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Related papers: The ArDM project: a Liquid Argon TPC for Dark Matt…

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Observational evidence for dark matter can be explained by Weakly Interacting Massive Particles (WIMPs). These dark matter particle candidates could indirectly be detected through the observation of signals produced as part of WIMP…

High Energy Astrophysical Phenomena · Physics 2015-06-11 Carsten Rott

In this study, the sensitivity of future lepton colliders to WIMP dark matter is evaluated assuming WIMP pair production accompanied by a photon from initial state radiation, through which the process can be identified. A full detector…

High Energy Physics - Experiment · Physics 2020-05-06 Moritz Habermehl , Mikael Berggren , Jenny List

Weakly interacting massive particles (WIMPs) are amongst the most interesting dark matter (DM) candidates. Many DM candidates naturally arise in theories beyond the standard model (SM) of particle physics, like weak-scale supersymmetry…

Cosmology and Nongalactic Astrophysics · Physics 2015-03-17 Yashar Akrami , Christopher Savage , Pat Scott , Jan Conrad , Joakim Edsjö

This review on weakly interacting massive particle (WIMP) dark matter direct detection focuses on experimental approaches and the corresponding physics basics. The presentation is intended to provide a quick and concise introduction for…

Astrophysics · Physics 2014-10-13 Y. Ramachers

Dark matter detection experiments using liquid argon rely on a precise characterization of the ionization response to nuclear recoils, especially in the keV energy range relevant for light dark matter interactions. In this work, we present…

