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Related papers: The Oscura Experiment

200 papers

We report on recent progress in the search for dark matter particles with masses from 1 MeV to 1 GeV. Several dark matter candidates in this mass range are expected to generate measurable electronic-recoil signals in direct-detection…

Cosmology and Nongalactic Astrophysics · Physics 2023-01-02 Alvaro E. Chavarria

This work briefly discusses the potential applications of the Skipper-CCD technology in astronomy and reviews its current use in dark matter and neutrino experiments. An overview of the ongoing efforts to build multi-kilogram experiments…

Instrumentation and Methods for Astrophysics · Physics 2022-11-23 B. A. Cervantes-Vergara , S. Perez , J. C. D'Olivo , J. Estrada , D. J. Grimm , S. Holland , M. Sofo-Haro , W. Wong

Oscura is a planned light-dark matter search experiment using Skipper-CCDs with a total active mass of 10 kg. As part of the detector development, the collaboration plans to build the Oscura Integration Test (OIT), an engineering test with…

The DAMIC (Dark Matter in CCDs) experiment searches for the interactions of dark matter particles with the nuclei and the electrons in the silicon bulk of thick fully depleted charge-coupled devices (CCDs). Because of the low noise and low…

High Energy Physics - Experiment · Physics 2020-04-02 Mariangela Settimo

Direct detection experiments have established the most stringent constraints on potential interactions between particle candidates for relic, thermal dark matter and Standard Model particles. To surpass current exclusion limits a new…

The Sub-Electron-Noise Skipper CCD Experimental Instrument (SENSEI) uses the recently developed Skipper-CCD technology to search for electron recoils from the interaction of sub-GeV dark matter particles with electrons in silicon. We report…

A direct dark matter search is performed using fully-depleted high-resistivity CCD detectors . Due to their low electronic readout noise (RMS ~ 7 eV) these devices operate with a very low detection threshold of 40 eV, making the search for…

Instrumentation and Methods for Astrophysics · Physics 2015-05-28 J. Barreto , H. Cease , H. T. Diehl , J. Estrada , B. Flaugher , N. Harrison , J. Jones , B. Kilminster , J. Molina , J. Smith , T. Schwarz , A. Sonnenschein

The DAMIC (Dark Matter in CCDs) experiment uses high resistivity, scientific grade CCDs to search for dark matter. The CCD's low electronic noise allows an unprecedently low energy threshold of a few tens of eV that make it possible to…

The DAMIC experiment employs large-area, thick charge-coupled devices (CCDs) to search for the interactions of low-mass dark matter particles in the galactic halo with silicon atoms in the CCD target. From 2017 to 2019, DAMIC collected data…

Cosmology and Nongalactic Astrophysics · Physics 2022-10-04 Alvaro E. Chavarria

The purpose of this project is to investigate the use of charge couple devices (CCDs) to detect electrons directly. This can be done in transmission electron microscopy (TEM) for electrons over 100 KeV, but for space plasma instruments,…

Instrumentation and Detectors · Physics 2015-10-28 S. R. Mirfayzi

Dark matter with mass below about a GeV is essentially unobservable in conventional direct detection experiments. However, newly proposed technology will allow the detection of single electron events in semiconductor materials with…

High Energy Physics - Phenomenology · Physics 2012-11-13 Peter W. Graham , David E. Kaplan , Surjeet Rajendran , Matthew T. Walters

Dark matter lighter than 10 GeV/c$^2$ encompasses a promising range of candidates. A conceptual design for a new detector, DarkSide-LowMass, is presented, based on the DarkSide-50 detector and progress toward DarkSide-20k, optimized for a…

