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The Argon Dark Matter (ArDM-1t) experiment is a ton-scale liquid argon (LAr) double-phase time projection chamber designed for direct Dark Matter searches. Such a device allows to explore the low energy frontier in LAr. After successful…

The Argon Dark Matter (ArDM) experiment consists of a liquid argon (LAr) time projection chamber (TPC) sensitive to nuclear recoils resulting from scattering of hypothetical Weakly Interacting Massive Particles (WIMPs) on argon targets.…

The ArDM project aims at developing and operating large noble liquid detectors to search for direct evidence of Weakly Interacting Massive Particle (WIMP) as Dark Matter in the Universe. The initial goal is to design, assemble and operate a…

High Energy Physics - Phenomenology · Physics 2009-11-11 A. Rubbia

The aim of the ArDM project is the development and operation of a one ton double-phase liquid argon detector for direct Dark Matter searches. The detector measures both the scintillation light and the ionization charge from ionizing…

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

ArDM-1t is the first operating ton-scale liquid argon detector for direct search of Dark Matter particles. Developed at CERN as Recognized Experiment RE18, the experiment has been approved in 2010 to be installed in the Spanish underground…

ArDM is a new-generation WIMP detector which will measure simultaneously light and charge from scintillation and ionization of liquid argon. Our goal is to construct, characterize and operate a 1 ton liquid argon underground detector. The…

Instrumentation and Detectors · Physics 2015-05-13 Vittorio Boccone

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 nucleus, producing nuclear recoils. These events will be discerned by their light to…

Instrumentation and Detectors · Physics 2010-03-26 Christian Regenfus

The Dark Matter part of the universe presumably consists of WIMPs (Weakly Interacting Massive Particles). The ArDM project aims at measuring signals induced by WIMPs in a liquid argon detector. A 1-ton prototype is currently developed with…

High Energy Physics - Phenomenology · Physics 2008-11-26 L. Kaufmann , A. Rubbia

The Argon Dark Matter experiment is a ton-scale double phase argon Time Projection Chamber designed for direct Dark Matter searches. It combines the detection of scintillation light together with the ionisation charge in order to…

WIMPs (Weakly Interacting Massive Particles) are considered the main candidates for Cold Dark Matter. The ArDM experiment aims at measuring signals directly induced by WIMPs in liquid argon. A 1-ton prototype is currently developed with the…

High Energy Physics - Phenomenology · Physics 2009-11-13 M. Laffranchi , A. Rubbia

Large liquid argon detectors offer one of the best avenues for the detection of galactic weakly interacting massive particles (WIMPs) via their scattering on atomic nuclei. The liquid argon target allows exquisite discrimination between…

