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XENON is a novel liquid xenon experiment concept for a sensitive dark matter search using a 1-tonne active target, distributed in an array of ten independent time projection chambers. The design relies on the simultaneous detection of…

Liquid Argon Time Projection Chamber 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 in…

Instrumentation and Detectors · Physics 2009-10-20 M. Soderberg

The search for dark matter weakly interacting massive particles with noble liquids has probed masses down and below a GeV/c^2. The ultimate limit is represented by the experimental threshold on the energy transfer to the nuclear recoil.…

High Energy Physics - Phenomenology · Physics 2020-11-11 Giovanni Grilli di Cortona , Andrea Messina , Stefano Piacentini

ArgoNeuT, or Argon Neutrino Test, is a 170 liter liquid argon time projection chamber designed to collect neutrino interactions from the NuMI beam at Fermi National Accelerator Laboratory. ArgoNeuT operated in the NuMI low-energy beam line…

The PICASSO dark matter search experiment operated an array of 32 superheated droplet detectors containing 3.0 kg of C$_{4}$F$_{10}$ and collected an exposure of 231.4 kgd at SNOLAB between March 2012 and January 2014. We report on the…

The Deep Underground Neutrino Experiment (DUNE) is a leading-edge experiment for long-baseline neutrino oscillation studies, neutrino astrophysics and nucleon decay searches. ProtoDUNE-Dual Phase (DP) is a 6x6x6 m$^3$ liquid argon…

Instrumentation and Detectors · Physics 2022-01-19 I. Gil-Botella

This paper describes the design and performance of a compact detector, BDX-MINI, that incorporates all features of a concept that optimized the detection of light dark matter produced by electrons in a beam dump. It represents a reduced…

Weakly Interacting Massive Particles (WIMPs) are the candidates of dark matter in our universe. Up to now any direct interaction of WIMP with nuclei has not been observed yet. The exclusion limits of the spin-independent cross section of…

The detection and characterization of lunar water are critical for enabling sustainable human and robotic exploration of the Moon. Orbital neutron spectrometers, such as instruments on Lunar Prospector and the Lunar Reconnaissance Orbiter,…

Driven by the null results in the searches for dark matter, the field of direct dark matter detection is constantly evolving to push new frontiers. Ultimately, a vast parameter space for dark matter masses below a few GeV is yet to be…

High Energy Physics - Experiment · Physics 2025-12-18 Melih Solmaz

XENON is a project for direct dark matter search located in the INFN underground laboratory LNGS. The previous generation of XENON detector, XENON1T, achieved an exposure of 1 ton$\times$year, setting the most stringent limits on the…

High Energy Physics - Experiment · Physics 2023-10-18 S. E. M. Ahmed Maouloud

The Scintillating Bubble Chamber (SBC) Collaboration is designing a new generation of low background, noble liquid bubble chamber experiments with sub-keV nuclear recoil threshold. These experiments combine the electronic recoil blindness…

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

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

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…

Instrumentation and Methods for Astrophysics · Physics 2012-06-28 Elena Aprile , XENON1T collaboration

The Deep Underground Neutrino Experiment (DUNE) will be the next generation long-baseline neutrino experiment. The far detector is designed as a complex of four LAr-TPC (Liquid Argon Time Projection Chamber) modules with 17 kt of liquid…

Instrumentation and Detectors · Physics 2022-01-11 Niccolò Gallice

In the direct detection of the galactic dark matter, experiments using cryogenic solid-state detectors or noble liquids play for years a very relevant role, with increasing target mass and more and more complex detection systems. But…

Instrumentation and Methods for Astrophysics · Physics 2021-03-31 Susana Cebrian

DarkSide-20k is a novel liquid argon dark matter detector currently under construction at the Laboratori Nazionali del Gran Sasso (LNGS) of the Istituto Nazionale di Fisica Nucleare (INFN) that will push the sensitivity for Weakly…