High Energy Physics - Experiment · Physics 2026-05-14 F. Acerbi , P. Adhikari , P. Agnes , I. Ahmad , S. Albergo , I. F. Albuquerque , T. Alexander , A. K. Alton , P. Amaudruz , M. Angiolilli , E. Aprile , M. Atzori Corona , D. J. Auty , M. Ave , I. C. Avetisov , O. Azzolini , H. O. Back , Z. Balmforth , A. I. Barrado Olmedo , P. Barrillon , G. Batignani , S. Bharat , P. Bhowmick , S. Blua , V. Bocci , W. Bonivento , B. Bottino , M. G. Boulay , T. Braun , A. Buchowicz , S. Bussino , J. Busto , M. Cadeddu , R. Calabrese , V. Camillo , A. Caminata , N. Canci , M. Caravati , M. Cárdenas-Montes , N. Cargioli , M. Carlini , P. Cavalcante , S. Cebrian , S. Chashin , A. Chepurnov , S. Choudhary , L. Cifarelli , B. Cleveland , Y. Coadou , I. Coarasa , V. Cocco , E. Conde Vilda , L. Consiglio , A. F. V. Cortez , B. S. Costa , M. Czubak , S. D'Auria , M. D. Da Rocha Rolo , A. Dainty , G. Darbo , S. Davini , R. de Asmundis , S. De Cecco , M. De Napoli , G. Dellacasa , A. V. Derbin , L. Di Noto , P. Di Stefano , L. K. Dias , D. Díaz Mairena , C. Dionisi , G. Dolganov , F. Dordei , V. Dronik , A. Elersich , T. Erjavec , N. Fearon , M. Fernández Díaz , L. Ferro , A. Ficorella , G. Fiorillo , D. Fleming , P. Franchini , D. Franco , H. Frandini Gatti , E. Frolov , F. Gabriele , D. Gahan , C. Galbiati , G. Galiński , G. Gallina , M. Garbini , P. Garcia Abia , A. Gawdzik , G. K. Giovanetti , V. Goicoechea Casanueva , A. Gola , L. Grandi , G. Grauso , G. Grilli di Cortona , A. Grobov , M. Gromov , J. Guerrero Cánovas , M. Gulino , B. R. Hackett , A. L. Hallin , M. Haranczyk , B. Harrop , T. Hessel , C. Hidalgo , J. Hollingham , J. Hu , F. Hubaut , D. Huff , T. Hugues , E. V. Hungerford , An. Ianni , V. Ippolito , A. Jamil , C. Jillings , R. Keloth , N. Kemmerich , M. Kimura , A. Klenin , K. Kondo , G. Korga , L. Kotsiopoulou , S. Koulosousas , A. Kubankin , P. Kunzé , M. Kuss , M. Kuźniak , M. Kuzwa , M. La Commara , M. Lai , E. Le Guirriec , E. Leason , A. Leoni , L. Lidey , J. Lipp , M. Lissia , L. Luzzi , O. Lychagina , O. Macfadyen , I. Machts , I. N. Machulin , S. Manecki , I. Manthos , L. Mapelli , A. Marasciulli , S. M. Mari , C. Mariani , J. Maricic , M. Martinez , C. J. Martoff , G. Matteucci , K. Mavrokoridis , A. B. McDonald , S. Merzi , A. Messina , R. Milincic , S. Minutoli , A. Mitra , J. Monroe , M. Morrocchi , A. Morsy , V. N. Muratova , M. Murra , P. Musico , R. Nania , M. Nessi , G. Nieradka , K. Nikolopoulos , E. Nikoloudaki , I. Nikulin , J. Nowak , K. Olchanski , A. Oleinik , V. Oleynikov , P. Organtini , A. Ortiz de Solórzano , A. Padmanabhan , M. Pallavicini , L. Pandola , E. Pantic , E. Paoloni , D. Papi , B. Park , G. Pastuszak , G. Paternoster , R. Pavarani , A. Peck , K. Pelczar , R. Perez , V. Pesudo , S. Piacentini , N. Pino , G. Plante , A. Pocar , S. Pordes , P. Pralavorio , E. Preosti , D. Price , M. Pronesti , S. Puglia , M. Queiroga Bazetto , F. Raffaelli , F. Ragusa , Y. Ramachers , A. Ramirez , S. Ravinthiran , M. Razeti , A. L. Renshaw , A. Repond , M. Rescigno , S. Resconi , F. Retiere , L. P. Rignanese , A. Ritchie-Yates , A. Rivetti , A. Roberts , C. Roberts , G. Rogers , L. Romero , M. Rossi , D. Rudik , J. Runge , M. A. Sabia , D. Sablone , P. Salomone , O. Samoylov , S. Sanfilippo , D. Santone , R. Santorelli , E. M. Santos , I. Sargeant , M. L. Sarsa , C. Savarese , E. Scapparone , F. G. Schuckman , D. A. Semenov , C. Seoane , M. Sestu , V. Shalamova , S. Sharma Poudel , A. Sheshukov , M. Simeone , P. Skensved , M. D. Skorokhvatov , O. Smirnov , T. Smirnova , B. Smith , F. Spadoni , M. Spangenberg , A. Steri , V. Stornelli , S. Stracka , A. Sung , C. Sunny , Y. Suvorov , A. M. Szelc , O. Taborda , R. Tartaglia , A. Taylor , J. Taylor , G. Testera , K. Thieme , A. Thompson , S. Torres-Lara , A. Tricomi , S. Tullio , E. V. Unzhakov , M. Van Uffelen , P. Ventura , G. Vera Díaz , S. Viel , A. Vishneva , R. B. Vogelaar , J. Vossebeld , B. Vyas , M. Wada , M. Walczak , Y. Wang , S. Westerdale , L. Williams , M. M. Wojcik , M. Wojcik , C. Yang , J. Yin , A. Zabihi , P. Zakhary , A. Zani , Y. Zhang , T. Zhu , A. Zichichi , G. Zuzel , M. P. Zykova

We report on the measurement of the specific activity of Ar-39 in natural argon. The measurement was performed with a 2.3-liter two-phase (liquid and gas) argon drift chamber. The detector was developed by the WARP Collaboration as a…

One of the major challenges of modern physics is to decipher the nature of dark matter. Astrophysical observations provide ample evidence for the existence of an invisible and dominant mass component in the observable universe, from the…

