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The three-dimensional (3-D) reconstruction of nuclear recoils is of interest for directional detection of fast neutrons and for direction-sensitive searches for weakly interacting massive particles(WIMPs), which may constitute the Dark…

Instrumentation and Detectors · Physics 2015-12-09 S. E. Vahsen , M. T. Hedges , I. Jaegle , S. J. Ross , I. S. Seong , T. N. Thorpe , J. Yamaoka , J. A. Kadyk , M. Garcia-Sciveres

There is currently vast evidence for Dark Matter (DM) from astronomical observations. However, in spite of tremendous efforts by large experimental groups, there is no confirmed direct detection of the dark matter in our galaxy. Recent…

Instrumentation and Methods for Astrophysics · Physics 2014-11-20 Juan Estrada

MIMAC (MIcro-TPC MAtrix of Chambers) is a directional WIMP Dark Matter detector project. Direct dark matter experiments need a high level of electron/recoil discrimination to search for nuclear recoils produced by WIMP-nucleus elastic…

Instrumentation and Methods for Astrophysics · Physics 2016-09-21 Q. Riffard , D. Santos , O. Guillaudin , G. Bosson , O. Bourrion , J. Bouvier , T. Descombes , J. -F. Muraz , L. Lebreton , D. Maire , P. Colas , I. Giomataris , J. Busto , D. Fouchez , J. Brunner , C. Tao

Direction measurement of weakly interacting massive particles in time-projection chambers can provide definite evidence of their existence and help to determine their properties. This article demonstrates several concepts for charge…

Over the past decades, several ideas and technologies have been developed to directly detect WIMP from the galactic halo. All these detection strategies share the common goal of discriminating a WIMP signal from the residual backgrounds. By…

Instrumentation and Detectors · Physics 2015-06-23 J. Billard

The direct search for dark matter in the form of weakly interacting massive particles (WIMP) is performed by detecting nuclear recoils (NR) produced in a target material from the WIMP elastic scattering. A promising experimental strategy…

