Signal yields, energy resolution, and recombination fluctuations in liquid xenon
PHYSICAL REVIEW D
Akerib, D. S., Alsum, S., Araujo, H. M., Bai, X., Bailey, A. J., Balajthy, J., Beltrame, P., Bernard, E. P., Bernstein, A., Biesiadzinski, T. P., Boulton, E. M., Bramante, R., BRAS, P., Byram, D., Cahn, S. B., Carmona-Benitez, M. C., Chan, C., Chiller, A. A., Chiller, C., Currie, A., Cutter, J. E., Davison, T. J., Dobi, A., Dobson, J. E., Druszkiewicz, E., Edwards, B. N., Faham, C. H., Fiorucci, S., Gaitskell, R. J., Gehman, V. M., Ghag, C., Gibson, K. R., Gilchriese, M. G., Hall, C. R., Hanhardt, M., Haselschwardt, S. J., Hertel, S. A., Hogan, D. P., Horn, M., Huang, D. Q., Ignarra, C. M., Ihm, M., Jacobsen, R. G., Ji, W., Kamdin, K., Kazkaz, K., Khaitan, D., Knoche, R., Larsen, N. A., Lee, C., Lenardo, B. G., Lesko, K. T., Lindote, A., Lopes, M. I., Manalaysay, A., Mannino, R. L., Marzioni, M. F., McKinsey, D. N., Mei, D., Mock, J., Moongweluwan, M., Morad, J. A., Murphy, A. S., NEHRKORN, C., Nelson, H. N., Neves, F., O'Sullivan, K., Oliver-Mallory, K. C., Palladino, K. J., Pease, E. K., Phelps, P., Reichhart, L., Rhyne, C., Shaw, S., Shutt, T. A., SILVA, C., Solmaz, M., Solovov, V. N., Sorensen, P., Stephenson, S., Sumner, T. J., Szydagis, M., Taylor, D. J., Taylor, W. C., Tennyson, B. P., Terman, P. A., Tiedt, D. R., TO, W. H., Tripathi, M., Tvrznikova, L., Uvarov, S., Verbus, J. R., Webb, R. C., White, J. T., Whitis, T. J., Witherell, M. S., Wolfs, F. L., Xu, J., Yazdani, K., Young, S. K., Zhang, C.
2017; 95 (1)
Results from a Search for Dark Matter in the Complete LUX Exposure
PHYSICAL REVIEW LETTERS
Akerib, D. S., Alsum, S., Araujo, H. M., Bai, X., Bailey, A. J., Balajthy, J., Beltrame, P., Bernard, E. P., Bernstein, A., Biesiadzinski, T. P., Boulton, E. M., Bramante, R., BRAS, P., Byram, D., Cahn, S. B., Carmona-Benitez, M. C., Chan, C., Chiller, A. A., Chiller, C., Currie, A., Cutter, J. E., Davison, T. J., Dobi, A., Dobson, J. E., Druszkiewicz, E., Edwards, B. N., Faham, C. H., Fiorucci, S., Gaitskell, R. J., Gehman, V. M., Ghag, C., Gibson, K. R., Gilchriese, M. G., Hall, C. R., Hanhardt, M., Haselschwardt, S. J., Hertel, S. A., Hogan, D. P., Horn, M., Huang, D. Q., Ignarra, C. M., Ihm, M., Jacobsen, R. G., Ji, W., Kamdin, K., Kazkaz, K., Khaitan, D., Knoche, R., Larsen, N. A., Lee, C., Lenardo, B. G., Lesko, K. T., Lindote, A., Lopes, M. I., Manalaysay, A., Mannino, R. L., Marzioni, M. F., McKinsey, D. N., Mei, D., Mock, J., Moongweluwan, M., Morad, J. A., Murphy, A. S., NEHRKORN, C., Nelson, H. N., Neves, F., O'Sullivan, K., Oliver-Mallory, K. C., Palladino, K. J., Pease, E. K., Phelps, P., Reichhart, L., Rhyne, C., Shaw, S., Shutt, T. A., SILVA, C., Solmaz, M., Solovov, V. N., Sorensen, P., Stephenson, S., Sumner, T. J., Szydagis, M., Taylor, D. J., Taylor, W. C., Tennyson, B. P., Terman, P. A., Tiedt, D. R., TO, W. H., Tripathi, M., Tvrznikova, L., Uvarov, S., Verbus, J. R., Webb, R. C., White, J. T., Whitis, T. J., Witherell, M. S., Wolfs, F. L., Xu, J., Yazdani, K., Young, S. K., Zhang, C.
