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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…

We assess the prospects for indirect detection of Weakly Interacting Massive Particles using a large Liquid Argon TPC detector. Signal events will consist of energetic electron (anti)neutrinos coming from the decay of $\tau$ leptons and $b$…

High Energy Physics - Phenomenology · Physics 2008-11-26 A. Bueno , R. Cid , S. Navas-Concha , D. Hooper , T. J. Weiler

A good particle candidate for Cold Dark Matter (CDM) is the supersymmetric neutralino or more generally a weakly interacting massive particle (WIMP). The expected interaction rate of WIMPs with the detector medium in the direct detection…

Instrumentation and Methods for Astrophysics · Physics 2010-02-17 V. Kozlov

Cosmological observations and the dynamics of the Milky Way provide ample evidence for an invisible and dominant mass component. This so-called dark matter could be made of new, colour and charge neutral particles, which were…

Instrumentation and Methods for Astrophysics · Physics 2014-08-20 Laura Baudis

The Deep Underground Neutrino Experiment (DUNE) is a leading-edge, international experiment for neutrino science and proton decay studies. This experiment is looking for answers regarding several fundamental questions about the nature of…

Instrumentation and Detectors · Physics 2021-08-24 Mihaela Parvu , Ionel Lazanu

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 present the TREX-DM experiment, a low background…

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…

Instrumentation and Methods for Astrophysics · Physics 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

Several experiments have been conducted worldwide, with the goal of observing low-energy nuclear recoils induced by WIMPs scattering off target nuclei in ultra-sensitive, low-background detectors. In the last few decades noble liquid…

Instrumentation and Detectors · Physics 2016-03-23 B. Rossi , A. Anastasio , A. Boiano , S. Catalanotti , A. G. Cocco , G. Covone , P. Di Meo , G. Longo , A. Vanzanella , S. Walker , H. Wang , Y. Wang , G. Fiorillo

Weakly Interacting Massive Particles (WIMPs) are one of the best motivated candidates to compose the Dark Matter of the Universe. The lack of experimental confirmation by direct detection experiments or collider searches has ruled out…

Instrumentation and Detectors · Physics 2025-07-04 Oscar Perez

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 2016-06-22 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 find that it is possible to increase sensitivity to low energy physics in a third or fourth DUNE-like module with careful controls over radiopurity and targeted modifications to a detector similar to the DUNE Far Detector design. In…

A technique using layered wavelength shifting, scintillating and non-scintillating films is presented to achieve discrimination of surface $\alpha$ events from low-energy nuclear recoils in liquid argon detectors. A discrimination power…

Instrumentation and Detectors · Physics 2020-07-08 M. G. Boulay , M. Kuźniak

Simulations of the neutron background for future large-scale particle dark matter detectors are presented. Neutrons were generated in rock and detector elements via spontaneous fission and (alpha,n) reactions, and by cosmic-ray muons. The…

DARk matter WImp search with liquid xenoN (DARWIN) will be an experiment for the direct detection of dark matter using a multi-ton liquid xenon time projection chamber at its core. Its primary goal will be to explore the experimentally…

Instrumentation and Methods for Astrophysics · Physics 2016-12-02 J. Aalbers , F. Agostini , M. Alfonsi , F. D. Amaro , C. Amsler , E. Aprile , L. Arazi , F. Arneodo , P. Barrow , L. Baudis , M. L. Benabderrahmane , T. Berger , B. Beskers , A. Breskin , P. A. Breur , A. Brown , E. Brown , S. Bruenner , G. Bruno , R. Budnik , L. Buetikofer , J. Calven , J. M. R. Cardoso , D. Cichon , D. Coderre , A. P. Colijn , J. Conrad , J. P. Cussonneau , M. P. Decowski , S. Diglio , G. Drexlin , E. Duchovni , E. Erdal , G. Eurin , A. Ferella , A. Fieguth , W. Fulgione , A. Gallo Rosso , P. Di Gangi , A. Di Giovanni , M. Galloway , M. Garbini , C. Geis , F. Glueck , L. Grandi , Z. Greene , C. Grignon , C. Hasterok , V. Hannen , E. Hogenbirk , J. Howlett , D. Hilk , C. Hils , A. James , B. Kaminsky , S. Kazama , B. Kilminster , A. Kish , L. M. Krauss , H. Landsman , R. F. Lang , Q. Lin , F. L. Linde , S. Lindemann , M. Lindner , J. A. M. Lopes , T. Marrodan Undagoitia , J. Masbou , F. V. Massoli , D. Mayani , M. Messina , K. Micheneau , A. Molinario , K. D. Mora , E. Morteau , M. Murra , J. Naganoma , J. L. Newstead , K. Ni , U. Oberlack , P. Pakarha , B. Pelssers , P. de Perio , R. Persiani , F. Piastra , M. C. Piro , G. Plante , L. Rauch , S. Reichard , A. Rizzo , N. Rupp , J. M. F. Dos Santos , G. Sartorelli , M. Scheibelhut , S. Schindler , M. Schumann , J. Schreiner , L. Scotto Lavina , M. Selvi , P. Shagin , M. C. Silva , H. Simgen , P. Sissol , M. von Sivers , D. Thers , J. Thurn , A. Tiseni , R. Trotta , C. D. Tunnell , K. Valerius , M. A. Vargas , H. Wang , Y. Wei , C. Weinheimer , T. Wester , J. Wulf , Y. Zhang , T. Zhu , K. Zuber

Dark matter detectors using the liquid noble gases xenon and argon as WIMP targets have evolved rapidly in the last decade and will continue to play a major role in the field. Due to the possibility to scale these detectors to larger masses…

Instrumentation and Methods for Astrophysics · Physics 2012-06-12 Marc Schumann

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 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…

Presented here are results of simulations of neutron background performed for a time projection chamber acting as a particle dark matter detector in an underground laboratory. The investigated background includes neutrons from rock and…