Instrumentation and Detectors · Physics 2024-01-12 20k Collaboration , P. Agnes , I. Ahmad , S. Albergo , I. F. M. Albuquerque , T. Alexander , A. K. Alton , P. Amaudruz , M. Atzori Corona , M. Ave , I. Ch. Avetisov , O. Azzolini , H. O. Back , Z. Balmforth , A. Barrado-Olmedo , P. Barrillon , A. Basco , G. Batignani , V. Bocci , W. M. Bonivento , B. Bottino , M. G. Boulay , J. Busto , M. Cadeddu , A. Caminata , N. Canci , G. Cappello , A. Capra , S. Caprioli , M. Caravati , N. Cargioli , M. Carlini , P. Castello , V. Cataudella , P. Cavalcante , S. Cavuoti , S. Cebrian , J. M. Cela Ruiz , S. Chashin , A. Chepurnov , E. Chyhyrynets , L. Cifarelli , D. Cintas , M. Citterio , B. Cleveland , V. Cocco , E. Conde Vilda , L. Consiglio , S. Copello , G. Covone , M. Czubak , M. D'Aniello , S. D'Auria , M. D. Da Rocha Rolo , S. Davini , A. de Candia , S. De Cecco , D. De Gruttola , G. De Filippis , D. Dell'Aquila , S. De Pasquale , G. De Rosa , G. Dellacasa , A. V. Derbin , A. Devoto , F. Di Capua , L. Di Noto , C. Dionisi , P. Di Stefano , G. Dolganov , F. Dordei , A. Elersich , E. Ellingwood , T. Erjavec , M. Fernandez Diaz , G. Fiorillo , P. Franchini , D. Franco , N. Funicello , F. Gabriele , D. Gahan , C. Galbiati , G. Gallina , G. Gallus , M. Garbini , P. Garcia Abia , A. Gendotti , C. Ghiano , C. Giganti , G. K. Giovanetti , V. Goicoechea Casanueva , A. Gola , G. Grauso , G. Grilli di Cortona , A. Grobov , M. Gromov , M. Guan , M. Guerzoni , M. Gulino , C. Guo , B. R. Hackett , A. L. Hallin , A. Hamer , M. Haranczyk , T. Hessel , S. Hill , S. Horikawa , F. Hubaut , J. Hucker , T. Hugues , An. Ianni , V. Ippolito , C. Jillings , S. Jois , P. Kachru , N. Kemmerich , A. A. Kemp , C. L. Kendziora , M. Kimura , I. Kochanek , K. Kondo , G. Korga , S. Koulosousas , A. Kubankin , M. Kuss , M. Kuzniak , M. La Commara , M. Lai , E. Le Guirriec , E. Leason , A. Leoni , X. Li , L. Lidey , M. Lissia , L. Luzzi , O. Lychagina , O. Macfadyen , I. N. Machulin , S. Manecki , I. Manthos , L. Mapelli , A. Margotti , S. M. Marik , C. Mariani , J. Maricic , A. Marini , M. Martínez , C. J. Martoff , G. Matteucci , K. Mavrokoridis , A. B. McDonald , A. Messina , R. Milincic , A. Mitra , A. Moharana , J. Monroe , E. Moretti , M. Morrocchi , T. Mróz , V. N. Muratova , C. Muscas , P. Musico , R. Nania , M. Nessi , G. Nieradka , K. Nikolopoulos , 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 , V. Pesudo , S. Piacentini , N. Pino , A. Pocar , D. M. Poehlmann , S. Pordes , P. Pralavorio , D. Price , F. Ragusa , Y. Ramachers , M. Razeti , A. L. Renshaw , M. Rescigno , F. Retiere , L. P. Rignanese , C. Ripoli , A. Rivetti , A. Roberts , C. Roberts , J. Rode , G. Rogers , L. Romero , M. Rossi , A. Rubbia , M. A. Sabia , P. Salomone , E. Sandford , S. Sanfilippo , D. Santone , R. Santorelli , C. Savarese , E. Scapparone , G. Schillaci , F. G. Schuckman , G. Scioli , M. Simeone , P. Skensved , M. D. Skorokhvatov , O. Smirnov , T. Smirnova , B. Smith , A. Sosa , F. Spadoni , M. Spangenberg , R. Stefanizzi , A. Steri , V. Stornelli , S. Stracka , M. Stringer , S. Sulis , A. Sung , Y. Suvorov , A. M. Szelc , R. Tartaglia , A. Taylor , J. Taylor , S. Tedesco , G. Testera , K. Thieme , T. N. Thorpe , A. Tonazzo , A. Tricomi , E. V. Unzhakov , T. Vallivilayil John , M. Van Uffelen , T. Viant , S. Viel , R. B. Vogelaar , J. Vossebeld , M. Wada , M. B. Walczak , H. Wang , Y. Wang , S. Westerdale , L. Williams , I. Wingerter-Seez , R. Wojaczynski , Ma. M. Wojcik , T. Wright , Y. Xie , C. Yang , A. Zabihi , P. Zakhary , A. Zani , A. Zichichi , G. Zuzel , M. P. Zykova

Directional detection is a promising Dark Matter search strategy. Even though it could accommodate to a sizeable background contamination, electron/recoil discrimination remains a key and challenging issue as for direction-insensitive…

Instrumentation and Methods for Astrophysics · Physics 2015-06-05 J. Billard , F. Mayet , D. Santos

The Dark Matter Time Projection Chamber collaboration recently reported a dark matter limit obtained with a 10 liter time projection chamber filled with CF4 gas. The 10 liter detector was capable of 2D tracking (perpendicular to the drift…

Instrumentation and Methods for Astrophysics · Physics 2015-05-30 J. B. R. Battat , S. Ahlen , M. Chernicoff , C. Deaconu , D. Dujmic , A. Dushkin , P. Fisher , S. Henderson , A. Inglis , A. Kaboth , L. Kirsch , J. P. Lopez , J. Monroe , H. Ouyang , G. Sciolla , H. Tomita , H. Wellenstein

