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We report the results of a search for inelastic scattering of weakly interacting massive particles (WIMPs) off $^{127}$I nuclei using NaI(Tl) crystals with a data exposure of 97.7 kg$\cdot$years from the COSINE-100 experiment. The signature…

We use the results of direct and indirect searches for weakly interacting massive particles (WIMPs) to obtain bounds on various electro-magnetic form factors of WIMPs. The limits on the recoil signal in underground dark matter detection…

High Energy Physics - Phenomenology · Physics 2009-10-31 Maxim Pospelov , Tonnis ter Veldhuis

The XENON100 experiment is the second phase of the XENON program for the direct detection of the dark matter in the universe. The XENON100 detector is a two-phase Time Projection Chamber filled with 161 kg of ultra pure liquid xenon. The…

Cosmology and Nongalactic Astrophysics · Physics 2019-08-13 S. E. A. Orrigo

We study the structure factors for spin-independent WIMP scattering off xenon based on state-of-the-art large-scale shell-model calculations, which are shown to yield a good spectroscopic description of all experimentally relevant isotopes.…

Nuclear Theory · Physics 2015-02-20 L. Vietze , P. Klos , J. Menéndez , W. C. Haxton , A. Schwenk

In a recent presentation at the TAUP97 conference about the analysis of data from a NaI(Tl) 100 kg underground detector run at the Gran Sasso Laboratory by the DAMA/NaI group, the speaker concluded there was a hint for a WIMP of mass 60 GeV…

Astrophysics · Physics 2007-05-23 G. Gerbier , J. Mallet , L. Mosca , C. Tao

Data are presented from the DRIFT-IId detector housed in the Boulby mine in northeast England. A 0.8 m^3 fiducial volume, containing partial pressures of 30 Torr CS2 and 10 Torr CF4, was exposed for a duration of 47.4 live-time days with…

The design and performance of the LUX-ZEPLIN (LZ) detector is described as of March 2015 in this Conceptual Design Report. LZ is a second-generation dark-matter detector with the potential for unprecedented sensitivity to weakly interacting…

Instrumentation and Detectors · Physics 2015-10-05 The LZ Collaboration , D. S. Akerib , C. W. Akerlof , D. Yu. Akimov , S. K. Alsum , H. M. Araújo , X. Bai , A. J. Bailey , J. Balajthy , S. Balashov , M. J. Barry , P. Bauer , P. Beltrame , E. P. Bernard , A. Bernstein , T. P. Biesiadzinski , K. E. Boast , A. I. Bolozdynya , E. M. Boulton , R. Bramante , J. H. Buckley , V. V. Bugaev , R. Bunker , S. Burdin , J. K. Busenitz , C. Carels , D. L. Carlsmith , B. Carlson , M. C. Carmona-Benitez , M. Cascella , C. Chan , J. J. Cherwinka , A. A. Chiller , C. Chiller , W. W. Craddock , A. Currie , J. E. Cutter , J. P. da Cunha , C. E. Dahl , S. Dasu , T. J. R. Davison , L. de Viveiros , A. Dobi , J. E. Y. Dobson , E. Druszkiewicz , T. K. Edberg , B. N. Edwards , W. R. Edwards , M. M. Elnimr , W. T. Emmet , C. H. Faham , S. Fiorucci , P. Ford , V. B. Francis , C. Fu , R. J. Gaitskell , N. J. Gantos , V. M. Gehman , R. M. Gerhard , C. Ghag , M. G. D. Gilchriese , B. Gomber , C. R. Hall , A. Harris , S. J. Haselschwardt , S. A. Hertel , M. D. Hoff , B. Holbrook , E. Holtom , D. Q. Huang , T. W. Hurteau , C. M. Ignarra , R. G. Jacobsen , W. Ji , X. Ji , M. Johnson , Y. Ju , K. Kamdin , K. Kazkaz , D. Khaitan , A. Khazov , A. V. Khromov , A. M. Konovalov , E. V. Korolkova , H. Kraus , H. J. Krebs , V. A. Kudryavtsev , A. V. Kumpan , S. Kyre , N. A. Larsen , C. Lee , B. G. Lenardo , K. T. Lesko , F. -T. Liao , J. Lin , A. Lindote , W. H. Lippincott , J. Liu , X. Liu , M. I. Lopes , W. Lorenzon , S. Luitz , P. Majewski , D. C. Malling , A. G. Manalaysay , L. Manenti , R. L. Mannino , D. J. Markley , T. J. Martin , M. F. Marzioni , D. N. McKinsey , D. -M. Mei , Y. Meng , E. H. Miller , J. Mock , M. E. Monzani , J. A. Morad , A. St. J. Murphy , H. N. Nelson , F. Neves , J. A. Nikkel , F. G. O'Neill , J. O'Dell , K. O'Sullivan , M. A. Olevitch , K. C. Oliver-Mallory , K. J. Palladino , M. Pangilinan , S. J. Patton , E. K. Pease , A. Piepke , S. Powell , R. M. Preece , K. Pushkin , B. N. Ratcliff , J. Reichenbacher , L. Reichhart , C. Rhyne , J. P. Rodrigues , H. J. Rose , R. Rosero , J. S. Saba , M. Sarychev , R. W. Schnee , M. S. G. Schubnell , P. R. Scovell , S. Shaw , T. A. Shutt , C. Silva , K. Skarpaas , W. Skulski , V. N. Solovov , P. Sorensen , V. V. Sosnovtsev , I. Stancu , M. R. Stark , S. Stephenson , T. M. Stiegler , T. J. Sumner , K. Sundarnath , M. Szydagis , D. J. Taylor , W. Taylor , B. P. Tennyson , P. A. Terman , K. J. Thomas , J. A. Thomson , D. R. Tiedt , W. H. To , A. Tomás , M. Tripathi , C. E. Tull , L. Tvrznikova , S. Uvarov , J. Va'vra , M. G. D. van der Grinten , J. R. Verbus , C. O. Vuosalo , W. L. Waldron , L. Wang , R. C. Webb , W. -Z. Wei , M. While , D. T. White , T. J. Whitis , W. J. Wisniewski , M. S. Witherell , F. L. H. Wolfs , E. Woods , D. Woodward , S. D. Worm , M. Yeh , J. Yin , S. K. Young , C. Zhang