Instrumentation and Detectors · Physics 2023-06-21 P. Agnes , I. Ahmad , S. Albergo , I. F. M. Albuquerque , T. Alexander , A. K. Alton , P. Amaudruz , M. Atzori Corona , D. J. Auty , M. Ave , I. Ch. Avetisov , R. I. Avetisov , O. Azzolini , H. O. Back , Z. Balmforth , V. Barbarian , A. Barrado Olmedo , P. Barrillon , A. Basco , G. Batignani , E. Berzin , A. Bondar , W. M. Bonivento , E. Borisova , B. Bottino , M. G. Boulay , G. Buccino , S. Bussino , J. Busto , A. Buzulutskov , M. Cadeddu , M. Cadoni , A. Caminata , N. Canci , A. Capra , S. Caprioli , M. Caravati , M. Cárdenas-Montes , N. Cargioli , M. Carlini , P. Castello , V. Cataudella , P. Cavalcante , S. Cavuoti , S. Cebrian , J. M. Cela Ruiz , S. Chashin , A. Chepurnov , E Chyhyrynets , C. Cicalò , L. Cifarelli , D. Cintas , V. Cocco , E. Conde Vilda , L. Consiglio , S. Copello , G. Covone , S. Cross , P. Czudak , M. D'Aniello , S. D'Auria , M. D. Da Rocha Rolo , O. Dadoun , M. Daniel , S. Davini , A. De Candia , S. De Cecco , A. De Falco , G. De Filippis , D. De Gruttola , S. De Pasquale , G. De Rosa , G. Dellacasa , A. V. Derbin , A. Devoto , F. Di Capua , L. Di Noto , P. Di Stefano , C. Dionisi , G. Dolganov , F. Dordei , L. Doria , T. Erjavec , M. Fernandez Diaz , G. Fiorillo , A. Franceschi , P. Franchini , D. Franco , E. Frolov , N. Funicello , F. Gabriele , D. Gahan , C. Galbiati , G. Gallina , G. Gallus , M. Garbini , P. Garcia Abia , A. Gendotti , C. Ghiano , R. A. Giampaolo , C. Giganti , M. A. Giorgi , G. K. Giovanetti , V. Goicoechea Casanueva , A. Gola , D. Gorman , R. Graciani Diaz , G. Grauso , G. Grilli di Cortona , A. Grobov , M. Gromov , M. Guan , M. Guerzoni , M. Gulino , C. Guo , B. R. Hackett , J. B. Hall , A. L. Hallin , A. Hamer , H. Helton , M. Haranczyk , T. Hessel , S. Hill , S. Horikawa , F. Hubaut , T. Hugues , E. V. Hungerford , An. Ianni , V. Ippolito , C. Jillings , P. Kachru , A. A. Kemp , C. L. Kendziora , G. Keppel , A. V. Khomyakov , M. Kimura , I. Kochanek , K. Kondo , G. Korga , S. Koulosousas , A. Kubankin , M. Kuss , M. Kuźniak , M. La Commara , M. Lai , E. Le Guirriec , E. Leason , X. Li , L. Lidey , J. Lipp , M. Lissia , G. Longo , L. Luzzi , O. Macfadyen , I. N. Machulin , I. Manthos , L. Mapelli , A. Margotti , S. M. Mari , C. Mariani , J. Maricic , A. Marini , M. Martínez , C. J. Martoff , A. Masoni , K. Mavrokoridis , A. Mazzi , A. B. McDonald , A. Messina , R. Milincic , A. Moggi , A. Moharana , J. Monroe , M. Morrocchi , E. N. Mozhevitina , T. Mróz , V. N. Muratova , C. Muscas , P. Musico , R. Nania , T. Napolitano , M. Nessi , G. Nieradka , K. Nikolopoulos , I. Nikulin , J. Nowak , K. Olchansky , A. Oleinik , V. Oleynikov , P. Organtini , A. Ortiz de Solórzano , L. Pagani , M. Pallavicini , L. Pandola , E. Pantic , E. Paoloni , G. Paternoster , P. A. Pegoraro , K. Pelczar , C. Pellegrino , F. Perotti , V. Pesudo , S. Piacentini , F. Pietropaolo , N. Pino , C. Pira , A. Pocar , D. M. Poehlmann , S. Pordes , P. Pralavorio , D. Price , F. Raffaelli , F. Ragusa , Y. Ramachers , A. Ramirez , M. Razeti , A. Razeto , A. L. Renshaw , M. Rescigno , F. Resnati , F. Retiere , L. P. Rignanese , C. Ripoli , A. Rivetti , A. Roberts , C. Roberts , J. Rode , G. Rogers , L. Romero , M. Rossi , A. Rubbia , S. Sadashivajois , T. R. Saffold , O. Samoylov , E. Sandford , S. Sanfilippo , D. Santone , R. Santorelli , C. Savarese , E. Scapparone , G. Scioli , D. A. Semenov , A. Shchagin , A. Sheshukov , M. Simeone , P. Skensved , M. D. Skorokhvatov , O. Smirnov , T. Smirnova , B. Smith , A. Sokolov , M. Spangenberg , R. Stefanizzi , A. Steri , S. Stracka , V. Strickland , M. Stringer , S. Sulis , A. Sung , Y. Suvorov , A. M. Szelc , C. Türkoğ , R. Tartaglia , A. Taylor , J. Taylor , S. Tedesco , G. Testera , K. Thieme , T. N. Thorpe , A. Tonazzo , S. Torres-Lara , A. Tricomi , E. V. Unzhakov , T. Vallivilayil John , M. Van Uffelen , T. Viant , S. Viel , A. Vishneva , R. B. Vogelaar , J. Vossebeld , M. Wada , M. B. Walczak , Y. Wang , S. Westerdale , R. J. Wheadon , L. Williams , I. Wingerter-Seez , R. Wojaczyński , Ma. M. Wojcik , Ma. Wojcik , T. Wright , Y. Xie , C. Yang , A. Zabihi , P. Zakhary , A. Zani , A. Zichichi , G. Zuzel , M. P. Zykova

