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Related papers: The SIMPLE Phase II Dark Matter Search

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LUX-ZEPLIN (LZ) is a dark matter detector expected to obtain world-leading sensitivity to weakly interacting massive particles (WIMPs) interacting via nuclear recoils with a ~7-tonne xenon target mass. This manuscript presents sensitivity…

High Energy Physics - Experiment · Physics 2022-02-18 The LZ Collaboration , D. S. Akerib , A. K. Al Musalhi , S. K. Alsum , C. S. Amarasinghe , A. Ames , T. J. Anderson , N. Angelides , H. M. Araújo , J. E. Armstrong , M. Arthurs , X. Bai , J. Balajthy , S. Balashov , J. Bang , J. W. Bargemann , D. Bauer , A. Baxter , P. Beltrame , E. P. Bernard , A. Bernstein , A. Bhatti , A. Biekert , T. P. Biesiadzinski , H. J. Birch , G. M. Blockinger , E. Bodnia , B. Boxer , C. A. J. Brew , P. Brás , S. Burdin , J. K. Busenitz , M. Buuck , R. Cabrita , M. C. Carmona-Benitez , M. Cascella , C. Chan , N. I. Chott , A. Cole , M. V. Converse , A. Cottle , G. Cox , O. Creaner , J. E. Cutter , C. E. Dahl , L. de Viveiros , J. E. Y. Dobson , E. Druszkiewicz , S. R. Eriksen , A. Fan , S. Fayer , N. M. Fearon , S. Fiorucci , H. Flaecher , E. D. Fraser , T. Fruth , R. J. Gaitskell , J. Genovesi , C. Ghag , E. Gibson , S. Gokhale , M. G. D. van der Grinten , C. B. Gwilliam , C. R. Hall , C. A. Hardy , S. J. Haselschwardt , S. A. Hertel , M. Horn , D. Q. Huang , C. M. Ignarra , O. Jahangir , R. S. James , W. Ji , J. Johnson , A. C. Kaboth , A. C. Kamaha , K. Kamdin , K. Kazkaz , D. Khaitan , A. Khazov , I. Khurana , D. Kodroff , L. Korley , E. V. Korolkova , H. Kraus , S. Kravitz , L. Kreczko , B. Krikler , V. A. Kudryavtsev , E. A. Leason , J. Lee , D. S. Leonard , K. T. Lesko , C. Levy , J. Li , J. Liao , A. Lindote , R. Linehan , W. H. Lippincott , X. Liu , M. I. Lopes , E. Lopez Asamar , B. López Paredes , W. Lorenzon , S. Luitz , P. A. Majewski , A. Manalaysay , L. Manenti , R. L. Mannino , N. Marangou , M. E. McCarthy , D. N. McKinsey , J. McLaughlin , E. H. Miller , E. Mizrachi , A. Monte , M. E. Monzani , J. A. Morad , J. D. Morales Mendoza , E. Morrison , B. J. Mount , A. St. J. Murphy , D. Naim , A. Naylor , C. Nedlik , H. N. Nelson , F. Neves , J. A. Nikoleyczik , A. Nilima , A. Nguyen , I. Olcina , K. C. Oliver-Mallory , S. Pal , K. J. Palladino , J. Palmer , S. Patton , N. Parveen , E. K. Pease , B. Penning , G. Pereira , A. Piepke , Y. Qie , J. Reichenbacher , C. A. Rhyne , A. Richards , Q. Riffard , G. R. C. Rischbieter , R. Rosero , P. Rossiter , D. Santone , A. B. M. R. Sazzad , R. W. Schnee , P. R. Scovell , S. Shaw , T. A. Shutt , J. J. Silk , C. Silva , R. Smith , M. Solmaz , V. N. Solovov , P. Sorensen , J. Soria , I. Stancu , A. Stevens , K. Stifter , B. Suerfu , T. J. Sumner , N. Swanson , M. Szydagis , W. C. Taylor , R. Taylor , D. J. Temples , P. A. Terman , D. R. Tiedt , M. Timalsina , W. H. To , D. R. Tovey , M. Tripathi , D. R. Tronstad , W. Turner , U. Utku , A. Vaitkus , B. Wang , J. J. Wang , W. Wang , J. R. Watson , R. C. Webb , R. G. White , T. J. Whitis , M. Williams , F. L. H. Wolfs , D. Woodward , C. J. Wright , X. Xiang , J. Xu , M. Yeh , P. Zarzhitsky

The Cryogenic Dark Matter Search (CDMS II) experiment aims to detect dark matter particles that elastically scatter from nuclei in semiconductor detectors. The resulting nuclear-recoil energy depositions are detected by ionization and…