The Cryogenic Dark Matter Search (CDMS) employs low-temperature Ge and Si detectors to search for Weakly Interacting Massive Particles (WIMPs) via their elastic-scattering interactions with nuclei while discriminating against interactions…

Astrophysics · Physics 2012-08-27 CDMS Collaboration

In this paper, we present a Time Projection Chamber (TPC) system for low-background beta radiation measurements. The system consists of a TPC with two-dimensional-strip readout Micromegas and an anti-coincidence detector with readout pads…

Instrumentation and Detectors · Physics 2026-01-01 Ruiyang Zhang , Zhiyong Zhang , Zengxuan Huang , Yong Zhou , Jianbei Liu , Songsong Tang , Yuanfei Cheng , Changqing Feng , Ming Shao , Yi Zhou

There is a worldwide effort toward the development of a large TPC (Time Projection Chamber) devoted to directional Dark Matter detection. All current projects are being designed to fulfill a unique goal : identifying weakly interacting…

Cosmology and Nongalactic Astrophysics · Physics 2012-04-12 J. Billard , F. Mayet , D. Santos

The possibility of using CCD detectors in a low threshold direct detection dark matter search experiment is discussed. We present the main features of the DECam detectors that make them a good alternative for such an experiment, namely…

High Energy Physics - Experiment · Physics 2008-07-01 J. Estrada , H. Cease , H. T. Diehl , B. Flaugher , J. Jones , D. Kubik , A. Sonnenschein

Directional detection of nuclear recoils is broadly desirable in nuclear and particle physics. At low recoil energies, this capability may be used to confirm the cosmological origin of a dark matter signal, to penetrate the so-called…

Instrumentation and Detectors · Physics 2021-10-13 Majd Ghrear , Sven E. Vahsen , Cosmin Deaconu

Gas-filled Time Projection Chambers (TPCs) with Gas Electron Multipliers (GEMs) and pixels appear suitable for direction-sensitive WIMP dark matter searches. We present the background and motivation for our work on this technology, past and…

Instrumentation and Methods for Astrophysics · Physics 2015-05-30 S. E. Vahsen , H. Feng , M. Garcia-Sciveres , I. Jaegle , J. Kadyk , Y. Nguyen , M. Rosen , S. Ross , T. Thorpe , J. Yamaoka

Low-pressure gaseous TPCs are well suited detectors to correlate the directions of nuclear recoils to the galactic Dark Matter (DM) halo. Indeed, in addition to providing a measure of the energy deposition due to the elastic scattering of a…

Instrumentation and Methods for Astrophysics · Physics 2017-12-06 C. Couturier , Q. Riffard , N. Sauzet , O. Guillaudin , F. Naraghi , D. Santos

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

We study the dependence of the exposure required to directly detect a WIMP directional recoil signal on the capabilities of a directional detector. Specifically we consider variations in the nuclear recoil energy threshold, the background…

Astrophysics · Physics 2008-11-26 Anne M. Green , Ben Morgan

Directional detection of non-baryonic DarkMatter is a promising search strategy for discriminating WIMP events from background ones. This strategy requires both a measurement of the recoil energy down to a few keV and 3D reconstruction of…

Instrumentation and Methods for Astrophysics · Physics 2011-11-08 D. Santos , J. Billard , G. Bosson , J. L. Bouly , O. Bourrion , Ch. Fourel , O. Guillaudin , F. Mayet , J. P. Richer , A. Delbart , E. Ferrer , I. Giomataris , F. J. Iguaz , J. P. Mols , C. Golabek , L. Lebreton

If Dark Matter is made of Weakly Interacting Massive Particles (WIMPs) with masses below $\sim$20 GeV, the corresponding nuclear recoils in mainstream WIMP experiments are of energies too close, or below, the experimental threshold. Gas…

Instrumentation and Detectors · Physics 2016-10-21 F. J. Iguaz , J. G. Garza , F. Aznar , J. F. Castel , S. Cebrián , T. Dafni , J. A. García , I. G. Irastorza , A. Lagraba , G. Luzón , A. Peiró