中文
相关论文

相关论文: First results with the ORPHEUS dark matter detecto…

200 篇论文

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…

高能物理 - 实验 · 物理学 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…

宇宙学与河外天体物理 · 物理学 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…

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…

高能物理 - 实验 · 物理学 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…

高能天体物理现象 · 物理学 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…

高能物理 - 唯象学 · 物理学 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…

仪器与探测器 · 物理学 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…

天体物理仪器与方法 · 物理学 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…

天体物理仪器与方法 · 物理学 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…

核实验 · 物理学 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…

天体物理学 · 物理学 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…

高能物理 - 唯象学 · 物理学 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…

天体物理仪器与方法 · 物理学 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…

高能天体物理现象 · 物理学 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…