Cosmology and Nongalactic Astrophysics · Physics 2015-09-04 Laura Baudis

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

Light cold dark matter consisting of weakly interacting slim (or sub-eV) particles (WISPs) has been in the focus of a large number of studies made over the past two decades. The QCD axion and axion-like particles with masses in the…

High Energy Physics - Experiment · Physics 2014-10-24 Dieter Horns , Axel Lindner , Andrei Lobanov , Andreas Ringwald

The DARWIN/XLZD experiment is a next-generation dark matter detector with a multi-ten-ton liquid xenon time projection chamber at its core. Its principal goal will be to explore the experimentally accessible parameter space for Weakly…

Instrumentation and Methods for Astrophysics · Physics 2024-05-01 Laura Baudis

Liquid xenon and liquid argon detectors are leading the direct dark matter search and are expected to be the candidate technology for the forthcoming generation of ultra-sensitive large-mass detectors. At present, the scintillation light…

High Energy Physics - Experiment · Physics 2022-09-20 Alessandro Razeto , Nicola Rossi

Dark Matter experiments are recently focusing their detection techniques in low-mass WIMPs, which requires the use of light elements and low energy threshold. In this context, we describe the TREX-DM experiment, a low background…

Instrumentation and Detectors · Physics 2015-09-08 F. J. Iguaz , J. G. Garza , F. Aznar , J. F. Castel , S. Cebrian , T. Dafni , J. A. Garcia , I. G. Irastorza , A. Lagraba , G. Luzon , A. Peiro

We investigate novel strategies to extend the sensitivity of dark matter direct detection experiments to energy deposits well below the thresholds of conventional detectors. In liquid-argon time-projection chambers equipped with silicon…

Instrumentation and Detectors · Physics 2026-01-12 Faeq Abed , Asmaa AlMellah , Kareem Al-Jubouri , Alex Lumoski

The DEAP-3600 experiment uses 3.6 tons of liquid argon for a sensitive dark matter search, with a sensitivity to the spin-independent WIMP-nucleon cross-section of $10^{-46}$ cm$^2$ at 100 GeV WIMP mass. This high sensitivity is achievable…

Instrumentation and Methods for Astrophysics · Physics 2019-08-14 Bei Cai

We review several current aspects of dark matter theory and experiment. We overview the present experimental status, which includes current bounds and recent claims and hints of a possible signal in a wide range of experiments: direct…

High Energy Physics - Phenomenology · Physics 2018-06-13 Leszek Roszkowski , Enrico Maria Sessolo , Sebastian Trojanowski

The ARAPUCA is a novel concept for liquid argon scintillation light detection which has been proposed for the photon detection system of the Deep Underground Neutrino Experiment. The test in liquid argon of one of the first ARAPUCA…

Discrimination between electron and nuclear recoil events in a liquid argon scintillation detector has been demonstrated with simulations by using the differences in the scintillation photon time distribution between these classes of…

Astrophysics · Physics 2007-05-23 M. G. Boulay , A. Hime

In the last decade, Direct Dark Matter searches has become a very active research program, spawning dozens of projects world wide and leading to contradictory results. It is on this stage that the Dark matter Experiment with liquid Argon…

Instrumentation and Methods for Astrophysics · Physics 2014-06-03 P. Gorel

Weakly interactive slim particles (WISPs), including the QCD axion, axion-like particles (ALPs), and hidden photons, are considered to be strong candidates for the dark matter carrier particle. The microwave cavity experiment WISPDMX is the…

Instrumentation and Detectors · Physics 2015-11-11 Le Hoang Nguyen , Dieter Horns , Andrei Lobanov , Andreas Ringwald

We are conducting an experiment to search for WIMPs, or weakly-interacting massive particles, in the galactic halo using terrestrial detectors. This generic class of hypothetical particles, whose properties are similar to those predicted by…