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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

A search for dark matter was conducted by looking for an annual modulation signal due to the Earth's rotation around the Sun using XMASS, a single phase liquid xenon detector. The data used for this analysis was 359.2 live days times 832 kg…

The China Dark matter Experiment collaboration reports the first experimental limit on WIMP dark matter from 14.6 kg-day of data taken with a 994 g p-type point-contact germanium detector at the China Jinping underground Laboratory where…

The DEAP-3600 experiment is searching for WIMP dark matter with a 3.3 tonne single phase liquid argon (LAr) target, located 2.1 km underground at SNOLAB. The experimental signature of dark matter interactions is keV-scale $^{40}$Ar nuclear…

The Any Light Particle Search II (ALPS II) experiment at DESY, Hamburg, is a Light-Shining-through-a-Wall (LSW) experiment aiming to probe the existence of axions and axion-like particles (ALPs), which are candidates for dark matter. Data…

The LUX collaboration new results advance the search for dark matter candidate particles in the 4 GeV/c^2 and higher mass range, with a maximal spin-independent 90% C.L. limit of 2 x 10^-46 cm^2 at 50 GeV/c^2 for its 332 live-day run,…

Cosmology and Nongalactic Astrophysics · Physics 2019-08-15 M. Szydagis

WIMPs are promising dark matter candidates. A WIMP occasionally collides with a mirror equipped with interferometric gravitational wave detectors such as LIGO, Virgo, KAGRA and the Einstein Telescope (ET). When WIMPs collide with a mirror…

High Energy Astrophysical Phenomena · Physics 2020-03-10 Satoshi Tsuchida , Nobuyuki Kanda , Yousuke Itoh , Masaki Mori

We present here a search for WIMP dark matter using 790.8 live-days of data collected with 3269 kg of liquid argon (1266 kg fiducial) by the DEAP-3600 detector at SNOLAB, using the Profile Likelihood Ratio method. The likelihood model is…

High Energy Physics - Experiment · Physics 2026-03-17 DEAP Collaboration , P. Adhikari , R. Ajaj , M. Alpízar-Venegas , P. -A. Amaudruz , J. Anstey , D. J. Auty , M. Baldwin , M. Batygov , B. Beltran , A. Bigentini , C. E. Bina , W. Bonivento , M. G. Boulay , J. F. Bueno , P. M. Burghardt , A. Butcher , M. Cadeddu , B. Cai , M. Cárdenas-Montes , S. Cavuoti , Y. Chen , S. Choudhary , B. T. Cleveland , R. Crampton , S. Daugherty , P. DelGobbo , P. Di Stefano , G. Dolganov , L. Doria , F. A. Duncan , M. Dunford , E. Ellingwood , A. Erlandson , S. S. Farahani , N. Fatemighomi , G. Fiorillo , R. J. Ford , D. Gahan , D. Gallacher , A. Garai , P. García Abia , S. Garg , P. Giampa , A. Giménez-Alcázar , D. Goeldi , P. Gorel , K. Graham , A. Grobov , A. L. Hallin , M. Hamstra , S. Haskins , J. Hu , J. Hucker , D. Huff , T. Hugues , A. Ilyasov , B. Jigmeddorj , C. J. Jillings , A. Joy , G. Kaur , A. Kemp , M. Khoshraftar Yazdi , M. Kuźniak , F. La Zia , M. Lai , S. Langrock , B. Lehnert , J. LePage-Bourbonnais , M. Lissia , L. Luzzi , I. Machulin , P. Majewski , A. Maru , J. Mason , A. B. McDonald , T. McElroy , J. B. McLaughlin , C. Mielnichuk , L. Mirasola , A. Moharana , J. Monroe , A. Murray , M. Needs , C. Ng , G. Oliviéro , M. Olszewski , S. Pal , D. Papi , B. Park , M. Perry , V. Pesudo , T. R. Pollmann , F. Rad , C. Rethmeier , F. Retière , I. Rodríguez García , L. Roszkowski , R. Santorelli , F. G. Schuckman , N. Seeburn , S. Seth , V. Shalamova , P. Skensved , T. Smirnova , N. J. T. Smith , K. Sobotkiewich , T. Sonley , J. Sosiak , J. Soukup , R. Stainforth , M. Stringer , J. Tang , P. Taylor , R. Turcotte-Tardif , E. Vázquez-Jáuregui , G. Vera Díaz , S. Viel , B. Vyas , M. Walczak , J. Walding , M. Ward , S. Westerdale , R. Wormington , A. Zuñiga-Reyes

Recent progress on the development of very low noise high purity germanium ionization spectrometers has produced an instrument of 1.2 kg mass and excellent noise performance. The detector was installed in a low-background cryostat intended…

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…

An annual modulation signal due to the Earth orbiting around the Sun would be one of the strongest indications of the direct detection of dark matter. In 2016, we reported a search for dark matter by looking for this annual modulation with…

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 CONUS experiment is searching for coherent elastic neutrino nucleus scattering of reactor anti-neutrinos with four low energy threshold point-contact high-purity germanium spectrometers. An excellent background suppression within the…

Instrumentation and Detectors · Physics 2024-01-01 H. Bonet , A. Bonhomme , C. Buck , K. Fülber , J. Hakenmüller , J. Hempfling , G. Heusser , T. Hugle , M. Lindner , W. Maneschg , T. Rink , H. Strecker , R. Wink

