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The Dark Matter Time Projection Chamber collaboration recently reported a dark matter limit obtained with a 10 liter time projection chamber filled with CF4 gas. The 10 liter detector was capable of 2D tracking (perpendicular to the drift…

Instrumentation and Methods for Astrophysics · Physics 2015-05-30 J. B. R. Battat , S. Ahlen , M. Chernicoff , C. Deaconu , D. Dujmic , A. Dushkin , P. Fisher , S. Henderson , A. Inglis , A. Kaboth , L. Kirsch , J. P. Lopez , J. Monroe , H. Ouyang , G. Sciolla , H. Tomita , H. Wellenstein

Current cosmological models and data suggest the existence of a cold Dark Matter (DM) component, however the nature of DM particles remains unknown. A favored candidate for DM is a Weakly Interacting Massive Particle (WIMP) in the mass…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Benjamin Zitzer

The LUX-ZEPLIN experiment is a dark matter detector centered on a dual-phase xenon time projection chamber operating at the Sanford Underground Research Facility in Lead, South Dakota, USA. This Letter reports results from LUX-ZEPLIN's…

High Energy Physics - Experiment · Physics 2023-08-07 J. Aalbers , D. S. Akerib , C. W. Akerlof , A. K. Al Musalhi , F. Alder , A. Alqahtani , S. K. Alsum , C. S. Amarasinghe , A. Ames , T. J. Anderson , N. Angelides , H. M. Araújo , J. E. Armstrong , M. Arthurs , S. Azadi , A. J. Bailey , A. Baker , J. Balajthy , S. Balashov , J. Bang , J. W. Bargemann , M. J. Barry , J. Barthel , D. Bauer , A. Baxter , K. Beattie , J. Belle , P. Beltrame , J. Bensinger , T. Benson , E. P. Bernard , A. Bhatti , A. Biekert , T. P. Biesiadzinski , H. J. Birch , B. Birrittella , G. M. Blockinger , K. E. Boast , B. Boxer , R. Bramante , C. A. J. Brew , P. Brás , J. H. Buckley , V. V. Bugaev , S. Burdin , J. K. Busenitz , M. Buuck , R. Cabrita , C. Carels , D. L. Carlsmith , B. Carlson , M. C. Carmona-Benitez , M. Cascella , C. Chan , A. Chawla , H. Chen , J. J. Cherwinka , N. I. Chott , A. Cole , J. Coleman , M. V. Converse , A. Cottle , G. Cox , W. W. Craddock , O. Creaner , D. Curran , A. Currie , J. E. Cutter , C. E. Dahl , A. David , J. Davis , T. J. R. Davison , J. Delgaudio , S. Dey , L. de Viveiros , A. Dobi , J. E. Y. Dobson , E. Druszkiewicz , A. Dushkin , T. K. Edberg , W. R. Edwards , M. M. Elnimr , W. T. Emmet , S. R. Eriksen , C. H. Faham , A. Fan , S. Fayer , N. M. Fearon , S. Fiorucci , H. Flaecher , P. Ford , V. B. Francis , E. D. Fraser , T. Fruth , R. J. Gaitskell , N. J. Gantos , D. Garcia , A. Geffre , V. M. Gehman , J. Genovesi , C. Ghag , R. Gibbons , E. Gibson , M. G. D. Gilchriese , S. Gokhale , B. Gomber , J. Green , A. Greenall , S. Greenwood , M. G. D. van der Grinten , C. B. Gwilliam , C. R. Hall , S. Hans , K. Hanzel , A. Harrison , E. Hartigan-O'Connor , S. J. Haselschwardt , S. A. Hertel , G. Heuermann , C. Hjemfelt , M. D. Hoff , E. Holtom , J. Y-K. Hor , M. Horn , D. Q. Huang , D. Hunt , C. M. Ignarra , R. G. Jacobsen , O. Jahangir , R. S. James , S. N. Jeffery , W. Ji , J. Johnson , A. C. Kaboth , A. C. Kamaha , K. Kamdin , V. Kasey , K. Kazkaz , J. Keefner , D. Khaitan , M. Khaleeq , A. Khazov , I. Khurana , Y. D. Kim , C. D. Kocher , D. Kodroff , L. Korley , E. V. Korolkova , J. Kras , H. Kraus , S. Kravitz , H. J. Krebs , L. Kreczko , B. Krikler , V. A. Kudryavtsev , S. Kyre , B. Landerud , E. A. Leason , C. Lee , J. Lee , D. S. Leonard , R. Leonard , K. T. Lesko , C. Levy , J. Li , F. -T. Liao , J. Liao , J. Lin , A. Lindote , R. Linehan , W. H. Lippincott , R. Liu , X. Liu , Y. Liu , C. Loniewski , M. I. Lopes , E. Lopez Asamar , B. López Paredes , W. Lorenzon , D. Lucero , S. Luitz , J. M. Lyle , P. A. Majewski , J. Makkinje , D. C. Malling , A. Manalaysay , L. Manenti , R. L. Mannino , N. Marangou , M. F. Marzioni , C. Maupin , M. E. McCarthy , C. T. McConnell , D. N. McKinsey , J. McLaughlin , Y. Meng , J. Migneault , E. H. Miller , E. Mizrachi , J. A. Mock , A. Monte , M. E. Monzani , J. A. Morad , J. D. Morales Mendoza , E. Morrison , B. J. Mount , M. Murdy , A. St. J. Murphy , D. Naim , A. Naylor , C. Nedlik , C. Nehrkorn , F. Neves , A. Nguyen , J. A. Nikoleyczik , A. Nilima , J. O'Dell , F. G. O'Neill , K. O'Sullivan , I. Olcina , M. A. Olevitch , K. C. Oliver-Mallory , J. Orpwood , D. Pagenkopf , S. Pal , K. J. Palladino , J. Palmer , M. Pangilinan , N. Parveen , S. J. Patton , E. K. Pease , B. Penning , C. Pereira , G. Pereira , E. Perry , T. Pershing , I. B. Peterson , A. Piepke , J. Podczerwinski , D. Porzio , S. Powell , R. M. Preece , K. Pushkin , Y. Qie , B. N. Ratcliff , J. Reichenbacher , L. Reichhart , C. A. Rhyne , A. Richards , Q. Riffard , G. R. C. Rischbieter , J. P. Rodrigues , A. Rodriguez , H. J. Rose , R. Rosero , P. Rossiter , T. Rushton , G. Rutherford , D. Rynders , J. S. Saba , D. Santone , A. B. M. R. Sazzad , R. W. Schnee , P. R. Scovell , D. Seymour , S. Shaw , T. Shutt , J. J. Silk , C. Silva , G. Sinev , K. Skarpaas , W. Skulski , R. Smith , M. Solmaz , V. N. Solovov , P. Sorensen , J. Soria , I. Stancu , M. R. Stark , A. Stevens , T. M. Stiegler , K. Stifter , R. Studley , B. Suerfu , T. J. Sumner , P. Sutcliffe , N. Swanson , M. Szydagis , M. Tan , D. J. Taylor , R. Taylor , W. C. Taylor , D. J. Temples , B. P. Tennyson , P. A. Terman , K. J. Thomas , D. R. Tiedt , M. Timalsina , W. H. To , A. Tomás , Z. Tong , D. R. Tovey , J. Tranter , M. Trask , M. Tripathi , D. R. Tronstad , C. E. Tull , W. Turner , L. Tvrznikova , U. Utku , J. Va'vra , A. Vacheret , A. C. Vaitkus , J. R. Verbus , E. Voirin , W. L. Waldron , A. Wang , B. Wang , J. J. Wang , W. Wang , Y. Wang , J. R. Watson , R. C. Webb , A. White , D. T. White , J. T. White , R. G. White , T. J. Whitis , M. Williams , W. J. Wisniewski , M. S. Witherell , F. L. H. Wolfs , J. D. Wolfs , S. Woodford , D. Woodward , S. D. Worm , C. J. Wright , Q. Xia , X. Xiang , Q. Xiao , J. Xu , M. Yeh , J. Yin , I. Young , P. Zarzhitsky , A. Zuckerman , E. A. Zweig

Solving the Dark Matter enigma represents one of the key objectives of contemporary physics. Recent astrophysical and cosmological measurements have unambiguously demonstrated that ordinary matter contributes to less than 5 % of the energy…

Astrophysics · Physics 2015-06-24 Gabriel Chardin

The Dark matter Experiment using Argon Pulse-shape discrimination (DEAP) has been designed for a direct detection search for particle dark matter using a single-phase liquid argon target. The projected cross section sensitivity for…