2017; 118 (2)
Abstract
We report constraints on spin-independent weakly interacting massive particle (WIMP)-nucleon scattering using a 3.35×10^{4} kg day exposure of the Large Underground Xenon (LUX) experiment. A dual-phase xenon time projection chamber with 250 kg of active mass is operated at the Sanford Underground Research Facility under Lead, South Dakota (USA). With roughly fourfold improvement in sensitivity for high WIMP masses relative to our previous results, this search yields no evidence of WIMP nuclear recoils. At a WIMP mass of 50 GeV c^{-2}, WIMP-nucleon spin-independent cross sections above 2.2×10^{-46} cm^{2} are excluded at the 90% confidence level. When combined with the previously reported LUX exposure, this exclusion strengthens to 1.1×10^{-46} cm^{2} at 50 GeV c^{-2}.
View details for DOI 10.1103/PhysRevLett.118.021303
View details for Web of Science ID 000391926900002
View details for PubMedID 28128598
REVIEW OF PARTICLE PHYSICS Particle Data Group
CHINESE PHYSICS C
Patrignani, C., Agashe, K., Aielli, G., Amsler, C., Antonelli, M., Asner, D. M., Baer, H., Banerjee, S., Barnett, R. M., Basaglia, T., Bauer, C. W., Beatty, J. J., Belousov, V. I., Beringer, J., Bethke, S., Bichsel, H., Biebel, O., Blucher, E., Brooijmans, G., Buchmueller, O., Burkert, V., Bychkov, M. A., Cahn, R. N., Carena, M., Ceccucci, A., Cerri, A., Chakraborty, D., Chen, M., Chivukula, R. S., Copic, K., Cowan, G., Dahl, O., D'Ambrosio, G., Damour, T., de Florian, D., de Gouvea, A., DeGrand, T., de Jong, P., Dissertori, G., Dobrescu, B. A., D'onofrio, M., Doser, M., Drees, M., Dreiner, H. K., Dwyer, D. A., Eerola, P., Eidelman, S., Ellis, J., Erler, J., Ezhela, V. V., Fetscher, W., Fields, B. D., Foster, B., FREITAS, A., Gallagher, H., Garren, L., Gerber, H., Gerbier, G., Gershon, T., Gherghetta, T., Godizov, A. A., Goodman, M., Grab, C., Gritsan, A. V., Grojean, C., Groom, D. E., Gruenewald, M., Gurtu, A., Gutsche, T., Haber, H. E., Hagiwara, K., Hanhart, C., Hashimoto, S., Hayato, Y., Hayes, K. G., Hebecker, A., Heltsley, B., Hernandez-Rey, J. J., Hikasa, K., Hisano, J., Hoecker, A., Holder, J., Holtkamp, A., Huston, J., Hyodo, T., Irwin, K., Jackson, J. D., Johnson, K. F., Kado, M., Karliner, M., Katz, U. F., Klein, S. R., Klempt, E., Kowalewski, R. V., Krauss, F., Kreps, M., Krusche, B., Kuyanov, Y. V., Kwon, Y., Lahav, O., Laiho, J., Langacker, P., Liddle, A., Ligeti, Z., Lin, C., Lippmann, C., Liss, T. M., Littenberg, L., Lugovsky, K. S., Lugovsky, S. B., Lusiani, A., Makida, Y., Maltoni, F., Mannel, T., Manohar, A. V., Marciano, W. J., Martin, A. D., Masoni, A., Matthews, J., Meissner, U., Milstead, D., Mitchell, R. E., Molaro, P., Monig, K., Moortgat, F., Mortonson, M. J., Murayama, H., Nakamura, K., Narain, M., Nason, P., Navas, S., Neubert, M., Nevski, P., Nir, Y., Olive, K. A., Griso, S. P., Parsons, J