Instrumentation and Detectors · Physics 2025-03-20 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. Barrado Olmedo , P. Barrillon , G. Batignani , P. Bhowmick , M. Bloem , S. Blua , V. Bocci , W. Bonivento , B. Bottino , M. G. Boulay , A. Buchowicz , S. Bussino , J. Busto , M. Cadeddu , M. Cadoni , R. Calabrese , V. Camillo , A. Caminata , N. Canci , A. Capra , M. Caravati , M. Cardenas-Montes , N. Cargioli , M. Carlini , P. Castello , P. Cavalcante , S. Cebrian , J. Cela Ruiz , S. Chashin , A. Chepurnov , L. Cifarelli , D. Cintas , B. Cleveland , Y. Coadou , V. Cocco , D. Colaiuda , E. Conde Vilda , L. Consiglio , B. S. Costa , M. Czubak , S. D'Auria , M. D. Da Rocha Rolo , G. Darbo , S. Davini , R. de Asmundis , S. De Cecco , G. Dellacasa , A. V. Derbin , F. Di Capua , L. Di Noto , P. Di Stefano , L. K. Dias , C. Dionisi , G. Dolganov , F. Dordei , V. Dronik , A. Elersich , E. Ellingwood , T. Erjavec , N. Fearon , M. Fernandez Diaz , A. Ficorella , G. Fiorillo , P. Franchini , D. Franco , H. Frandini Gatti , E. Frolov , F. Gabriele , D. Gahan , C. Galbiati , G. Galiski , G. Gallina , G. Gallus , M. Garbini , P. Garcia Abia , A. Gawdzik , A. Gendotti , G. K. Giovanetti , V. Goicoechea Casanueva , A. Gola , L. Grandi , G. Grauso , G. Grilli di Cortona , A. Grobov , M. Gromov , M. Gulino , C. Guo , B. R. Hackett , A. Hallin , A. Hamer , M. Haranczyk , T. Hessel , S. Horikawa , J. Hu , F. Hubaut , J. Hucker , T. Hugues , E. V. Hungerford , A. Ianni , G. Ippoliti , V. Ippolito , A. Jamil , C. Jillings , R. Keloth , N. Kemmerich , A. Kemp , Carlos E. Kester , M. Kimura , K. Kondo , G. Korga , L. Kotsiopoulou , S. Koulosousas , A. Kubankin , P. Kunze , M. Kuss , M. Kuźniak , M. Kuzwa , M. La Commara , M. Lai , E. LeGuirriec , E. Leason , A. Leoni , L. Lidey , M. Lissia , L. Luzzi , O. Lychagina , O. Macfadyen , I. N. Machulin , S. Manecki , I. Manthos , A. Marasciulli , G. Margutti , S. M. Mari , C. Mariani , J. Maricic , M. Martinez , C. J. Martoff , G. Matteucci , K. Mavrokoridis , E. Mazza , A. B. McDonald , S. Merzi , A. Messina , R. Milincic , S. Minutoli , A. Mitra , J. Monroe , E. Moretti , M. Morrocchi , T. Mroz , V. N. Muratova , M. Murphy , M. Murra , C. Muscas , P. Musico , R. Nania , M. Nessi , G. Nieradka , K. Nikolopoulos , E. Nikoloudaki , J. Nowak , K. Olchanski , A. Oleinik , V. Oleynikov , P. Organtini , A. Ortiz de Solrzano , M. Pallavicini , L. Pandola , E. Pantic , E. Paoloni , D. Papi , G. Pastuszak , G. Paternoster , P. A. Pegoraro , K. Pelczar , R. Perez , V. Pesudo , S. Piacentini , N. Pino , G. Plante , A. Pocar , M. Poehlmann , S. Pordes , P. Pralavorio , E. Preosti , D. Price , S. Puglia , M. Queiroga Bazetto , F. Ragusa , Y. Ramachers , A. Ramirez , S. Ravinthiran , M. Razeti , A. L. Renshaw , M. Rescigno , S. Resconi , F. Retiere , L. P. Rignanese , A. Rivetti , A. Roberts , C. Roberts , G. Rogers , L. Romero , M. Rossi , A. Rubbia , D. Rudik , M. Sabia , P. Salomone , O. Samoylov , S. Sanfilippo , D. Santone , R. Santorelli , E. Moura Santos , C. Savarese , E. Scapparone , F. G. Schuckman , G. Scioli , D. A. Semenov , A. Sheshukov , M. Simeone , P. Skensved , M. D. Skorokhvatov , O. Smirnov , T. Smirnova , B. Smith , A. Sotnikov , F. Spadoni , M. Spangenberg , R. Stefanizzi , A. Steri , V. Stornelli , S. Stracka , S. Sulis , 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 , E. V. Unzhakov , M. Van Uffelen , T. Viant , S. Viel , A. Vishneva , R. B. Vogelaar , J. Vossebeld , B. Vyas , M. Wada , M. Walczak , Y. Wang , H. Wang , S. Westerdale , L. Williams , R. Wojaczyski , M. M. Wojcik , M. Wojcik , T. Wright , Y. Xie , C. Yang , J. Yin , A. Zabihi , P. Zakhary , A. Zani , Y. Zhang , T. Zhu , A. Zichichi , G. Zuzel , M. P. Zykova

XMASS-I uses single phase liquid xenon technology for aiming at the direct detection of dark matter. The detector observes only scintillation light by 2 inch 642 PMTs which are placed in sphere shape around an active volume. With its large…

Cosmology and Nongalactic Astrophysics · Physics 2018-05-28 Masaki Yamashita
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