. The novel detectors allow a high...
Status and Results from the Cryogenic Dark Matter (2007)
Search Cdms Gaitskell, Castle Ringberg, R J Gaitskell, D S Akerib, P D Barnes, D Bauer, ...
The Cryogenic Dark Matter Search (CDMS) experiment utilizes novel cryogenic particle detectors for a direct search of dark matter particles in the form of WIMPs in our galaxy. The detectors are able...
Present Results and Future Goals of the (2007)
Cryogenic Dark Matter, T. A. Perera, D. Abrams, D. S. Akerib, D. A. Bauer, A. Bolozdynya, ...
The Cryogenic Dark Matter Search (CDMS) uses Ge and Si detectors to search for Weakly Interacting Massive Particles (WIMPs) via their elastic-scattering interaction with atomic nuclei. The present...
Results and Status of the Cryogenic Dark Matter Search (CDMS) (2007)
Schnee Akerib, R. W. Schnee, D. S. Akerib, P. D. Barnes, D. A. Bauer, P. L. Brink, ...
The Cryogenic Dark Matter Search experiment uses cooled germanium and silicon detectors for a direct search for weakly-interacting massive particles in our Galaxy. The novel detectors allow a high...
Hennings-Yeomans, R., Akerib, D. S.
We present the design of an instrument capable of measuring the high energy ($>$60 MeV) muon-induced neutron flux deep underground. The instrument is based on applying the Gd-loaded...
Deep Underground Science and Engineering Lab: S1 Dark Matter Working Group (2006)
Akerib, D. S., Aprile, E., Baltz, E. A., Dragowsky, M. R., Gaitskell, R. J., Gondolo, P., ...
A study of the current status of WIMP dark matter searches has been made in the context of scientific and technical planning for a Deep Underground Science and Engineering Laboratory (DUSEL) in the...
Beyond the CDMS-II Dark Matter Search: SuperCDMS (2005)
Brink, P. L., Cabrera, B., Chang, C. L., Cooley, J., Ogburn, R. W., Akerib, D. S., ...
Presently the CDMS-II collaboration's Weakly Interacting Massive Particle (WIMP) search at the Soudan Underground Laboratory sets the most stringent exclusion limits of any WIMP cold dark matter...
Exclusion limits on the WIMP-nucleon cross section from the Cryogenic Dark Matter Search (2002)
Abrams, D., Akerib, D. S., Armel-Funkhouser, M. S., Baudis, L., Bauer, D. A., Bolozdynya, A., ...
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...
Expected Performance of CryoArray (2002)
Schnee, R. W., Akerib, D. S., Gaitskell, R. J.
WIMP-nucleon cross sections below 10^(-9) pb may be probed by ton-scale experiments with low thresholds and background rates ~20 events per year. An array of cryogenic detectors ("CryoArray") could...
Exclusion limits on the WIMP-nucleon cross section from the Cryogenic Dark Matter Search (2000)
Abusaidi, R., Akerib, D. S., Bauer, D. A., Bolozdynya, A., Brink, P. L., ...
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...
Upper Limit on the Decay K+ --> e+ nu mu+ mu- (1998)
Atiya, M. S., Chiang, I-H., Frank, J. S., Haggerty, J. S., Kycia, T. F., ...
An upper limit on the branching ratio for the decay K+ --> e+ nu mu+ mu- is set at 5.0 x 10^{-7} at 90% confidence level, consistent with predictions from chiral perturbation theory.
Observation of the Decay K^+ --> pi^+ gamma gamma (1997)
Nakano, T., Rozon, M., Soluk, R., Adler, S., Atiya, M. S., ...
The first observation of the decay K^+ --> pi^+ gamma gamma is reported. A total of 31 events was observed with an estimated background of 5.1 +- 3.3 events in the pi+ momentum range from 100 MeV/c...
Observation of the Decay K+ --> pi+ mu+ mu- (1997)
Atiya, M. S., Chiang, I-H., Frank, J. S., Haggerty, J. S., Kycia, T. F., ...
We have observed the rare decay K+ --> pi+ mu+ mu- and measured the branching ratio Gamma(K+ --> pi+ mu+ mu-)/Gamma(K+ --> all) = (5.0 +/- 0.4 (stat.) +/- 0.7 (sys.) +/- 0.6 (theor.)) x 10^{-8}. We...
Search for the Decay $K^+ \to \pi^+ \nu \overline{\nu}$ (1995)
Adler, S., Atiya, M. S., Chiang, I-H., Frank, J. S., Haggerty, J. S., Kycia, T. F., ...
An upper limit on the branching ratio for the decay $K^+ \! \rightarrow \! \pi^+ \nu \overline{\nu}$ is set at $2.4 \times 10^{-9}$ at the 90\% C.L. using pions in the kinematic region $214~{\rm...