The CRESST experiment is a direct dark matter search which aims to measure interactions of potential dark matter particles in an earth-bound detector. With the current stage, CRESST-III, we focus on a low energy threshold for increased…

DarkSHINE is an electron fixed target experiment under proposal that aims to probe light dark matter in the MeV-GeV mass range via the invisible decay of dark photons, leveraging the High repetition rate 8 GeV electron beam from the…

High Energy Physics - Experiment · Physics 2025-12-16 Haijun Yang

The DAMIC (Dark Matter in CCDs) experiment at the SNOLAB underground laboratory uses fully depleted, high resistivity CCDs to search for dark matter particles with masses below 10 GeV/c$^2$. An upgrade of the detector using an array of…

Instrumentation and Methods for Astrophysics · Physics 2018-07-01 Mariangela Settimo

This report presents an overview of the unconventional use of charge-coupled devices (CCDs) to search for Dark Matter (DM). The DArk Matter In CCDs (DAMIC Experiment) employs the bulk silicon of thick, fully-depleted CCDs as a target for…

Instrumentation and Detectors · Physics 2020-01-14 N. Castello-Mor , DAMIC-M Collaboration

We present constraints on low-mass dark matter electron scattering and absorption interactions using a SuperCDMS high-voltage eV-resolution (HVeV) detector. Data were taken underground in the NEXUS facility located at Fermilab with an…

High Energy Physics - Experiment · Physics 2026-03-17 SuperCDMS Collaboration , M. F. Albakry , I. Alkhatib , D. Alonso-González , J. Anczarski , T. Aralis , T. Aramaki , I. Ataee Langroudy , C. Bathurst , R. Bhattacharyya , A. J. Biffl , P. L. Brink , M. Buchanan , R. Bunker , B. Cabrera , R. Calkins , R. A. Cameron , C. Cartaro , D. G. Cerdeño , Y. -Y. Chang , M. Chaudhuri , J. -H. Chen , R. Chen , N. Chott , J. Cooley , H. Coombes , P. Cushman , R. Cyna , S. Das , S. Dharani , M. L. di Vacri , M. D. Diamond , M. Elwan , S. Fallows , E. Fascione , E. Figueroa-Feliciano , S. L. Franzen , A. Gevorgian , M. Ghaith , G. Godden , J. Golatkar , S. R. Golwala , R. Gualtieri , J. Hall , S. A. S. Harms , C. Hays , B. A. Hines , Z. Hong , L. Hsu , M. E. Huber , V. Iyer , V. K. S. Kashyap , S. T. D. Keller , M. H. Kelsey , K. T. Kennard , Z. Kromer , A. Kubik , N. A. Kurinsky , M. Lee , J. Leyva , B. Lichtenberg , J. Liu , Y. Liu , E. Lopez Asamar , P. Lukens , R. López Noé , D. B. MacFarlane , R. Mahapatra , J. S. Mammo , N. Mast , A. J. Mayer , P. C. McNamara , H. Meyer zu Theenhausen , É. Michaud , E. Michielin , K. Mickelson , N. Mirabolfathi , M. Mirzakhani , B. Mohanty , D. Mondal , D. Monteiro , J. Nelson , H. Neog , V. Novati , J. L. Orrell , M. D. Osborne , S. M. Oser , L. Pandey , S. Pandey , R. Partridge , P. K. Patel , D. S. Pedreros , W. Peng , W. L. Perry , R. Podviianiuk , M. Potts , S. S. Poudel , A. Pradeep , M. Pyle , W. Rau , R. Ren , T. Reynolds , M. Rios , A. Roberts , A. E. Robinson , L. Rosado Del Rio , J. L. Ryan , T. Saab , D. Sadek , B. Sadoulet , S. P. Sahoo , I. Saikia , S. Salehi , J. Sander , B. Sandoval , A. Sattari , B. Schmidt , R. W. Schnee , B. Serfass , A. E. Sharbaugh , R. S. Shenoy , A. Simchony , P. Sinervo , Z. J. Smith , R. Soni , K. Stifter , J. Street , M. Stukel , H. Sun , E. Tanner , N. Tenpas , D. Toback , A. N. Villano , J. Viol , B. von Krosigk , Y. Wang , O. Wen , Z. Williams , M. J. Wilson , J. Winchell , S. Yellin , B. A. Young , B. Zatschler , S. Zatschler , A. Zaytsev , E. Zhang , L. Zheng , A. Zuniga , M. J. Zurowski

The XENON experimental program aims to detect cold dark matter particles via their elastic collisions with xenon nuclei in two-phase time projection chambers (TPCs). We are currently testing a new TPC at the 100 kg scale, XENON100. This…

Instrumentation and Methods for Astrophysics · Physics 2019-08-14 Elena Aprile , Laura Baudis
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