Instrumentation and Methods for Astrophysics · Physics 2019-02-19 P. -A. Amaudruz , M. Baldwin , M. Batygov , B. Beltran , C. E. Bina , D. Bishop , J. Bonatt , G. Boorman , M. G. Boulay , B. Broerman , T. Bromwich , J. F. Bueno , P. M. Burghardt , A. Butcher , B. Cai , S. Chan , M. Chen , R. Chouinard , S. Churchwell , B. T. Cleveland , D. Cranshaw , K. Dering , J. DiGioseffo , S. Dittmeier , F. A. Duncan , M. Dunford , A. Erlandson , N. Fatemighomi , S. Florian , A. Flower , R. J. Ford , R. Gagnon , P. Giampa , V. V. Golovko , P. Gorel , R. Gornea , E. Grace , K. Graham , D. R. Grant , E. Gulyev , A. Hall , A. L. Hallin , M. Hamstra , P. J. Harvey , C. Hearns , C. J. Jillings , O. Kamaev , A. Kemp , M. Kuźniak , S. Langrock , F. La Zia , B. Lehnert , O. Li , J. J. Lidgard , P. Liimatainen , C. Lim , T. Lindner , Y. Linn , S. Liu , P. Majewski , R. Mathew , A. B. McDonald , T. McElroy , K. McFarlane , T. McGinn , J. B. McLaughlin , S. Mead , R. Mehdiyev , C. Mielnichuk , J. Monroe , A. Muir , P. Nadeau , C. Nantais , C. Ng , A. J. Noble , E. O'Dwyer , C. Ohlmann , K. Olchanski , K. S. Olsen , C. Ouellet , P. Pasuthip , S. J. M. Peeters , T. R. Pollmann , E. T. Rand , W. Rau , C. Rethmeier , F. Retière , N. Seeburn , B. Shaw , K. Singhrao , P. Skensved , B. Smith , N. J. T. Smith , T. Sonley , J. Soukup , R. Stainforth , C. Stone , V. Strickland , B. Sur , J. Tang , J. Taylor , L. Veloce , E. Vázquez-Jáuregui , J. Walding , M. Ward , S. Westerdale , R. White , E. Woolsey , J. Zielinski

The recent WMAP data have confirmed that exotic dark matter together with the vacuum energy (cosmological constant) dominate in the flat Universe. Modern particle theories naturally provide viable cold dark matter candidates with masses in…

Cosmology and Nongalactic Astrophysics · Physics 2009-12-17 J. D. Vergados , Ch. C. Moustakidis

Direct dark matter searches are promising techniques to identify the nature of dark matter particles. I describe the future of this field of research, focussing on the question of what can be achieved in the next decade. I will present the…

Instrumentation and Methods for Astrophysics · Physics 2012-12-04 Laura Baudis

Indirect detection of dark matter particles, i.e. the detection of annihilation or decay products of Weakly Interacting Massive Particles, has entered a pivotal phase as experiments reach sensitivities that probe the most interesting…

High Energy Physics - Phenomenology · Physics 2014-11-10 Jan Conrad

Directional detection is a promising dark matter search strategy. Indeed, weakly interacting massive particle (WIMP)-induced recoils would present a direction dependence toward the Cygnus constellation, while background-induced recoils…

Cosmology and Nongalactic Astrophysics · Physics 2011-04-22 J. Billard , F. Mayet , D. Santos

A direction-sensitive dark matter search experiment at Kamioka underground laboratory with the NEWAGE-0.3a detector was performed. The NEWAGE- 0.3a detector is a gaseous micro-time-projection chamber filled with CF4 gas at 152 Torr. The…

Over the past decades, several ideas and technologies have been developed to directly detect WIMP from the galactic halo. All these detection strategies share the common goal of discriminating a WIMP signal from the residual backgrounds. By…

Instrumentation and Detectors · Physics 2015-06-23 J. Billard

Unveiling the nature of cosmic dark matter (DM) is an urgent issue in cosmology. Here we make use of a strategy based on the search for the imprints left on the cosmic microwave background temperature and polarization spectra by the energy…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-11 Carmelo Evoli , Stefania Pandolfi , Andrea Ferrara

Weakly Interacting Massive Particles (WIMPs) are one of the leading candidates for Dark Matter. We develop a model-independent method for determining the mass $m_\chi$ of the WIMP by using data (i.e., measured recoil energies) of direct…

High Energy Physics - Phenomenology · Physics 2009-01-06 Manuel Drees , Chung-Lin Shan