., Peacock, J. A., Pennington, M., Petcov, S. T., Petrov, V. A., Piepke, A., Pomarol, A., Quadt, A., Raby, S., Rademacker, J., Raffelt, G., Ratcliff, B. N., Richardson, P., Ringwald, A., Roesler, S., Rolli, S., Romaniouk, A., Rosenberg, L. J., Rosner, J. L., Rybka, G., Ryutin, R. A., Sachrajda, C. T., Sakai, Y., Salam, G. P., Sarkar, S., Sauli, F., Schneider, O., Scholberg, K., Schwartz, A. J., Scott, D., Sharma, V., Sharpe, S. R., Shutt, T., Silari, M., Sjostrand, T., Skands, P., Skwarnicki, T., Smith, J. G., Smoot, G. F., Spanier, S., Spieler, H., Spiering, C., Stahl, A., Stone, S. L., Sumino, Y., Sumiyoshi, T., Syphers, M. J., Takahashi, F., Tanabashi, M., Terashi, K., Terning, J., Thorne, R. S., Tiator, L., Titov, M., Tkachenko, N. P., Tornqvist, N. A., Tovey, D., Valencia, G., Van de Water, R., Varelas, N., Venanzoni, G., Vincter, M. G., Vogel, P., Vogt, A., Wakely, S. P., Walkowiak, W., Walter, C. W., Wands, D., Ward, D. R., Wascko, M. O., Weiglein, G., Weinberg, D. H., Weinberg, E. J., White, M., Wiencke, L. R., Wiliocq, S., Wohl, C. C., Wolfenstein, L., Womersley, J., Woody, C. L., Workman, R. L., Yao, W., Zeller, G. P., Zenin, O. V., Zhu, R., Zimmermann, F., Zyla, P. A., Anderson, J., Harper, G., Lugovsky, V. S., Schaffner, P.
2016; 40 (10)
FPGA-based trigger system for the LUX dark matter experiment
NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT
Akerib, D. S., Araujo, H. M., Bai, X., Bailey, A. J., Balajthy, J., Beltrame, P., Bernard, E. P., Bernstein, A., Biesiadzinski, T. P., Boulton, E. M., Bradley, A., Bramante, R., Cahn, S. B., Carmona-Benitez, M. C., Chan, C., Chapman, J. J., Chiller, A. A., Chiller, C., Currie, A., Cutter, J. E., Davison, T. J., de Viveiros, L., Dobi, A., Dobson, J. E., Druszkiewicz, E., Edwards, B. N., Faham, C. H., Fiorucci, S., Gaitskell, R. J., Gehmang, V. M., Ghag, C., Gibson, K. R., Gilchriese, M. G., Hall, C. R., Hanhardt, M., Haselschwardt, S. J., Herter, S. A., Hogan, D. P., Horn, M., Huang, D. Q., Ignarra, C. M., Ihm, M., Jacobsen, R. G., Ji, W., Kazkaz, K., Khaitang, D., Knoche, R., Larsen, N. A., Lee, C., Lenardo, B. G., Lesko, K. T., Lindote, A., Lopes, M. I., Mailing, D. C., Manalaysay, A. G., Mannino, R. L., Marzioni, M. F., McKinsey, D. N., Mei, D., Mock, J., Moongweluwan, M., Morad, J. A., Murphy, A. S., NEHRKORN, C., Nelson, H. N., Neves, E., O'Sullivan, K., Oliver-Mallory, K. C., Ott, R. A., Palladino, K. J., Pangilinan, M., Pease, E. K., Phelps, P., Reichhart, L., Rhyne, C., Shaw, S., Shutt, T. A., SILVA, C., Skulski, W., Solovovn, V. N., Sorensen, P., Stephenson, S., Sumner, T. J., Szydagis, M., Taylor, D. J., Taylor, W., Tennyson, B. P., Terman, P. A., Tiedt, D. R., TO, W. H., Tripathi, M., Tyrznikova, L., Uvarov, S., Verbus, J. R., Webb, R. C., White, J. T., Whitis, T. J., Witherell, M. S., Wolfs, F. L., Yin, J., Young, S. K., Zhang, C.