We make use of the EDELWEISS-III array of germanium bolometers to search for electron interactions at the keV scale induced by phenomena beyond the Standard Model. A 90% C.L. lower limit is set on the electron lifetime decaying to…

We report new limits on spin-independent WIMP-nucleon interaction cross-section using 39.5 kg-days of data taken with a p-type point-contact germanium detector of 840 g fiducial mass at the Kuo-Sheng Reactor Neutrino Laboratory. Crucial to…

High Energy Physics - Experiment · Physics 2014-05-29 TEXONO Collaboration

We report on a blinded search for dark matter (DM) using ionization-only (S2-only) signals in XENONnT with a total exposure of $7.83\mathrm{tonne}\times\mathrm{year}$ over 579 days in three science runs. Dedicated background suppression…

High Energy Physics - Experiment · Physics 2026-01-19 E. Aprile , J. Aalbers , K. Abe , M. Adrover , S. Ahmed Maouloud , L. Althueser , B. Andrieu , E. Angelino , D. Antón Martin , S. R. Armbruster , F. Arneodo , L. Baudis , M. Bazyk , V. Beligotti , L. Bellagamba , R. Biondi , A. Bismark , K. Boese , R. M. Braun , G. Bruni , G. Bruno , R. Budnik , C. Cai , C. Capelli , J. M. R. Cardoso , A. P. Cimental Chávez , A. P. Colijn , J. Conrad , J. J. Cuenca-García , V. D'Andrea , L. C. Daniel Garcia , M. P. Decowski , A. Deisting , C. Di Donato , P. Di Gangi , S. Diglio , K. Eitel , S. el Morabit , R. Elleboro , A. Elykov , A. D. Ferella , C. Ferrari , H. Fischer , T. Flehmke , M. Flierman , R. Frankel , D. Fuchs , W. Fulgione , C. Fuselli , F. Gao , R. Giacomobono , F. Girard , R. Glade-Beucke , L. Grandi , J. Grigat , H. Guan , M. Guida , P. Gyorgy , R. Hammann , C. Hils , L. Hoetzsch , N. F. Hood , M. Iacovacci , Y. Itow , J. Jakob , F. Joerg , Y. Kaminaga , M. Kara , S. Kazama , P. Kharbanda , M. Kobayashi , D. Koke , K. Kooshkjalali , A. Kopec , H. Landsman , R. F. Lang , L. Levinson , A. Li , I. Li , S. Li , S. Liang , Z. Liang , Y. -T. Lin , S. Lindemann , M. Lindner , K. Liu , M. Liu , F. Lombardi , J. A. M. Lopes , G. M. Lucchetti , T. Luce , Y. Ma , C. Macolino , G. C. Madduri , J. Mahlstedt , F. Marignetti , T. Marrodán Undagoitia , K. Martens , J. Masbou , S. Mastroianni , V. Mazza , A. Melchiorre , J. Merz , M. Messina , A. Michel , K. Miuchi , A. Molinario , S. Moriyama , M. Murra , J. Müller , K. Ni , C. T. Oba Ishikawa , U. Oberlack , S. Ouahada , B. Paetsch , Y. Pan , Q. Pellegrini , R. Peres , J. Pienaar , M. Pierre , G. Plante , T. R. Pollmann , F. Pompa , A. Prajapati , L. Principe , J. Qin , D. Ramírez García , A. Ravindran , A. Razeto , R. Singh , L. Sanchez , J. M. F. dos Santos , I. Sarnoff , G. Sartorelli , J. Schreiner , P. Schulte , H. Schulze Eißing , M. Schumann , L. Scotto Lavina , M. Selvi , F. Semeria , F. N. Semler , P. Shagin , S. Shi , H. Simgen , Z. Song , A. Stevens , C. Szyszka , A. Takeda , Y. Takeuchi , P. -L. Tan , D. Thers , G. Trinchero , C. D. Tunnell , K. Valerius , S. Vecchi , S. Vetter , G. Volta , B. von Krosigk , C. Weinheimer , M. Weiss , D. Wenz , C. Wittweg , V. H. S. Wu , Y. Xing , D. Xu , Z. Xu , M. Yamashita , J. Yang , L. Yang , J. Ye , M. Yoshida , L. Yuan , G. Zavattini , Y. Zhao , M. Zhong , T. Zhu

The Cryogenic Dark Matter Search (CDMS) II uses crystals operated at milliKelvin temperature to search for dark matter. We present the details of the profile likelihood analysis of 140.2 kg-day exposure from the final data set of the CDMS…

Instrumentation and Methods for Astrophysics · Physics 2019-08-13 J. Billard

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…

Astrophysics · Physics 2012-08-27 CDMS Collaboration

A technique to measure low intensity fast neutron flux has been developed. The design, calibrations, procedure for data analysis and interpretation of the results are discussed in detail. The technique has been applied to measure the…

High Energy Physics - Experiment · Physics 2008-11-26 E. Tziaferi , M. J. Carson , V. A. Kudryavtsev , R. Lerner , P. K. Lightfoot , S. M. Paling , M. Robinson , N. J. C. Spooner
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