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The XENON1T experiment searches for dark matter particles through their scattering off xenon atoms in a 2 tonne liquid xenon target. The detector is a dual-phase time projection chamber, which measures simultaneously the scintillation and…

Instrumentation and Detectors · Physics 2019-07-03 E. Aprile , J. Aalbers , F. Agostini , M. Alfonsi , L. Althueser , F. D. Amaro , V. C. Antochi , F. Arneodo , L. Baudis , B. Bauermeister , M. L. Benabderrahmane , T. Berger , P. A. Breur , 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 , L. Grandi , Z. Greene , C. Hasterok , E. Hogenbirk , J. Howlett , M. Iacovacci , R. Itay , F. Joerg , S. Kazama , A. Kish , G. Koltman , A. Kopec , H. Landsman , R. F. Lang , L. Levinson , Q. Lin , S. Lindemann , M. Lindner , F. Lombardi , J. A. M. Lopes , E. López Fune , C. Macolino , J. Mahlstedt , A. Manfredini , F. Marignetti , T. Marrodán Undagoitia , J. Masbou , D. Masson , S. Mastroianni , M. Messina , K. Micheneau , K. Miller , A. Molinario , K. Morå , Y. Mosbacher , M. Murra , J. Naganoma , K. Ni , U. Oberlack , K. Odgers , B. Pelssers , F. Piastra , J. Pienaar , V. Pizzella , G. Plante , R. Podviianiuk , H. Qiu , D. Ramírez García , S. Reichard , B. Riedel , A. Rizzo , A. Rocchetti , N. Rupp , J. M. F. dos Santos , G. Sartorelli , N. Šarčević , M. Scheibelhut , S. Schindler , J. Schreiner , D. Schulte , M. Schumann , L. Scotto Lavina , M. Selvi , P. Shagin , E. Shockley , M. Silva , H. Simgen , C. Therreau , D. Thers , F. Toschi , G. Trinchero , C. Tunnell , N. Upole , M. Vargas , O. Wack , H. Wang , Z. Wang , Y. Wei , C. Weinheimer , D. Wenz , C. Wittweg , J. Wulf , J. Ye , Y. Zhang , T. Zhu , J. P. Zopounidis

We propose new concepts for experiments in which intense high energy photon or muon beams are employed parasitically to detect scattering by cosmic heavy weakly interacting dark matter (DM) particles. We show that the scattering…

High Energy Physics - Phenomenology · Physics 2026-03-04 A. Acar , M. Bashkanov , D. P. Watts

The Large Underground Xenon experiment (LUX) searches for dark matter using a dual-phase xenon detector. LUX uses a custom-developed trigger system for event selection. In this paper, the trigger efficiency, which is defined as the…

Searching for dark matter (DM) at colliders is one of the biggest challenges in high-energy physics today. Significant efforts have been made to detect DM within the mass range of 1-10,000 GeV at the Large Hadron Collider and other…

High Energy Physics - Experiment · Physics 2025-11-17 Tamas Almos Vami

This article reviews the progress made over the last 20 years in the development and applications of liquid xenon detectors in particle physics, astrophysics and medical imaging experiments. We begin with a summary of the fundamental…

Instrumentation and Detectors · Physics 2010-12-01 E. Aprile , T. Doke

The status and plans of a research program on the development of ultra-low-energy germanium detectors with sub-keV sensitivities are reported. We survey the scientific goals which include the observation of neutrino-nucleus coherent…

High Energy Physics - Experiment · Physics 2008-11-26 Henry T. Wong

The dual-phase liquid argon time projection chamber is presently one of the leading technologies to search for dark matter particles with masses below 10 GeV/c$^2$. This was demonstrated by the DarkSide-50 experiment with approximately 50…