Instrumentation and Detectors · Physics 2018-07-31 R. Agnese , A. J. Anderson , T. Aramaki , W. Baker , D. Balakishiyeva , S. Banik , D. Barker , R. Basu Thakur , D. A. Bauer , T. Binder , A. Borgland , M. A. Bowles , P. L. Brink , R. Bunker , B. Cabrera , D. O. Caldwell , R. Calkins , C. Cartaro , D. G. Cerdeno , H. Chagani , Y. -Y. Chang , Y. Chen , J. Cooley , B. Cornell , P. Cushman , M. Daal , T. Doughty , E. M. Dragowsky , L. Esteban , S. Fallows , E. Fascione , E. Figueroa-Feliciano , M. Fritts , G. Gerbier , R. Germond , M. Ghaith , G. L. Godfrey , S. R. Golwala , J. Hall , H. R. Harris , D. Holmgren , Z. Hong , 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 , E. Lopez Asamar , P. Lukens , D. MacDonell , R. Mahapatra , V. Mandic , N. Mast , K. A. McCarthy , E. H. Miller , N. Mirabolfathi , R. A. Moffatt , B. Mohanty , D. Moore , J. D. Morales Mendoza , J. Nelson , S. M. Oser , K. Page , W. A. Page , R. Partridge , M. Penalver Martinez , M. Pepin , A. Phipps , S. Poudel , M. Pyle , H. Qiu , W. Rau , P. Redl , A. Reisetter , A. Roberts , H. E. Rogers , A. E. Robinson , T. Saab , B. Sadoulet , J. Sander , K. Schneck , R. W. Schnee , S. Scorza , K. Senapati , B. Serfass , D. Speller , P. C. F. Di Stefano , 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

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

The XENON experiment aims at the direct detection of dark matter in the form of WIMPs (Weakly Interacting Massive Particles) via their elastic scattering off Xenon nuclei. With a fiducial mass of 1000 kg of liquid xenon, a sufficiently low…

Astrophysics · Physics 2007-05-23 XENON Collaboration , Elena Aprile

At present, application of Superheated Droplet Detectors (SDDs) in WIMP dark matter searches has been limited to the spin-dependent sector, owing to the general use of fluorinated refrigerants which have high spin sensitivity. Given their…

Instrumentation and Detectors · Physics 2008-11-26 F. Giuliani , T. Morlat , T. A. Girard

The superheated emulsion detector consisting of the droplets of tetra-fluoroethane (C2HC$_2$H$_2$F$_4$2F4) has been fabricated at the laboratory and installed at the 555m deep underground laboratory, JUSL during July to Dec 2022. The 500ml…

Instrumentation and Detectors · Physics 2025-01-07 V. Kumar , S. Ali , M. Das , N. Biswas , S. Das , S. Sahoo , N. Chaddha , J. Basu , V. N. Jha

Weakly Interacting Massive Particles (WIMPs) are one of the leading candidates for Dark Matter. Currently, the most promising method to detect WIMPs is the direct detection of the recoil energy deposited in a low-background laboratory…

Astrophysics · Physics 2011-11-10 Chung-Lin Shan

The Cryogenic Rare Event Search with Superconducting Thermometers Phase II (CRESST-II) at the L.N.G.S in Italy is searching for Dark Matter using low-temperature calorimeters. These detectors allow to discriminate different particles by…

Low Temperature Detectors (LTDs) offer the best signal-to-noise performance and thus, lowest energy threshold among other particle detection technologies available today. The excellent background rejection provided by these detectors is…

Instrumentation and Methods for Astrophysics · Physics 2013-08-02 Nader Mirabolfathi

The phonon-mediated hybrid detector is made out of a monolithic silicon crystal characterized by two interconnected regions linked through a narrow neck. Operating solely on phonon signal measurements, the hybrid design facilitates the…

The three-dimensional (3-D) reconstruction of nuclear recoils is of interest for directional detection of fast neutrons and for direction-sensitive searches for weakly interacting massive particles(WIMPs), which may constitute the Dark…

Instrumentation and Detectors · Physics 2015-12-09 S. E. Vahsen , M. T. Hedges , I. Jaegle , S. J. Ross , I. S. Seong , T. N. Thorpe , J. Yamaoka , J. A. Kadyk , M. Garcia-Sciveres

Low mass nuclear recoil dark matter and coherent-elastic-neutrino-nucleus-scattering (CENNS) searches confront similar challenges in choosing ultra-low threshold and large-mass detectors. We report experimental results from the…

Directional detection can provide unambiguous observation of Dark Matter interactions even in presence of insidious backgrounds. The DM-TPC collaboration is developing a detector with the goal of measuring the direction and sense of nuclear…

If the dark matter particle has spin 0, only two types of WIMP-nucleon interaction can arise from the non-relativistic reduction of renormalisable single-mediator models for dark matter-quark interactions. Based on this crucial observation,…

High Energy Physics - Phenomenology · Physics 2018-01-17 Riccardo Catena , Jan Conrad , Christian Döring , Alfredo Davide Ferella , Martin B. Krauss

Astrophysical and cosmological observations suggest the existence of beyond standard model ingredient known as dark matter (DM). One of the most supported class of theories suggests that DM is composed of weakly interactive massive…

Instrumentation and Detectors · Physics 2025-07-04 Giorgio Dho

Using data from the $\nu$-cleus detector, based on the surface of the Earth, we place constraints on dark matter in the form of Strongly Interacting Massive Particles (SIMPs) which interact with nucleons via nuclear-scale cross sections.…

High Energy Physics - Phenomenology · Physics 2017-11-21 Jonathan H. Davis

Recent computational results suggest that directional dark matter detectors have potential to probe for WIMP dark matter particles below the neutrino floor. The DRIFT-IId detector used in this work is a leading directional WIMP search time…

Weakly Interacting Massive Particles (WIMPs) are a leading candidate for dark matter and are expected to produce nuclear recoil (NR) events within liquid xenon time-projection chambers. We present a measurement of the scintillation timing…