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In experiments for direct dark matter searches, neutrinos coherently scattering off nuclei can produce similar events as Weakly Interacting Massive Particles (WIMPs). To reach sensitivities better than about 10^-10 pb for the elastic WIMP…

As part of the T-REX project, a number of R&D and prototyping activities have been carried out during the last years to explore the applicability of Micromegas-read gaseous TPCs in rare event searches like double beta decay (DBD), axion…

TREX-DM is conceived to look for low-mass Weakly Interacting Massive Particles (WIMPs) using a gas Time Projection Chamber equipped with micromegas readout planes at the Canfranc Underground Laboratory. The detector can hold in the active…

天体物理仪器与方法 · 物理学 2019-10-23 J. Castel , S. Cebrian , I. Coarasa , T. Dafni , J. Galan , F. J. Iguaz , I. G. Irastorza , G. Luzon , H. Mirallas , A. Ortiz de Solorzano , E. Ruiz-Choliz

The DAMA experiment searches for Weakly Interacting Massive Particle (WIMP) dark matter via its expected but rare interactions within the detector, where the interaction rates will modulate throughout the year due to the orbital motion of…

宇宙学与河外天体物理 · 物理学 2015-06-16 Chris Kelso , Pearl Sandick , Christopher Savage

DARWIN (dark matter wimp search with noble liquids) is a design study for a next-generation, multi-ton dark matter detector in Europe. Liquid argon and/or liquid xenon are the target media for the direct detection of dark matter candidates…

天体物理仪器与方法 · 物理学 2019-08-14 Laura Baudis

The CDMS low ionization threshold experiment (CDMSlite) uses cryogenic germanium detectors operated at a relatively high bias voltage to amplify the phonon signal in the search for weakly interacting massive particles (WIMPs). Results are…

As part of the DarkSide program of direct dark matter searches using liquid argon TPCs, a prototype detector with an active volume containing 10 kg of liquid argon, DarkSide-10, was built and operated underground in the Gran Sasso National…

天体物理仪器与方法 · 物理学 2015-06-04 T. Alexander , D. Alton , K. Arisaka , H. O. Back , P. Beltrame , J. Benziger , G. Bonfini , A. Brigatti , J. Brodsky , L. Cadonati , F. Calaprice , A. Candela , H. Cao , P. Cavalcante , A. Chavarria , A. Chepurnov , D. Cline , A. G. Cocco , C. Condon , D. D'Angelo , S. Davini , E. De Haas , A. Derbin , G. Di Pietro , I. Dratchnev , D. Durben , A. Empl , A. Etenko , A. Fan , G. Fiorillo , K. Fomenko , F. Gabriele , C. Galbiati , S. Gazzana , C. Ghag , C. Ghiano , A. Goretti , L. Grandi , M. Gromov , M. Guan , C. Guo , G. Guray , E. V. Hungerford , Al. Ianni , An. Ianni , A. Kayunov , K. Keeter , C. Kendziora , S. Kidner , V. Kobychev , G. Koh , D. Korablev , G. Korga , E. Shields , P. Li , B. Loer , P. Lombardi , C. Love , L. Ludhova , L. Lukyanchenko , A. Lund , K. Lung , Y. Ma , I. Machulin , J. Maricic , C. J. Martoff , Y. Meng , E. Meroni , P. D. Meyers , T. Mohayai , D. Montanari , M. Montuschi , P. Mosteiro , B. Mount , V. Muratova , A. Nelson , A. Nemtzow , N. Nurakhov , M. Orsini , F. Ortica , M. Pallavicini , E. Pantic , S. Parmeggiano , R. Parsells , N. Pelliccia , L. Perasso , F. Perfetto , L. Pinsky , A. Pocar , S. Pordes , G. Ranucci , A. Razeto , A. Romani , N. Rossi , P. Saggese , R. Saldanha , C. Salvo , W. Sands , M. Seigar , D. Semenov , M. Skorokhvatov , O. Smirnov , A. Sotnikov , S. Sukhotin , Y. Suvorov , R. Tartaglia , J. Tatarowicz , G. Testera , A. Teymourian , J. Thompson , E. Unzhakov , R. B. Vogelaar , H. Wang , S. Westerdale , M. Wojcik , A. Wright , J. Xu , C. Yang , S. Zavatarelli , M. Zehfus , W. Zhong , G. Zuzel

For many working in particle physics and cosmology successful discovery and characterisation of the new particles that most likely explain the non-baryonic cold dark matter, known to comprise the majority of matter in the Universe, would be…

天体物理学 · 物理学 2009-06-23 N. J. Spooner

In the present work we examine the possibility of detecting light dark matter particles (WIMP) utilizing their possible interactions with the electrons. Employing reasonable theoretical models we evaluate the expected event rates in the…

高能物理 - 唯象学 · 物理学 2019-04-11 J. D. Vergados

XENONnT is a dark matter direct detection experiment, utilizing 5.9 t of instrumented liquid xenon, located at the INFN Laboratori Nazionali del Gran Sasso. In this work, we predict the experimental background and project the sensitivity of…

