English
Related papers

Related papers: First results with the ORPHEUS dark matter detecto…

200 papers

The EDELWEISS Dark Matter Search uses low-temperature Ge detectors with heat and ionisation read-out to identify nuclear recoils induced by elastic collisions with WIMPs from the galactic halo. Preliminary results obtained with 320g…

The DAMIC (Dark Matter in CCDs) experiment searches for the interactions of dark matter particles with the nuclei and the electrons in the silicon bulk of thick fully depleted charge-coupled devices (CCDs). Because of the low noise and low…

High Energy Physics - Experiment · Physics 2020-04-02 Mariangela Settimo

The quest for the particle nature of dark matter is one of the big open questions of modern physics. A well motivated candidate for dark matter is the so-called WIMP - a weakly interacting massive particle. Recently several theoretically…

Liquid argon is a bright scintillator with potent particle identification properties, making it an attractive target for direct-detection dark matter searches. The DarkSide-50 dark matter search here reports the first WIMP search results…

Cosmology and Nongalactic Astrophysics · Physics 2016-04-15 The DarkSide Collaboration , P. Agnes , L. Agostino , I. F. M. Albuquerque , T. Alexander , A. K. Alton , K. Arisaka , H. O. Back , B. Baldin , K. Biery , G. Bonfini , M. Bossa , B. Bottino , A. Brigatti , J. Brodsky , F. Budano , S. Bussino , M. Cadeddu , L. Cadonati , M. Cadoni , F. Calaprice , N. Canci , A. Candela , H. Cao , M. Cariello , M. Carlini , S. Catalanotti , P. Cavalcante , A. Chepurnov , A. G. Cocco , G. Covone , L. Crippa , D. D'Angelo , M. D'Incecco , S. Davini , S. De Cecco , M. De Deo , M. De Vincenzi , A. Derbin , A. Devoto , F. Di Eusanio , G. Di Pietro , E. Edkins , A. Empl , A. Fan , G. Fiorillo , K. Fomenko , G. Forster , D. Franco , F. Gabriele , C. Galbiati , C. Giganti , A. M. Goretti , F. Granato , L. Grandi , M. Gromov , M. Guan , Y. Guardincerri , B. R. Hackett , K. Herner , E. V. Hungerford , Al. Ianni , An. Ianni , I. James , C. Jollet , K. Keeter , C. L. Kendziora , V. Kobychev , G. Koh , D. Korablev , G. Korga , A. Kubankin , X. Li , M. Lissia , P. Lombardi , S. Luitz , Y. Ma , I. N. Machulin , A. Mandarano , S. M. Mari , J. Maricic , L. Marini , C. J. Martoff , A. Meregaglia , P. D. Meyers , T. Miletic , R. Milincic , D. Montanari , A. Monte , M. Montuschi , M. Monzani , P. Mosteiro , B. J. Mount , V. N. Muratova , P. Musico , J. Napolitano , A. Nelson , S. Odrowski , M. Orsini , F. Ortica , L. Pagani , M. Pallavicini , E. Pantic , S. Parmeggiano , K. Pelczar , N. Pelliccia , S. Perasso , A. Pocar , S. Pordes , D. A. Pugachev , H. Qian , K. Randle , G. Ranucci , A. Razeto , B. Reinhold , A. L. Renshaw , A. Romani , B. Rossi , N. Rossi , D. Rountree , D. Sablone , P. Saggese , R. Saldanha , W. Sands , S. Sangiorgio , C. Savarese , E. Segreto , D. A. Semenov , E. Shields , P. N. Singh , M. D. Skorokhvatov , M. Smallcomb , O. Smirnov , A. Sotnikov , C. Stanford , Y. Suvorov , R. Tartaglia , J. Tatarowicz , G. Testera , A. Tonazzo , P. Trinchese , E. V. Unzhakov , A. Vishneva , B. Vogelaar , M. Wada , S. Walker , H. Wang , Y. Wang , A. W. Watson , S. Westerdale , J. Wilhelmi , M. M. Wojcik , X. Xiang , J. Xu , C. Yang , J. Yoo , S. Zavatarelli , A. Zec , W. Zhong , C. Zhu , G. Zuzel

One of the most promising strategies to identify the nature of dark matter consists in the search for new particles at accelerators and with so-called direct detection experiments. Working within the framework of simplified models, and…

