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The DarkSide-20k experiment represents the present goal of the Global Argon Dark Matter Collaboration program. Bringing together the experience from previous argon-based detectors, as well as the knowledge gained on large volume membrane…

Instrumentation and Detectors · Physics 2025-12-01 Andrea Zani

We propose a new beam-dump experiment, SHADOWS, to search for a large variety of feebly-interacting particles possibly produced in the interactions of a 400 GeV proton beam with a high-Z material dump. SHADOWS will use the 400 GeV primary…

A brief outline of Dark Matter detection experiments using liquid argon technology is presented. The Pulse Shape background discrimination method (PSD) is described and the example of its use in 2.3 l R&D detector is given. Methods of…

Instrumentation and Detectors · Physics 2019-08-14 Pawel Kryczynski

The DAMIC experiment employs large-area, thick charge-coupled devices (CCDs) to search for the interactions of low-mass dark matter particles in the galactic halo with silicon atoms in the CCD target. From 2017 to 2019, DAMIC collected data…

Cosmology and Nongalactic Astrophysics · Physics 2022-10-04 Alvaro E. Chavarria

We search for dark matter in the form of axionlike particles (ALPs) in the mass range $5.576741 \,\mathrm{neV/c^2}$ - $5.577733\,\mathrm{neV/c^2}$ by probing their possible coupling to fermion spins through the ALP field gradient. This is…

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

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…

Instrumentation and Detectors · Physics 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

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

We report direct-detection constraints on light dark matter particles interacting with electrons. The results are based on a method that exploits the extremely low levels of leakage current of the DAMIC detector at SNOLAB of…

We report results of a 14.1 kgd measurement with 15 superheated droplet detectors of total active mass 0.208 kg, comprising the first stage of a 30 kgd Phase II experiment. In combination with the results of the neutron-spin sensitive…

Cosmology and Nongalactic Astrophysics · Physics 2010-12-03 M. Felizardo , T. Morlat , A. C. Fernandes , TA Girard , J. G. Marques , A. R. Ramos , M. Auguste , D. Boyer , A. Cavaillou , C. Sudre , J. Poupeney , R. F. Payne , H. S. Miley , J. Puibasset

The Cryogenic Dark Matter search experiment (CDMS) employs low-temperature Ge and Si detectors to detect WIMPs via their elastic scattering of target nuclei. The last analysis with an germanium exposure of 397.8 kg-days resulted in zero…

Instrumentation and Methods for Astrophysics · Physics 2019-08-13 T. Bruch

The search for dark matter has been performed mainly for weakly interacting massive particles and massive compact halo objects, and the intermediate mass region has not been investigated experimentally. A method to search dark matter with…

Instrumentation and Detectors · Physics 2019-01-23 Akio Kawasaki

New light particles may be produced in large numbers in the far-forward region at the LHC and then decay to dark matter, which can be detected through its scattering in far-forward experiments. We consider the example of invisibly-decaying…

High Energy Physics - Phenomenology · Physics 2021-04-28 Brian Batell , Jonathan L. Feng , Sebastian Trojanowski

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

The ArDM experiment, a 1 ton liquid argon TPC/Calorimeter, is designed for the detection of dark matter particles which can scatter off the spinless argon nuclei. These events producing a recoiling nucleus will be discerned by their light…

Instrumentation and Detectors · Physics 2008-12-09 C. Regenfus

The ZEPLIN-III experiment in the Palmer Underground Laboratory at Boulby uses a 12kg two-phase xenon time projection chamber to search for the weakly interacting massive particles (WIMPs) that may account for the dark matter of our Galaxy.…

DarkSide-50 is the first physics detector of the DarkSide dark matter search program. The detector features a dual-phase underground-argon Time Projection Chamber (TPC) of 50 kg active mass surrounded by an organic liquid-scintillator…

Instrumentation and Detectors · Physics 2019-08-13 Alden Fan

A search for dark matter using an underground single-phase liquid xenon detector was conducted at the Kamioka Observatory in Japan, particularly for Weakly Interacting Massive Particles (WIMPs). We have used 705.9 live days of data in a…

We report on a search for Weakly Interacting Massive Particles (WIMPs) using 278.8 days of data collected with the XENON1T experiment at LNGS. XENON1T utilizes a liquid xenon time projection chamber with a fiducial mass of $(1.30 \pm 0.01)$…

Cosmology and Nongalactic Astrophysics · Physics 2018-09-14 E. Aprile , J. Aalbers , F. Agostini , M. Alfonsi , L. Althueser , F. D. Amaro , M. Anthony , F. Arneodo , L. Baudis , B. Bauermeister , M. L. Benabderrahmane , T. Berger , P. A. Breur , A. Brown , A. Brown , E. Brown , S. Bruenner , G. Bruno , R. Budnik , C. Capelli , J. M. R. Cardoso , 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 , A. Elykov , G. Eurin , J. Fei , A. D. Ferella , A. Fieguth , W. Fulgione , A. Gallo Rosso , M. Galloway , F. Gao , M. Garbini , C. Geis , L. Grandi , Z. Greene , H. Qiu , C. Hasterok , E. Hogenbirk , J. Howlett , R. Itay , F. Joerg , B. Kaminsky , S. Kazama , A. Kish , G. Koltman , H. Landsman , R. F. Lang , L. Levinson , Q. Lin , S. Lindemann , M. Lindner , F. Lombardi , J. A. M. Lopes , J. Mahlstedt , A. Manfredini , T. Marrodán Undagoitia , J. Masbou , D. Masson , M. Messina , K. Micheneau , K. Miller , A. Molinario , K. Morå , M. Murra , J. Naganoma , K. Ni , U. Oberlack , B. Pelssers , F. Piastra , J. Pienaar , V. Pizzella , G. Plante , R. Podviianiuk , N. Priel , D. Ramírez García , L. Rauch , S. Reichard , C. Reuter , B. Riedel , A. Rizzo , A. Rocchetti , N. Rupp , J. M. F. dos Santos , G. Sartorelli , M. Scheibelhut , S. Schindler , J. Schreiner , D. Schulte , M. Schumann , L. Scotto Lavina , M. Selvi , P. Shagin , E. Shockley , M. Silva , H. Simgen , D. Thers , F. Toschi , G. Trinchero , C. Tunnell , N. Upole , M. Vargas , O. Wack , H. Wang , Z. Wang , Y. Wei , C. Weinheimer , C. Wittweg , J. Wulf , J. Ye , Y. Zhang , T. Zhu