High Energy Physics - Experiment · Physics 2025-01-07 20k Collaboration , F. Acerbi , P. Adhikari , P. Agnes , I. Ahmad , S. Albergo , I. F. M. Albuquerque , T. Alexander , A. K. Alton , P. Amaudruz , M. Angiolilli , E. Aprile , R. Ardito , 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 , 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. Cárdenas-Montes , N. Cargioli , M. Carlini , A. Castellani , P. Castello , P. Cavalcante , S. Cebrian , J. M. Cela Ruiz , S. Chashin , A. Chepurnov , L. Cifarelli , D. Cintas , M. Citterio , B. Cleveland , Y. Coadou , V. Cocco , D. Colaiuda , E. Conde Vilda , L. Consiglio , B. S. Costa , M. Czubak , M. D'Aniello , S. D'Auria , M. D. Da Rocha Rolo , G. Darbo , S. Davini , S. De Cecco , G. De Guido , G. Dellacasa , A. V. Derbin , A. Devoto , F. Di Capua , A. Di Ludovico , L. Di Noto , P. Di Stefano , L. K. Dias , D. Díaz Mairena , X. Ding , C. Dionisi , G. Dolganov , F. Dordei , V. Dronik , A. Elersich , E. Ellingwood , T. Erjavec , M. Fernandez Diaz , A. Ficorella , G. Fiorillo , P. Franchini , D. Franco , H. Frandini Gatti , E. Frolov , F. Gabriele , D. Gahan , C. Galbiati , G. Galiński , G. Gallina , G. Gallus , M. Garbini , P. Garcia Abia , A. Gawdzik , A. Gendotti , A. Ghisi , G. K. Giovanetti , V. Goicoechea Casanueva , A. Gola , L. Grandi , G. Grauso , G. Grilli di Cortona , A. Grobov , M. Gromov , M. Guerzoni , M. Gulino , C. Guo , B. R. Hackett , A. Hallin , A. Hamer , M. Haranczyk , B. Harrop , T. Hessel , S. Hill , S. Horikawa , J. Hu , F. Hubaut , J. Hucker , T. Hugues , E. V. Hungerford , A. Ianni , V. Ippolito , A. Jamil , C. Jillings , S. Jois , P. Kachru , R. Keloth , N. Kemmerich , A. Kemp , C. L. Kendziora , M. Kimura , 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 , M. Lissia , L. Luzzi , O. Lychagina , O. Macfadyen , 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 , J. Mclaughlin , S. Merzi , A. Messina , R. Milincic , S. Minutoli , A. Mitra , S. Moioli , 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 Solórzano , M. Pallavicini , L. Pandola , E. Pantic , E. Paoloni , D. Papi , G. Pastuszak , G. Paternoster , A. Peck , P. A. Pegoraro , K. Pelczar , L. A. Pellegrini , R. Perez , F. Perotti , V. Pesudo , S. Piacentini , N. Pino , G. Plante , A. Pocar , M. Poehlmann , S. Pordes , P. Pralavorio , D. Price , S. Puglia , M. Queiroga Bazetto , F. Ragusa , Y. Ramachers , A. Ramirez , S. Ravinthiran , M. Razeti , A. L. Renshaw , M. Rescigno , 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 , E. Sandford , S. Sanfilippo , D. Santone , R. Santorelli , E. M. Santos , C. Savarese , E. Scapparone , G. Schillaci , F. G. Schuckman , G. Scioli , D. A. Semenov , V. Shalamova , 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 , S. Tedesco , G. Testera , K. Thieme , A. Thompson , A. Tonazzo , S. Torres-Lara , A. Tricomi , E. V. Unzhakov , T. J. Vallivilayil , M. Van Uffelen , L. Velazquez-Fernandez , T. Viant , S. Viel , A. Vishneva , R. B. Vogelaar , J. Vossebeld , B. Vyas , M. B. Walczak , Y. Wang , H. Wang , S. Westerdale , L. Williams , R. Wojaczyński , M. Wojcik , M. 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

PandaX is a large upgradable liquid-xenon detector system that can be used for both direct dark-matter detection and $^{136}$Xe double-beta decay search. It is located in the Jinping Deep-Underground Laboratory in Sichuan, China. The…

The Edelweiss programme is dedicated to the direct search for Dark Matter as massive weakly interacting particles (WIMPs) with Germanium cryogenic detectors operated in the Laboratoire Souterrain de Modane in the French Alps at a depth of…

Astrophysics · Physics 2007-11-01 A. Chantelauze

Weakly interacting massive particles (WIMPs) are among the favored candidates for cold dark matter in the universe. The phenomenology of supersymmetric WIMPs has been quite developed during recent years. However, there are other…

High Energy Physics - Phenomenology · Physics 2009-11-07 E. A. Baltz , L. Bergstrom

The next generation of large scale WIMP direct detection experiments have the potential to go beyond the discovery phase and reveal detailed information about both the particle physics and astrophysics of dark matter. We report here on…

Cosmology and Nongalactic Astrophysics · Physics 2014-02-05 Jayden L. Newstead , Thomas D. Jacques , Lawrence M. Krauss , James B. Dent , Francesc Ferrer

Bosonic superweakly interacting massive particles (super-WIMPs) are a candidate for warm dark matter. With the absorption of such a boson by a xenon atom these dark matter candidates would deposit an energy equivalent to their rest mass in…

The China Dark Matter Experiment (CDEX) aims at direct searches of light Weakly Interacting Massive Particles (WIMPs) at the China Jinping Underground Laboratory (CJPL) with an overburden of about 2400m rock. Results from a prototype CDEX-1…

High Energy Physics - Experiment · Physics 2020-02-04 Hao Ma , Yang Chen , Qian Yue , Li Wang , Tao Xue , Zhi Zeng , Kejun Kang , Jianping Cheng , Yuanjing Li , Jianmin Li , Yulan Li for CDEX Collaboration

We present the most recent results from XENON100, the current phase of the XENON dark matter search program. XENON100 is a dual phase time-projection chamber operated at the Laboratori Nazionali del Gran Sasso (LNGS) whose ultra-low…

Cosmology and Nongalactic Astrophysics · Physics 2013-05-14 Paolo Beltrame

We report results from searches of pseudoscalar and vector bosonic super-weakly interacting massive particles (super-WIMP) in the TEXONO experiment at the Kuo-Sheng Nuclear Power Station, using 314.15 kg days of data from $n$-type…

High Energy Physics - Experiment · Physics 2019-02-27 Manoj Kumar Singh , Lakhwinder Singh , Mehmet Agartioglu , Vivek Sharma , Venktesh Singh , Henry Tsz-king Wong

Weakly Interacting Massive Particles (WIMPs) are a leading candidate for dark matter and are expected to produce nuclear recoil (NR) events within liquid xenon time-projection chambers. We present a measurement of the scintillation timing…

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

We study the prospects for long-lived charged particle (LLCP) searches at current and future LHC runs and at a 100 TeV pp collider, using Drell-Yan slepton pair production as an example. Because momentum measurements become more challenging…

High Energy Physics - Phenomenology · Physics 2016-02-16 Jonathan L. Feng , Sho Iwamoto , Yael Shadmi , Shlomit Tarem

This paper presents a novel technique for mitigating electrode backgrounds that limit the sensitivity of searches for low-mass dark matter (DM) using xenon time projection chambers. In the LUX detector, signatures of low-mass DM…

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