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…

At present, restrictions on the spin-independent parameter space of WIMP dark matter searches have been limited to the results provided by relatively heavy nuclei experiments, based on the conventional wisdom that only such experiments can…

Astrophysics · Physics 2007-05-23 F. Giuliani , TA Girard , T. Morlat

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

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

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

Super-Kamiokande (SK) can search for weakly interacting massive particles (WIMPs) by detecting neutrinos produced from WIMP annihilations occurring inside the Sun. In this analysis, we include neutrino events with interaction vertices in…

High Energy Physics - Experiment · Physics 2015-03-18 Kamiokande Collaboration , K. Choi , K. Abe , Y. Haga , Y. Hayato , K. Iyogi , J. Kameda , Y. Kishimoto , M. Miura , S. Moriyama , M. Nakahata , Y. Nakano , S. Nakayama , H. Sekiya , M. Shiozawa , Y. Suzuki , A. Takeda , T. Tomura , R. A. Wendell , T. Irvine , 2 T. Kajita , I. Kametani , 2 K. Kaneyuki , K. P. Lee , Y. Nishimura , 2 K. Okumura , T. McLachlan , 2 L. Labarga , E. Kearns , J. L. Raaf , 4 J. L. Stone , L. R. Sulak , 4 S. Berkman , 5 H. A. Tanaka , 5 S. Tobayama , M. Goldhaber , G. Carminati , W. R. Kropp , S. Mine , A. Renshaw , M. B. Smy , H. W. Sobel , K. S. Ganezer , J. Hill , N. Hong , J. Y. Kim , I. T. Lim , T. Akiri , A. Himmel , K. Scholberg , C. W. Walter , T. Wongjirad , T. Ishizuka , S. Tasaka , J. S. Jang , J. G. Learned , S. Matsuno , S. N. Smith , T. Hasegawa , T. Ishida , T. Ishii , T. Kobayashi , T. Nakadaira , K. Nakamura , Y. Oyama , K. Sakashita , T. Sekiguchi , T. Tsukamoto , A. T. Suzuki , Y. Takeuchi , C. Bronner , S. Hirota , K. Huang , K. Ieki , M. Ikeda , T. Kikawa , A. Minamino , T. Nakaya , K. Suzuki , S. Takahashi , Y. Fukuda , Y. Itow , G. Mitsuka , P. Mijakowski , J. Hignight , J. Imber , C. K. Jung , C. Yanagisawa , H. Ishino , A. Kibayashi , Y. Koshio , T. Mori , M. Sakuda , T. Yano , Y. Kuno , R. Tacik , S. B. Kim , H. Okazawa , Y. Choi , K. Nishijima , M. Koshiba , Y. Totsuka , M. Yokoyama , K. Martens , Ll. Marti , M. R. Vagins , J. F. Martin , P. de Perio , A. Konaka , M. J. Wilking , S. Chen , Y. Zhang , R. J. Wilkes

In experiments for direct dark matter searches, neutrinos coherently scattering off nuclei can produce similar events as Weakly Interacting Massive Particles (WIMPs). To reach sensitivities better than about 10^-10 pb for the elastic WIMP…

We examine whether the annual modulation found by the DAMA dark matter experiment can be explained by Weakly Interacting Massive Particles (WIMPs), in light of new null results from other experiments. CDMS II has already ruled out most…

Astrophysics · Physics 2009-11-10 Christopher Savage , Paolo Gondolo , Katherine Freese

Weakly Interacting Massive Particles (WIMPs) are one of the leading candidates for Dark Matter. For understanding the nature of WIMPs and identifying them among new particles produced at colliders (hopefully in the near future),…

High Energy Physics - Phenomenology · Physics 2011-08-17 Chung-Lin Shan

This letter reports results from a search for muon-neutrino to electron-neutrino transitions by the MINOS experiment based on a 7x10^20 protons-on-target exposure. Our observation of 54 candidate electron-neutrino events in the Far Detector…

High Energy Physics - Experiment · Physics 2012-08-27 The MINOS Collaboration

Experimentally have we got what it takes to pursue the direct observation of WIMP interactions down to sensitivities of a few events /100 kg/year? For a Ge target with a low energy threshold (<20 keVr) this corresponds to a WIMP-nucleon…

Astrophysics · Physics 2016-11-03 R. J. Gaitskell

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…

High Energy Physics - Experiment · Physics 2019-08-13 Oleg Kamaev

XENON is a project for direct dark matter search located in the INFN underground laboratory LNGS. The previous generation of XENON detector, XENON1T, achieved an exposure of 1 ton$\times$year, setting the most stringent limits on the…

High Energy Physics - Experiment · Physics 2023-10-18 S. E. M. Ahmed Maouloud