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Velocity distribution of dark matter is assumed to be isotropic in most cases, however, anisotropy is suggested in some simulations. Directional direct detection of dark matter is a hopeful way to discriminate the anisotropy of dark matter…

Cosmology and Nongalactic Astrophysics · Physics 2020-07-10 Keiko I. Nagao

Directional detection is an important way to detect dark matter. An input to these experiments is the dark matter velocity distribution. Recent hydrodynamical simulations have shown that the dark matter velocity distribution differs…

Cosmology and Nongalactic Astrophysics · Physics 2018-02-12 Ranjan Laha

Dark Matter detectors with directional sensitivity have the potential of yielding an unambiguous positive observation of WIMPs as well as discriminating between galactic Dark Matter halo models. In this article, we introduce the motivation…

Instrumentation and Methods for Astrophysics · Physics 2014-11-20 Gabriella Sciolla , C. Jeff Martoff

Paleodetection has been proposed as a competitive method for detecting dark matter and other new physics interactions, complementing conventional direct detection experiments. In this work, we utilise TRIM simulations to improve the…

High Energy Physics - Phenomenology · Physics 2025-04-15 Audrey Fung , Thalles Lucas , Levente Balogh , Matthew Leybourne , Aaron C. Vincent

One of the most promising strategies to identify the nature of dark matter consists in the search for new particles at accelerators and with so-called direct detection experiments. Working within the framework of simplified models, and…

High Energy Physics - Phenomenology · Physics 2018-05-04 Gianfranco Bertone , Nassim Bozorgnia , Jong Soo Kim , Sebastian Liem , Christopher McCabe , Sydney Otten , Roberto Ruiz de Austri

Directional detection is a promising search strategy to discover galactic Dark Matter. Taking advantage on the rotation of the Solar system around the Galactic center through the Dark Matter halo, it allows to show a direction dependence of…

Cosmology and Nongalactic Astrophysics · Physics 2010-09-14 J. Billard , F. Mayet , D. Santos

The known direction of motion of dark matter particles relative to the Earth may be a key for their unambiguous identification even in the presence of backgrounds. We describe a prototype detector that is able to reconstruct direction…

We explore the ability of directional nuclear-recoil detectors to constrain the local velocity distribution of weakly interacting massive particle (WIMP) dark matter by performing Bayesian parameter estimation on simulated recoil-event data…

Cosmology and Nongalactic Astrophysics · Physics 2012-05-04 Samuel K. Lee , Annika H. G. Peter

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

Pixel tracklets, disappearing tracks reconstructed with only pixel hits, have proven to be a promising technique in LHC analyses to search for dark matter candidates at the LHC that belong to a nearly-degenerate electroweak multiplet.…

High Energy Physics - Phenomenology · Physics 2023-03-22 Matthew Gignac , Can Kilic , Rakhi Mahbubani , Taewook Youn

Inelastic dark matter reconciles the DAMA anomaly with other null direct detection experiments and points to a non-minimal structure in the dark matter sector. In addition to the dominant inelastic interaction, dark matter scattering may…

High Energy Physics - Phenomenology · Physics 2015-03-13 Mariangela Lisanti , Jay G. Wacker

The nature of dark matter (DM) remains one of the most fundamental open questions in physics. Among the main DM candidates are Weakly Interacting Massive Particles (WIMPs), expected to interact with matter through scattering. Directional…

High Energy Physics - Experiment · Physics 2025-09-16 David José Gaspar Marques

The aim of the MIMAC project is to detect non-baryonic Dark Matter with a directional TPC. The recent Micromegas efforts towards building a large size detector will be described, in particular the characterization measurements of a…

A direction sensitive dark matter detector using organic crystals is being developed. It exploits the anisotropic scintillation efficiency of organic crystals with respect to the direction of nuclear recoils relative to crystallographic…

Astrophysics · Physics 2016-12-07 H. Sekiya , M. Minowa , Y. Shimizu , W. Suganuma , Y. Inoue

New techniques for the laboratory direct detection of dark matter weakly interacting massive particles (WIMPs) are sensitive to the recoil direction of the struck nuclei. We compute and compare the directional recoil rates…

Astrophysics · Physics 2008-11-26 Moqbil S. Alenazi , Paolo Gondolo

Velocity distribution of dark matter is supposed to be isotropic Maxwell-Boltzmann distribution in most cases, however, other distribution models including anisotropic one are suggested by simulations. Directional direct detection of dark…

Cosmology and Nongalactic Astrophysics · Physics 2019-09-20 Keiko I. Nagao

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

Light dark matter in the context of dark sector theories is an attractive candidate for the dark matter thought to make up the bulk of the mass of our universe. We explore here the possibility of using a low-pressure, negative-ion, time…

Instrumentation and Methods for Astrophysics · Physics 2019-03-27 D. P. Snowden-Ifft , J. L. Harton , N. Ma , F. G. Schuckman

A new fitting method is explored for momentum reconstruction of tracks in a constant magnetic field for a silicon-strip tracker. Substantial increases of momentum resolution respect to standard fit is obtained. The key point is the use of a…

Instrumentation and Detectors · Physics 2018-12-11 Gregorio Landi , Giovanni E. Landi

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…