2016; 818: 57-67
Tritium calibration of the LUX dark matter experiment
PHYSICAL REVIEW D
Akerib, D. S., Araujo, H. M., Bai, X., Bailey, A. J., Balajthy, J., Beltrame, P., Bernard, E. P., Bernstein, A., Biesiadzinski, T. P., Boulton, E. M., Bradley, A., Bramante, R., Cahn, S. B., Carmona-Benitez, M. C., Chan, C., Chapman, J. J., Chiller, A. A., Chiller, C., Currie, A., Cutter, J. E., Davison, T. J., de Viveiros, L., Dobi, A., Dobson, J. E., Druszkiewicz, E., Edwards, B. N., Faham, C. H., Fiorucci, S., Gaitskell, R. J., Gehman, V. M., Ghag, C., Gibson, K. R., Gilchriese, M. G., Hall, C. R., Hanhardt, M., Haselschwardt, S. J., Hertel, S. A., Hogan, D. P., Horn, M., Huang, D. Q., Ignarra, C. M., Ihm, M., Jacobsen, R. G., Ji, W., Kazkaz, K., Khaitan, D., Knoche, R., Larsen, N. A., Lee, C., Lenardo, B. G., Lesko, K. T., Lindote, A., Lopes, M. I., Malling, D. C., Manalaysay, A. G., Mannino, R. L., Marzioni, M. F., McKinsey, D. N., Mei, D., Mock, J., Moongweluwan, M., Morad, J. A., Murphy, A. S., NEHRKORN, C., Nelson, H. N., Neves, F., O'Sullivan, K., Oliver-Mallory, K. C., Ott, R. A., Palladino, K. J., Pangilinan, M., Pease, E. K., Phelps, P., Reichhart, L., Rhyne, C., Shaw, S., Shutt, T. A., SILVA, C., Solovov, V. N., Sorensen, P., Stephenson, S., Sumner, T. J., Szydagis, M., Taylor, D. J., Taylor, W., Tennyson, B. P., Terman, P. A., Tiedt, D. R., TO, W. H., Tripathi, M., Tvrznikova, L., Uvarov, S., Verbus, J. R., Webb, R. C., White, J. T., Whitis, T. J., Witherell, M. S., Wolfs, F. L., Young, S. K., Zhang, C.