High Energy Physics - Phenomenology · Physics 2018-05-04 Gianfranco Bertone , Nassim Bozorgnia , Jong Soo Kim , Sebastian Liem , Christopher McCabe , Sydney Otten , Roberto Ruiz de Austri

The first run for the dark matter direct search experiment at Jaduguda Underground Science Laboratory is presented in this article. The experiment named InDEx; the Indian Dark matter search Experiment has been initiated with superheated…

High Energy Physics - Experiment · Physics 2026-01-07 Vimal Kumar , Susmita Das , Mala Das

Dark matter is thought to make up most of the matter density of the Universe, yet its true nature remains uncertain. Among dark matter theories, Weakly Interacting Massive Particles (WIMPs) are a prominent candidate for dark matter because…

High Energy Astrophysical Phenomena · Physics 2023-09-20 Micael Andrade , Aion Viana

The dark matter of our galactic halo may be constituted by elementary particles that interact weakly with ordinary matter (WIMPs). In spite of the very low counting rates expected for these dark matter particles to scatter off nuclei in a…

High Energy Physics - Phenomenology · Physics 2007-05-23 Paolo Gondolo

A new general purpose fixed target facility is proposed at the CERN SPS accelerator which is aimed at exploring the domain of hidden particles and make measurements with tau neutrinos. Hidden particles are predicted by a large number of…

Instrumentation and Detectors · Physics 2015-04-21 SHiP Collaboration , M. Anelli , S. Aoki , G. Arduini , J. J. Back , A. Bagulya , W. Baldini , A. Baranov , G. J. Barker , S. Barsuk , M. Battistin , J. Bauche , A. Bay , V. Bayliss , L. Bellagamba , G. Bencivenni , M. Bertani , O. Bezshyyko , D. Bick , N. Bingefors , A. Blondel , M. Bogomilov , A. Boyarsky , D. Bonacorsi , D. Bondarenko , W. Bonivento , J. Borburgh , T. Bradshaw , R. Brenner , D. Breton , N. Brook , M. Bruschi , A. Buonaura , S. Buontempo , S. Cadeddu , A. Calcaterra , M. Calviani , M. Campanelli , C. Capoccia , A. Cecchetti , A. Chatterjee , J. Chauveau , A. Chepurnov , M. Chernyavskiy , P. Ciambrone , C. Cicalo , G. Conti , K. Cornelis , M. Courthold , M. G. Dallavalle , N. D'Ambrosio , G. De Lellis , M. De Serio , L. Dedenko , A. Di Crescenzo , N. Di Marco , C. Dib , J. Dietrich , H. Dijkstra , D. Domenici , S. Donskov , D. Druzhkin , J. Ebert , U. Egede , A. Egorov , V. Egorychev , M. A. El Alaoui , T. Enik , A. Etenko , F. Fabbri , L. Fabbri , G. Fedorova , G. Felici , M. Ferro-Luzzi , R. A. Fini , M. Franke , M. Fraser , G. Galati , B. Giacobbe , B. Goddard , L. Golinka-Bezshyyko , D. Golubkov , A. Golutvin , D. Gorbunov , E. Graverini , J-L Grenard , A. M. Guler , C. Hagner , H. Hakobyan , J. C. Helo , E. van Herwijnen , D. Horvath , M. Iacovacci , G. Iaselli , R. Jacobsson , I. Kadenko , M. Kamiscioglu , C. Kamiscioglu , G. Khaustov , A. Khotjansev , B. Kilminster , V. Kim , N. Kitagawa , K. Kodama , A. Kolesnikov , D. Kolev , M. Komatsu , N. Konovalova , S. Koretskiy , I. Korolko , A. Korzenev , S. Kovalenko , Y. Kudenko , E. Kuznetsova , H. Lacker , A. Lai , G. Lanfranchi , A. Lauria , H. Lebbolo , J. -M. Levy , L. Lista , P. Loverre , A. Lukiashin , V. E. Lyubovitskij , A. Malinin , M. Manfredi , A. Perillo-Marcone , A. Marrone , R. Matev , E. N. Messomo , P. Mermod , S. Mikado , Yu. Mikhaylov , J. Miller , D. Milstead , O. Mineev , R. Mingazheva , G. Mitselmakher , M. Miyanishi , P. Monacelli , A. Montanari , M. C. Montesi , G. Morello , K. Morishima , S. Movtchan , V. Murzin , N. Naganawa , T. Naka , M. Nakamura , T. Nakano , N. Nurakhov , B. Obinyakov , K. Ocalan , S. Ogawa , V. Oreshkin , A. Orlov , J. Osborne , P. Pacholek , J. Panman , A. Paoloni , L. Paparella , A. Pastore , M. Patel , K. Petridis , M. Petrushin , M. Poli-Lener , N. Polukhina , V. Polyakov , M. Prokudin , G. Puddu , F. Pupilli , F. Rademakers , A. Rakai , T. Rawlings , F. Redi , S. Ricciardi , R. Rinaldesi , T. Roganova , A. Rogozhnikov , H. Rokujo , A. Romaniouk , G. Rosa , I. Rostovtseva , T. Rovelli , O. Ruchayskiy , T. Ruf , G. Saitta , V. Samoylenko , V. Samsonov , A. Sanz Ull , A. Saputi , O. Sato , W. Schmidt-Parzefall , N. Serra , S. Sgobba , M. Shaposhnikov , P. Shatalov , A. Shaykhiev , L. Shchutska , V. Shevchenko , H. Shibuya , Y. Shitov , S. Silverstein , S. Simone , M. Skorokhvatov , S. Smirnov , E. Solodko , V. Sosnovtsev , R. Spighi , M. Spinetti , N. Starkov , B. Storaci , C. Strabel , P. Strolin , S. Takahashi , P. Teterin , V. Tioukov , D. Tommasini , D. Treille , R. Tsenov , T. Tshchedrina , A. Ustyuzhanin , F. Vannucci , V. Venturi , M. Villa , Heinz Vincke , Helmut Vincke , M. Vladymyrov , S. Xella , M. Yalvac , N. Yershov , D. Yilmaz , A. U. Yilmazer , G. Vankova-Kirilova , Y. Zaitsev , A. Zoccoli