仪器与探测器 · 物理学 2020-11-18 The XENON collaboration , E. Aprile , J. Aalbers , F. Agostini , M. Alfonsi , L. Althueser , F. D. Amaro , V. C. Antochi , E. Angelino , J. R. Angevaare , F. Arneodo , D. Barge , L. Baudis , B. Bauermeister , L. Bellagamba , M. L. Benabderrahmane , T. Berger , A. Brown , E. Brown , S. Bruenner , G. Bruno , R. Budnik , C. Capelli , J. M. R. Cardoso , D. Cichon , B. Cimmino , M. Clark , D. Coderre , A. P. Colijn , J. Conrad , J. P. Cussonneau , M. P. Decowski , A. Depoian , P. Di Gangi , A. Di Giovanni , R. Di Stefano , S. Diglio , A. Elykov , G. Eurin , A. D. Ferella , W. Fulgione , P. Gaemers , R. Gaior , M. Galloway , F. Gao , L. Grandi , C. Hasterok , C. Hils , K. Hiraide , L. Hoetzsch , J. Howlett , M. Iacovacci , Y. Itow , F. Joerg , N. Kato , S. Kazama , M. Kobayashi , G. Koltman , A. Kopec , H. Landsman , R. F. Lang , L. Levinson , Q. Lin , S. Lindemann , M. Lindner , F. Lombardi , J. Long , J. A. M. Lopes , E. López Fune , C. Macolino , J. Mahlstedt , A. Mancuso , L. Manenti , A. Manfredini , F. Marignetti , T. Marrodán Undagoitia , K. Martens , J. Masbou , D. Masson , S. Mastroianni , M. Messina , K. Miuchi , K. Mizukoshi , A. Molinario , K. Morå , S. Moriyama , Y. Mosbacher , M. Murra , J. Naganoma , K. Ni , U. Oberlack , K. Odgers , J. Palacio , B. Pelssers , R. Peres , J. Pienaar , V. Pizzella , G. Plante , J. Qin , H. Qiu , D. Ramírez García , S. Reichard , A. Rocchetti , N. Rupp , J. M. F. dos Santos , G. Sartorelli , N. Šarčević , M. Scheibelhut , J. Schreiner , D. Schulte , M. Schumann , L. Scotto Lavina , M. Selvi , F. Semeria , P. Shagin , E. Shockley , M. Silva , H. Simgen , A. Takeda , C. Therreau , D. Thers , F. Toschi , G. Trinchero , C. Tunnell , K. Valerius , M. Vargas , G. Volta , H. Wang , Y. Wei , C. Weinheimer , M. Weiss , D. Wenz , C. Wittweg , Z. Xu , M. Yamashita , J. Ye , G. Zavattini , Y. Zhang , T. Zhu , J. P. Zopounidis

Liquid Argon Time Projection Chambers are planned to comprise a central role in the future of the U.S. High Energy Physics neutrino program. In particular, this detector technology will form the basis for the 40 kton Deep Underground…

仪器与探测器 · 物理学 2020-09-22 Eric Church , Christopher Jackson , Richard Saldanha

We report the result of a blinded search for Weakly Interacting Massive Particles (WIMPs) using the majority of the SuperCDMS Soudan dataset. With an exposure of 1690 kg days, a single candidate event is observed, consistent with expected…

Various WIMP dark matter searches using the full data set of XMASS-I, a single-phase liquid xenon detector, are reported in this paper. Stable XMASS-I data taking accumulated a total live time of 1590.9 days between November 20, 2013 and…

The Dark Matter Time Projection Chamber (DMTPC) is a low pressure (75 Torr CF4) 10 liter detector capable of measuring the vector direction of nuclear recoils with the goal of directional dark matter detection. In this paper we present the…

Dark matter is a key piece of the current cosmological scenario, with weakly interacting massive particles (WIMPs) a leading dark matter candidate. WIMPs have not been detected in their conventional parameter space (100 GeV $\lesssim…

The worldwide race towards direct dark matter detection in the form of Weakly Interacting Massive Particles (WIMPs) has been dramatically accelerated by the remarkable progress and evolution of liquid xenon time projection chambers…

天体物理仪器与方法 · 物理学 2012-06-28 Elena Aprile , XENON1T collaboration

AMS-02 has reached the sensitivity to probe canonical thermal WIMPs by their annihilation into antiprotons. Due to the high precision of the data, uncertainties in the astrophysical background have become the most limiting factor for…

高能天体物理现象 · 物理学 2018-02-14 Annika Reinert , Martin Wolfgang Winkler

We consider a Dark Matter candidate particle of spin 3/2 with neutrino-like Standard Model strength interactions. In the Majorana case, the particle can account for all of the Dark Matter for a range of masses between 70-160 GeV, depending…

高能物理 - 唯象学 · 物理学 2014-04-02 Konstantin G. Savvidy , J. D. Vergados

We report results of a search for light weakly interacting massive particle (WIMP) dark matter from the CDEX-1 experiment at the China Jinping Underground Laboratory (CJPL). Constraints on WIMP-nucleon spin-independent (SI) and…

Weakly Interacting Massive Particles (WIMPs), are a leading candidate for the dark matter that is observed to constitute ~25% of the total mass-energy density of the Universe. The direct detection of relic WIMPs (those produced during the…

仪器与探测器 · 物理学 2017-08-23 Tarek Saab