2016; 93 (7)
Improved Limits on Scattering of Weakly Interacting Massive Particles from Reanalysis of 2013 LUX Data
PHYSICAL REVIEW LETTERS
Akerib, D. S., Araujo, H. M., Bai, X., Bailey, A. J., Balajthy, J., Beltrame, P., Bernard, E. P., Bernstein, A., Biesiadzinski, T. P., Boulton, E. M., Bradley, A., Bramante, R., Cahn, S. B., Carmona-Benitez, M. C., Chan, C., Chapman, J. J., Chiller, A. A., Chiller, C., Currie, A., Cutter, J. E., Davison, T. J., de Viveiros, L., Dobi, A., Dobson, J. E., Druszkiewicz, E., Edwards, B. N., Faham, C. H., Fiorucci, S., Gaitskell, R. J., Gehman, V. M., Ghag, C., Gibson, K. R., Gilchriese, M. G., Hall, C. R., Hanhardt, M., Haselschwardt, S. J., Hertel, S. A., Hogan, D. P., Horn, M., Huang, D. Q., Ignarra, C. M., Ihm, M., Jacobsen, R. G., Ji, W., Kazkaz, K., Khaitan, D., Knoche, R., Larsen, N. A., Lee, C., Lenardo, B. G., Lesko, K. T., Lindote, A., Lopes, M. I., Malling, D. C., Manalaysay, A., Mannino, R. L., Marzioni, M. F., McKinsey, D. N., Mei, D., Mock, J., Moongweluwan, M., Morad, J. A., Murphy, A. S., NEHRKORN, C., Nelson, H. N., Neves, F., O'Sullivan, K., Oliver-Mallory, K. C., Ott, R. A., Palladino, K. J., Pangilinan, M., Pease, E. K., Phelps, P., Reichhart, L., Rhyne, C., Shaw, S., Shutt, T. A., SILVA, C., Solovov, V. N., Sorensen, P., Stephenson, S., Sumner, T. J., Szydagis, M., Taylor, D. J., Taylor, W., Tennyson, B. P., Terman, P. A., Tiedt, D. R., TO, W. H., Tripathi, M., Tvrznikova, L., Uvarov, S., Verbus, J. R., Webb, R. C., White, J. T., Whitis, T. J., Witherell, M. S., Wolfs, F. L., Yazdani, K., Young, S. K., Zhang, C.
2016; 116 (16)
Abstract
We present constraints on weakly interacting massive particles (WIMP)-nucleus scattering from the 2013 data of the Large Underground Xenon dark matter experiment, including 1.4×10^{4} kg day of search exposure. This new analysis incorporates several advances: single-photon calibration at the scintillation wavelength, improved event-reconstruction algorithms, a revised background model including events originating on the detector walls in an enlarged fiducial volume, and new calibrations from decays of an injected tritium β source and from kinematically constrained nuclear recoils down to 1.1 keV. Sensitivity, especially to low-mass WIMPs, is enhanced compared to our previous results which modeled the signal only above a 3 keV minimum energy. Under standard dark matter halo assumptions and in the mass range above 4 GeV c^{-2}, these new results give the most stringent direct limits on the spin-independent WIMP-nucleon cross section. The 90% C.L. upper limit has a minimum of 0.6 zb at 33 GeV c^{-2} WIMP mass.
View details for DOI 10.1103/PhysRevLett.116.161301
View details for Web of Science ID 000374559300003
View details for PubMedID 27152785
Results on the Spin-Dependent Scattering of Weakly Interacting Massive Particles on Nucleons from the Run 3 Data of the LUX Experiment
PHYSICAL REVIEW LETTERS