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

We study a three stage dark matter and neutrino observatory based on multi-ton two-phase liquid Xe and Ar detectors with sufficiently low backgrounds to be sensitive to WIMP dark matter interaction cross sections down to 10E-47 cm^2, and to…

Instrumentation and Methods for Astrophysics · Physics 2015-03-19 K. Arisaka , P. Beltrame , C. W. Lam , P. F. Smith , C. Ghag , D. B. Cline , K. Lung , Y. Meng , E. Pantic , P. R. Scovell , A. Teymourian , H. Wang

A new type of radiation detector, a p-type modified electrode germanium diode, is presented. The prototype displays, for the first time, a combination of features (mass, energy threshold and background expectation) required for a…

Nuclear Experiment · Physics 2011-05-12 P. S. Barbeau , J. I. Collar , O. Tench

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

Probing low mass (sub-GeV -- few GeV) Weakly Interacting Massive Particle (WIMP) candidates of dark matter through WIMP-induced nuclear recoils in direct detection experiments requires use of detector materials consisting of low mass target…

High Energy Physics - Phenomenology · Physics 2020-05-13 Susnata Seth , Sunita Sahoo , Pijushpani Bhattacharjee , Mala Das

XENON100 is a liquid xenon (LXe) time projection chamber built to search for rare collisions of hypothetical, weakly interacting massive particles (WIMPs). Operated in a low-background shield at the Gran Sasso underground laboratory in…

Instrumentation and Methods for Astrophysics · Physics 2012-06-29 P. R. Scovell , XENON100 Collaboration

The details of what constitutes the majority of the mass that makes up dark matter in the Universe remains one of the prime puzzles of cosmology and particle physics today - eighty years after the first observational indications. Today, it…

High Energy Astrophysical Phenomena · Physics 2015-12-16 Stefan Funk

The EDELWEISS collaboration has performed a search for dark matter particles with masses below the GeV-scale with a 33.4-g germanium cryogenic detector operated in a surface lab. The energy deposits were measured using a…

We report the results of a weakly-interacting massive particle (WIMP) dark matter search using the full 80.1\;live-day exposure of the first stage of the PandaX experiment (PandaX-I) located in the China Jin-Ping Underground Laboratory. The…

The Large Underground Xenon (LUX) experiment, a dual-phase xenon time-projection chamber operating at the Sanford Underground Research Facility (Lead, South Dakota), was cooled and filled in February 2013. We report results of the first…