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One IGEX 76Ge double-beta decay detector is currently operating in the Canfranc Underground Laboratory in a search for dark matter WIMPs, through the Ge nuclear recoil produced by the WIMP elastic scattering. In this talk we report on the…

Liquid Argon Time Projection Chambers are planned to comprise a central role in the future of the U.S. High Energy Physics neutrino program. In particular, this detector technology will form the basis for the 40 kton Deep Underground…

Instrumentation and Detectors · Physics 2020-09-22 Eric Church , Christopher Jackson , Richard Saldanha

We investigate the power of low-energy, high-luminosity electron--positron colliders to probe hidden sectors with a mass below ~10 GeV that couple to Standard Model particles through a light mediator. Such sectors provide well-motivated…

High Energy Physics - Phenomenology · Physics 2015-02-24 Rouven Essig , Jeremy Mardon , Michele Papucci , Tomer Volansky , Yi-Ming Zhong

Precision measurements of solar neutrinos emitted by specific nuclear reaction chains in the Sun are of great interest for developing an improved understanding of star formation and evolution. Given the expected neutrino fluxes and known…

ANAIS is a direct dark matter detection experiment aiming at the confirmation or refutation of the DAMA/LIBRA positive annual modulation signal in the low energy detection rate, using the same target and technique. ANAIS-112, located at the…

Instrumentation and Methods for Astrophysics · Physics 2022-03-02 I. Coarasa , J. Apilluelo , J. Amaré , S. Cebrián , D. Cintas , E. García , M. Martínez , M. A. Oliván , Y. Ortigoza , A. Ortiz de Solórzano , J. Puimedón , A. Salinas , M. L. Sarsa , P. Villar

COSINE-100 is a dark matter direct detection experiment with 106 kg NaI(Tl) as the target material. 210Pb and daughter isotopes are a dominant background in the WIMP region of interest and are detected via beta decay and alpha decay.…

We report on the search for weakly interacting massive particle (WIMP) dark matter candidates in the galactic halo that interact with sodium and iodine nuclei in the COSINE-100 experiment and produce energetic electrons that accompany…

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

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

Dark Matter (DM) comprising particles in the mass range of a few MeV to GeV is waiting to be explored, given the many theoretical models accommodating cosmological abundance. We hereby propose an experiment with the LHC proton beam of 7 TeV…

High Energy Physics - Experiment · Physics 2016-09-04 Ashok Kumar , Archana Sharma

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 with a charge imaging…

We have developed ultra-low-background NaI(Tl) crystals to reproduce the DAMA results with the ultimate goal of achieving purity levels that are comparable to or better than those of the DAMA/LIBRA crystals. Even though the achieved…

Instrumentation and Methods for Astrophysics · Physics 2017-08-02 G. Adhikari , P. Adhikari , C. Ha , E. J. Jeon , N. Y. Kim , Y. D. Kim , S. Y. Kong , H. S. Lee , S. Y. Oh , J. S. Park , K. S. Park

Many experiments that aim at the direct detection of Dark Matter are able to distinguish a dominant background from the expected feeble signals, based on some measured discrimination parameter. We develop a statistical model for such…

Dark sector models present a rich phenomenology that requires high-intensity beams and precision detectors for thorough exploration. The NA62 experiment has already published several constraints on dark sector models, leveraging proton beam…

High Energy Physics - Phenomenology · Physics 2026-03-26 F. Arias-Aragón , L. Darmé , R. Gargiulo , G. Grilli di Cortona , V. Kozhuharov , E. Nardi , M. Raggi , T. Spadaro , P. Valente

Building on the successful experience in operating the DarkSide-50 detector, the DarkSide Collaboration is going to construct DarkSide-20k, a direct WIMP search detector using a two-phase Liquid Argon Time Projection Chamber (LArTPC) with…