Akerib, D. S., Araujo, H. M., Bai, X., Bailey, A. J., Balajthy, J., Beltrame, P., Bernard, E. P., Bernstein, A., Biesiadzinski, T. P., Boulton, E. M., Bradley, A., Bramante, R., Cahn, S. B., Carmona-Benitez, M. C., Chan, C., Chapman, J. J., Chiller, A. A., Chiller, C., Currie, A., Cutter, J. E., Davison, T. J., de Viveiros, L., Dobi, A., Dobson, J. E., Druszkiewicz, E., Edwards, B. N., Faham, C. H., Fiorucci, S., Gaitskell, R. J., Gehman, V. M., Ghag, C., Gibson, K. R., Gilchriese, M. G., Hall, C. R., Hanhardt, M., Haselschwardt, S. J., Hertel, S. A., Hogan, D. P., Horn, M., Huang, D. Q., Ignarra, C. M., Ihm, M., Jacobsen, R. G., Ji, W., Kazkaz, K., Khaitan, D., Knoche, R., Larsen, N. A., Lee, C., Lenardo, B. G., Lesko, K. T., Lindote, A., Lopes, M. I., Malling, D. C., Manalaysay, A., Mannino, R. L., Marzioni, M. F., McKinsey, D. N., Mei, D., Mock, J., Moongweluwan, M., Morad, J. A., Murphy, A. S., NEHRKORN, C., Nelson, H. N., Neves, F., O'Sullivan, K., Oliver-Mallory, K. C., Ott, R. A., Palladino, K. J., Pangilinan, M., Pease, E. K., Phelps, P., Reichhart, L., Rhyne, C., Shaw, S., Shutt, T. A., SILVA, C., Solovov, V. N., Sorensen, P., Stephenson, S., Sumner, T. J., Szydagis, M., Taylor, D. J., Taylor, W., Tennyson, B. P., Terman, P. A., Tiedt, D. R., TO, W. H., Tripathi, M., Tvrznikova, L., Uvarov, S., Verbus, J. R., Webb, R. C., White, J. T., Whitis, T. J., Witherell, M. S., Wolfs, F. L., Yazdani, K., Young, S. K., Zhang, C.
2016; 116 (16)
Abstract
We present experimental constraints on the spin-dependent WIMP (weakly interacting massive particle)-nucleon elastic cross sections from LUX data acquired in 2013. LUX is a dual-phase xenon time projection chamber operating at the Sanford Underground Research Facility (Lead, South Dakota), which is designed to observe the recoil signature of galactic WIMPs scattering from xenon nuclei. A profile likelihood ratio analysis of 1.4×10^{4} kg day of fiducial exposure allows 90% C.L. upper limits to be set on the WIMP-neutron (WIMP-proton) cross section of σ_{n}=9.4×10^{-41} cm^{2} (σ_{p}=2.9×10^{-39} cm^{2}) at 33 GeV/c^{2}. The spin-dependent WIMP-neutron limit is the most sensitive constraint to date.
View details for DOI 10.1103/PhysRevLett.116.161302
View details for Web of Science ID 000374559300004
View details for PubMedID 27152786
Low-threshold analysis of CDMS shallow-site data
PHYSICAL REVIEW D
Akerib, D. S., Attisha, M. J., Baudis, L., Bauer, D. A., Bolozdynya, A. I., Brink, P. L., Bunker, R., Cabrera, B., Caldwell, D. O., Chang, C. L., Clarke, R. M., Cooley, J., Crisler, M. B., Cushman, P., DeJongh, F., Dixon, R., Driscoll, D. D., Filippini, J., FUNKHOUSER, S., Gaitskell, R. J., Golwala, S. R., Holmgren, D., Hsu, L., Huber, M. E., Kamat, S., Mahapatra, R., Mandic, V., Meunier, P., Mirabolfathi, N., Moore, D., Nam, S. W., Nelson, H., Ogburn, R. W., Qiu, X., Rau, W., Reisetter, A., Saab, T., Sadoulet, B., Sander, J., Savage, C., Schnee, R. W., Seitz, D. N., Shutt, T. A., Wang, G., Yellin, S., Yoo, J., Young, B. A.
2010; 82 (12)
Design and performance of a modular low-radioactivity readout system for cryogenic detectors in the CDMS experiment
NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT
Akerib, D. S., Barnes, P. D., Brink, P. L., Cabrera, B., Clarke, R. M., Gaitskell, R. J., Golwala, S. R., Huber, M. E., Kurylowicz, M., Mandic, V., Martinis, J. M., Meunier, P., Mirabolfathi, N., Nam, S. W., Perillo-Isaac, M., Saab, T., Sadoulet, B., Schnee, R. W., Seitz, D. N., Shutt, T., Smith, G. W., Stockwell, W. K., Sundqvist, K. M., White, S.