We report the first dark matter search results from XENON1T, a $\sim$2000-kg-target-mass dual-phase (liquid-gas) xenon time projection chamber in operation at the Laboratori Nazionali del Gran Sasso in Italy and the first ton-scale detector…

Cosmology and Nongalactic Astrophysics · Physics 2017-11-27 E. Aprile , J. Aalbers , F. Agostini , M. Alfonsi , F. D. Amaro , M. Anthony , F. Arneodo , P. Barrow , L. Baudis , B. Bauermeister , M. L. Benabderrahmane , T. Berger , P. A. Breur , A. Brown , A. Brown , E. Brown , S. Bruenner , G. Bruno , R. Budnik , L. Bütikofer , J. Calvén , J. M. R. Cardoso , M. Cervantes , D. Cichon , D. Coderre , A. P. Colijn , J. Conrad , J. P. Cussonneau , M. P. Decowski , P. de Perio , P. Di Gangi , A. Di Giovanni , S. Diglio , G. Eurin , J. Fei , A. D. Ferella , A. Fieguth , W. Fulgione , A. Gallo Rosso , M. Galloway , F. Gao , M. Garbini , R. Gardner , C. Geis , L. W. Goetzke , L. Grandi , Z. Greene , C. Grignon , C. Hasterok , E. Hogenbirk , J. Howlett , R. Itay , B. Kaminsky , S. Kazama , G. Kessler , A. Kish , H. Landsman , R. F. Lang , D. Lellouch , L. Levinson , Q. Lin , S. Lindemann , M. Lindner , F. Lombardi , J. A. M. Lopes , A. Manfredini , I. Mariş , T. Marrodán Undagoitia , J. Masbou , F. V. Massoli , D. Masson , D. Mayani , M. Messina , K. Micheneau , A. Molinario , K. Morå , M. Murra , J. Naganoma , K. Ni , U. Oberlack , P. Pakarha , B. Pelssers , R. Persiani , F. Piastra , J. Pienaar , V. Pizzella , M. -C. Piro , G. Plante , N. Priel , L. Rauch , S. Reichard , C. Reuter , B. Riedel , A. Rizzo , S. Rosendahl , N. Rupp , R. Saldanha , J. M. F. dos Santos , G. Sartorelli , M. Scheibelhut , S. Schindler , J. Schreiner , M. Schumann , L. Scotto Lavina , M. Selvi , P. Shagin , E. Shockley , M. Silva , H. Simgen , M. v. Sivers , A. Stein , S. Thapa , D. Thers , A. Tiseni , G. Trinchero , C. Tunnell , M. Vargas , N. Upole , H. Wang , Z. Wang , Y. Wei , C. Weinheimer , J. Wulf , J. Ye , Y. Zhang , T. Zhu

Coherent scattering of solar, atmospheric and diffuse supernovae neutrinos creates an irreducible background for direct dark matter experiments with sensitivities to WIMP-nucleon spin-independent scattering cross-sections of…

High Energy Physics - Phenomenology · Physics 2014-10-01 Philipp Grothaus , Malcolm Fairbairn , Jocelyn Monroe

The XENON1T experiment uses a time projection chamber (TPC) with liquid Xenon to search for Weakly Interacting Massive Particles (WIMPs), a proposed Dark Matter particle, via direct detection. As this experiment relies on capturing rare…

High Energy Physics - Phenomenology · Physics 2020-08-03 Charanjit K. Khosa , Lucy Mars , Joel Richards , Veronica Sanz

The Cryogenic Dark Matter Search (CDMS) is an experiment to detect weakly interacting massive particles (WIMPs) based on their interactions with Ge and Si nuclei. We report the results of an analysis of data from the first two runs of CDMS…

Astrophysics · Physics 2012-08-27 CDMS Collaboration

We report the WIMP dark matter search results using the first physics-run data of the PandaX-II 500 kg liquid xenon dual-phase time-projection chamber, operating at the China JinPing Underground Laboratory. No dark matter candidate is…

Large arrays of aligned carbon nanotubes (CNTs), open at one end, could be used as target material for the directional detection of weakly interacting dark matter particles (WIMPs). As a result of a WIMP elastic scattering on a CNT, a…

Instrumentation and Detectors · Physics 2016-07-20 G. Cavoto , E. N. M. Cirillo , F. Cocina , J. Ferretti , A. D. Polosa