Instrumentation and Methods for Astrophysics · Physics 2020-04-22 The DarkSide Collaboration , C. E. Aalseth , S. Abdelhakim , F. Acerbi , P. Agnes , R. Ajaj , I. F. M. Albuquerque , T. Alexander , A. Alici , A. K. Alton , P. Amaudruz , F. Ameli , J. Anstey , P. Antonioli , M. Arba , S. Arcelli , R. Ardito , I. J. Arnquist , P. Arpaia , D. M. Asner , A. Asunskis , M. Ave , H. O. Back , A. Barrado Olmedo , G. Batignani , M. G. Bisogni , V. Bocci , A. Bondar , G. Bonfini , W. Bonivento , E. Borisova , B. Bottino , M. G. Boulay , R. Bunker , S. Bussino , A. Buzulutskov , M. Cadeddu , M. Cadoni , A. Caminata , N. Canci , A. Candela , C. Cantini , M. Caravati , M. Cariello , F. Carnesecchi , M. Carpinelli , A. Castellani , P. Castello , S. Catalanotti , V. Cataudella , P. Cavalcante , D. Cavazza , S. Cavuoti , S. Cebrian , J. M. Cela Ruiz , B. Celano , R. Cereseto , W. Cheng , A. Chepurnov , C. Cicalò , L. Cifarelli , M. Citterio , A. G. Cocco , V. Cocco , M. Colocci , L. Consiglio , F. Cossio , G. Covone , P. Crivelli , I. D'Antone , M. D'Incecco , D. D'Urso , M. D. Da Rocha Rolo , O. Dadoun , M. Daniel , S. Davini , A. De Candia , S. De Cecco , M. De Deo , A. De Falco , G. De Filippis , D. De Gruttola , G. De Guido , G. De Rosa , G. Dellacasa , P. Demontis , S. DePaquale , A. V. Derbin , A. Devoto , F. Di Eusanio , L. Di Noto , G. Di Pietro , P. Di Stefano , C. Dionisi , G. Dolganov , F. Dordei , M. Downing , F. Edalatfar , A. Empl , M. Fernandez Diaz , A. Ferri , C. Filip , G. Fiorillo , K. Fomenko , A. Franceschi , D. Franco , G. E. Froudakis , F. Gabriele , A. Gabrieli , C. Galbiati , P. Garcia Abia , D. Gascón Fora , A. Gendotti , C. Ghiano , A. Ghisi , S. Giagu , P. Giampa , R. A. Giampaolo , C. Giganti , M. A. Giorgi , G. K. Giovanetti , M. L. Gligan , A. Gola , O. Gorchakov , M. Grab , R. Graciani Diaz , F. Granato , M. Grassi , J. W. Grate , G. Y. Grigoriev , A. Grobov , M. Gromov , M. Guan , M. B. B. Guerra , M. Guerzoni , M. Gulino , R. K. Haaland , B. R. Hackett , A. Hallin , B. Harrop , E. W. Hoppe , S. Horikawa , B. Hosseini , F. Hubaut , P. Humble , E. V. Hungerford , An. Ianni , A. Ilyasov , V. Ippolito , C. Jillings , K. Keeter , C. L. Kendziora , S. Kim , I. Kochanek , K. Kondo , G. Kopp , D. Korablev , G. Korga , A. Kubankin , R. Kugathasan , M. Kuss , M. Kuźniak , M. La Commara , L. La Delfa , M. Lai , S. Langrock , M. Lebois , B. Lehnert , N. Levashko , X. Li , Q. Liqiang , M. Lissia , G. U. Lodi , G. Longo , R. López Manzano , R. Lussana , L. Luzzi , A. A. Machado , I. N. Machulin , A. Mandarano , L. Mapelli , M. Marcante , A. Margotti , S. M. Mari , M. Mariani , J. Maricic , M. Marinelli , D. Marras , M. Martínez , J. J. Martínez Morales , A. D. Martinez Rojas , C. J. Martoff , M. Mascia , J. Mason , A. Masoni , A. Mazzi , A. B. McDonald , A. Messina , P. D. Meyers , T. Miletic , R. Milincic , A. Moggi , S. Moioli , J. Monroe , M. Morrocchi , T. Mroz , W. Mu , V. N. Muratova , S. Murphy , C. Muscas , P. Musico , R. Nania , T. Napolitano , A. Navrer Agasson , M. Nessi , I. Nikulin , A. Oleinik , V. Oleynikov , M. Orsini , F. Ortica , L. Pagani , M. Pallavicini , S. Palmas , L. Pandola , E. Pantic , E. Paoloni , G. Paternoster , V. Pavletcov , F. Pazzona , S. Peeters , P. A. Pegoraro , K. Pelczar , L. A. Pellegrini , C. Pellegrino , N. Pelliccia , F. Perotti , V. Pesudo , E. Picciau , C. Piemonte , F. Pietropaolo , A. Pocar , T. Pollman , D. Portaluppi , S. S. Poudel , P. Pralavorio , D. Price , B. Radics , F. Raffaelli , F. Ragusa , M. Razeti , A. Razeto , V. Regazzoni , C. Regenfus , A. L. Renshaw , S. Rescia , M. Rescigno , F. Retiere , L. P. Rignanese , A. Rivetti , A. Romani , L. Romero , N. Rossi , A. Rubbia , D. Sablone , P. Sala , P. Salatino , O. Samoylov , E. Sánchez García , S. Sanfilippo , M. Sant , D. Santone , R. Santorelli , C. Savarese , E. Scapparone , B. Schlitzer , G. Scioli , E. Segreto , A. Seifert , D. A. Semenov , A. Shchagin , A. Sheshukov , S. Siddhanta , M. Simeone , P. N. Singh , P. Skensved , M. D. Skorokhvatov , O. Smirnov , G. Sobrero , A. Sokolov , A. Sotnikov , R. Stainforth , A. Steri , S. Stracka , V. Strickland , G. B. Suffritti , S. Sulis , Y. Suvorov , A. M. Szelc , R. Tartaglia , G. Testera , T. Thorpe , A. Tonazzo , A. Tosi , M. Tuveri , E. V. Unzhakov , G. Usai , A. Vacca , E. Vázquez-Jáuregui , M. Verducci , T. Viant , S. Viel , F. Villa , A. Vishneva , R. B. Vogelaar , M. Wada , J. Wahl , J. J. Walding , H. Wang , Y. Wang , S. Westerdale , R. J. Wheadon , R. Williams , J. Wilson , Marcin Wojcik , Mariusz Wojcik , S. Wu , X. Xiao , C. Yang , Z. Ye , M. Zuffa , G. Zuzel

The ArDM project aims at operating a large noble liquid detector to search for direct evidence of Weakly Interacting Massive Particles (WIMP) as Dark Matter in the universe. Background sources relevant to ton-scale liquid and gaseous argon…

High Energy Physics - Phenomenology · Physics 2016-11-09 L. Kaufmann , A. Rubbia

ArDM-1t is the prototype for a next generation WIMP detector measuring both the scintillation light and the ionization charge from nuclear recoils in a 1-ton liquid argon target. The goal is to reach a minimum recoil energy of 30\,keVr to…

One of the most powerful techniques for direct detection of dark matter via elastic scattering of galactic WIMPs is the use of liquid argon time projection chambers. Atmospheric argon (AAr) has a naturally occurring radioactive isotope,…

Instrumentation and Detectors · Physics 2020-08-12 E. Sánchez García

Liquid Argon Time Projection Chamber (LAr TPC) detectors are ideally suited for studying neutrino interactions and probing the parameters that characterize neutrino oscillations. The ability to drift ionization particles over long distances…

Instrumentation and Detectors · Physics 2010-02-04 M. Soderberg

Large (up to $\sim 100$ kt) liquid argon time-projection chamber detectors are presently being considered for proton decay searches and neutrino astrophysics, as well as for far detectors for the next generation of long-baseline neutrino…

Instrumentation and Detectors · Physics 2015-06-16 Alberto Marchionni

In this paper we describe the design, construction, and operation of a first large area double-phase liquid argon Large Electron Multiplier Time Projection Chamber (LAr LEM-TPC). The detector has a maximum drift length of 60 cm and the…

Large liquid argon (LAr) detectors, up to 100 kton scale, are presently being considered for proton decay searches and neutrino astrophysics as well as far detectors for the next generation of long baseline neutrino oscillation experiments,…

Instrumentation and Detectors · Physics 2009-12-23 A. Marchionni

Liquid argon (LAr) with a high light yield of approximately 40 photons per keV is an attractive target for the direct detection of weakly interacting massive particles (WIMPs), which are well motivated galactic dark matter candidates. We…

Instrumentation and Detectors · Physics 2018-06-26 X. Zhu , Z. Shen , C. Feng , S. Liu , Q. An
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