2008; 591 (3): 476-489
New results from the Cryogenic Dark Matter Search experiment
PHYSICAL REVIEW D
Akerib, D. S., Alvaro-Dean, J., Armel, M. S., Attisha, M. J., Baudis, L., Bauer, D. A., Bolozdynya, A. I., Brink, P. L., Bunker, R., Cabrera, B., Caldwell, D. O., Castle, J. P., Chang, C. L., Clarke, R. M., Crisler, M. B., Cushman, P., Davies, A. K., Dixon, R., Driscoll, D. D., Duong, L., Emes, J., Ferril, R., Gaitskell, R. J., Golwala, S. R., Haldeman, M., Hellmig, J., Hennessey, M., Holmgren, D., Huber, M. E., Kamat, S., Kurylowicz, M., Lu, A., Mahapatra, R., Mandic, V., Martinis, J. M., Meunier, P., Mirabolfathi, N., Nam, S. W., Nelson, H., Nelson, R., Ogburn, R. W., Perales, J., Perera, T. A., Isaac, M. C., Rau, W., Reisetter, A., Ross, R. R., Saab, T., Sadoulet, B., Sander, J., Savage, C., Schnee, R. W., Seitz, D. N., Shutt, T. A., Smith, G., Spadafora, A. L., Thompson, J. P., Tomada, A., Wang, G., Yellin, S., Young, B. A.
2003; 68 (8)
Exclusion limits on the WIMP-nucleon cross section from the cryogenic dark matter search
PHYSICAL REVIEW D
Abrams, D., Akerib, D. S., Armel-Funkhouser, M. S., Baudis, L., Bauer, D. A., Bolozdynya, A., Brink, P. L., Bunker, R., Cabrera, B., Caldwell, D. O., Castle, J. P., Chang, C. L., Clarke, R. M., Crisler, M. B., Dixon, R., Driscoll, D., Eichblatt, S., Gaitskell, R. J., Golwala, S. R., Haller, E. E., Hellmig, J., Holmgren, D., Huber, M. E., Kamat, S., Lu, A., Mandic, V., Martinis, J. M., Meunier, P., Nam, S. W., Nelson, H., Perera, T. A., Isaac, M. C., Rau, W., Ross, R. R., Saab, T., Sadoulet, B., Sander, J., Schnee, R. W., Shutt, T., Smith, A., Sonnenschein, A. H., Spadafora, A. L., Wang, G., Yellin, S., Young, B. A.
2002; 66 (12)
Exclusion limits on the WIMP-nucleon cross section from the Cryogenic Dark Matter Search
PHYSICAL REVIEW LETTERS
Abusaidi, R., Akerib, D. S., Barnes, P. D., Bauer, D. A., Bolozdynya, A., Brink, P. L., Bunker, R., Cabrera, B., Caldwell, D. O., Castle, J. P., Clarke, R. M., Colling, P., Crisler, M. B., Cummings, A., Silva, A. D., Davies, A. K., Dixon, R., Dougherty, B. L., Driscoll, D., Eichblatt, S., Emes, J., Gaitskell, R. J., Golwala, S. R., Hale, D., Haller, E. E., Hellmig, J., Huber, M. E., Irwin, K. D., Jochum, J., Lipschultz, F. P., Lu, A., Mandic, V., Martinis, J. M., Nam, S. W., Nelson, H., Neuhauser, B., Penn, M. J., Perera, T. A., Isaac, M. C., Pritychenko, B., Ross, R. R., Saab, T., Sadoulet, B., Schnee, R. W., Seitz, D. N., Shestople, P., Shutt, T., Smith, A., Smith, G. W., Sonnenschein, A. H., Spadafora, A. L., Stockwell, W., Taylor, J. D., White, S.
2000; 84 (25): 5699-5703
Abstract
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/c2 WIMP mass and, at >75% C.L., the entire 3sigma allowed region for the WIMP signal reported by the DAMA experiment.
View details for PubMedID 10991035