Instrumentation and Detectors · Physics 2018-08-09 C. E. Aalseth , F. Acerbi , P. Agnes , I. F. M. Albuquerque , T. Alexander , A. Alici , A. K. Alton , P. Antonioli , S. Arcelli , R. Ardito , I. J. Arnquist , D. M. Asner , M. Ave , H. O. Back , A. I. Barrado Olmedo , G. Batignani , E. Bertoldo , S. Bettarini , M. G. Bisogni , V. Bocci , A. Bondar , G. Bonfini , W. Bonivento , M. Bossa , B. Bottino , M. Boulay , R. Bunker , S. Bussino , A. Buzulutskov , M. Cadeddu , M. Cadoni , A. Caminata , N. Canci , A. Candela , C. Cantini , M. Caravati , M. Cariello , M. Carlini , M. Carpinelli , A. Castellani , S. Catalanotti , V. Cataudella , P. Cavalcante , S. Cavuoti , R. Cereseto , A. Chepurnov , C. Cicalò , L. Cifarelli , M. Citterio , A. G. Cocco , M. Colocci , S. Corgiolu , G. Covone , P. Crivelli , I. D'Antone , M. D'Incecco , D. D'Urso , M. D. Da Rocha Rolo , M. Daniel , S. Davini , A. de Candia , S. De Cecco , M. De Deo , G. De Filippis , G. De Guido , G. De Rosa , G. Dellacasa , M. Della Valle , P. Demontis , A. Derbin , A. Devoto , F. Di Eusanio , G. Di Pietro , C. Dionisi , A. Dolgov , I. Dormia , S. Dussoni , A. Empl , M. Fernandez Diaz , A. Ferri , C. Filip , G. Fiorillo , K. Fomenko , D. Franco , G. E. Froudakis , F. Gabriele , A. Gabrieli , C. Galbiati , P. Garcia Abia , A. Gendotti , A. Ghisi , S. Giagu , P. Giampa , G. Gibertoni , C. Giganti , M. A. Giorgi , G. K. Giovanetti , M. L. Gligan , A. Gola , O. Gorchakov , A. M. Goretti , F. Granato , M. Grassi , J. W. Grate , G. Y. Grigoriev , M. Gromov , M. Guan , M. B. B. Guerra , M. Guerzoni , M. Gulino , R. K. Haaland , A. Hallin , B. Harrop , E. W. Hoppe , S. Horikawa , B. Hosseini , D. Hughes , P. Humble , E. V. Hungerford , An. Ianni , C. Jillings , T. N. Johnson , K. Keeter , C. L. Kendziora , S. Kim , G. Koh , D. Korablev , G. Korga , A. Kubankin , M. Kuss , M. Kuźniak , B. Lehnert , X. Li , M. Lissia , G. U. Lodi , B. Loer , G. Longo , P. Loverre , R. Lussana , L. Luzzi , Y. Ma , A. A. Machado , I. N. Machulin , A. Mandarano , L. Mapelli , M. Marcante , A. Margotti , S. M. Mari , M. Mariani , J. Maricic , C. J. Martoff , M. Mascia , M. Mayer , A. B. McDonald , A. Messina , P. D. Meyers , R. Milincic , A. Moggi , S. Moioli , J. Monroe , A. Monte , M. Morrocchi , B. J. Mount , W. Mu , V. N. Muratova , S. Murphy , P. Musico , R. Nania , A. Navrer Agasson , I. Nikulin , V. Nosov , A. O. Nozdrina , N. N. Nurakhov , 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 , K. Pelczar , L. A. Pellegrini , N. Pelliccia , F. Perotti , R. Perruzza , V. Pesudo Fortes , C. Piemonte , F. Pilo , A. Pocar , T. Pollmann , D. Portaluppi , D. A. Pugachev , H. Qian , B. Radics , F. Raffaelli , F. Ragusa , M. Razeti , A. Razeto , V. Regazzoni , C. Regenfus , B. Reinhold , A. L. Renshaw , M. Rescigno , F. Retière , Q. Riffard , A. Rivetti , S. Rizzardini , A. Romani , L. Romero , B. Rossi , N. Rossi , A. Rubbia , D. Sablone , P. Salatino , O. Samoylov , E. Sánchez García , W. Sands , M. Sant , R. Santorelli , C. Savarese , E. Scapparone , B. Schlitzer , G. Scioli , E. Segreto , A. Seifert , D. A. Semenov , A. Shchagin , L. Shekhtman , E. Shemyakina , A. Sheshukov , M. Simeone , P. N. Singh , P. Skensved , M. D. Skorokhvatov , O. Smirnov , G. Sobrero , A. Sokolov , A. Sotnikov , F. Speziale , R. Stainforth , C. Stanford , G. B. Suffritti , Y. Suvorov , R. Tartaglia , G. Testera , A. Tonazzo , A. Tosi , P. Trinchese , E. V. Unzhakov , A. Vacca , E. Vázquez-Jáuregui , M. Verducci , T. Viant , F. Villa , A. Vishneva , B. Vogelaar , M. Wada , J. Wahl , J. Walding , S. Walker , H. Wang , Y. Wang , A. W. Watson , S. Westerdale , R. Williams , M. M. Wojcik , S. Wu , X. Xiang , X. Xiao , C. Yang , Z. Ye , A. Yllera de Llano , F. Zappa , G. Zappalà , C. Zhu , A. Zichichi , M. Zullo , A. Zullo

The WARP programme is a graded programme intended to search for cold Dark Matter in the form of WIMP's. These particles may produce via weak interactions nuclear recoils in the energy range 10-100 keV. A cryogenic noble liquid like argon,…

We investigate the prospects for measuring the coherent elastic neutrino-nucleus scattering of solar and supernova neutrinos in future NaI(Tl) dark matter detection experiments. Considering the reduced background and improved light yield of…

High Energy Physics - Phenomenology · Physics 2023-08-29 Young Ju Ko , Hyun Su Lee

The MiniBooNE-DM collaboration searched for vector-boson mediated production of dark matter using the Fermilab 8 GeV Booster proton beam in a dedicated run with $1.86 \times 10^{20}$ protons delivered to a steel beam dump. The MiniBooNE…

The Cryogenic Dark Matter Search (CDMS) and XENON experiments aim to directly detect dark matter in the form of weakly interacting massive particles (WIMPs) via their elastic scattering on the target nuclei. The experiments use different…

Astrophysics · Physics 2008-11-26 Kaixuan Ni , Laura Baudis

The design, optimisation and construction of an anti-coincidence veto detector to complement the ZEPLIN-III direct dark matter search instrument is described. One tonne of plastic scintillator is arranged into 52 bars individually read out…