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Related papers: Direct Dark Matter search with the XENON program

200 papers

The Cryogenic Dark Matter Search (CDMS-II) employs low-temperature Ge and Si detectors to seek Weakly Interacting Massive Particles (WIMPs) via their elastic scattering interactions with nuclei. Simultaneous measurements of both ionization…

Astrophysics · Physics 2012-08-27 CDMS Collaboration

We present results of a dark matter search performed with a 0.6 kg day exposure of the DAMIC experiment at the SNOLAB underground laboratory. We measure the energy spectrum of ionization events in the bulk silicon of charge-coupled devices…

The XENON1T experiment is the most recent stage of the XENON Dark Matter Search, aiming for the direct detection of Weakly Interacting Massive Particles (WIMPs). To reach its projected sensitivity, the background has to be reduced by two…

Instrumentation and Detectors · Physics 2017-06-28 Christopher Geis , Cyril Grignon , Uwe Oberlack , Diego Ramírez García , Quirin Weitzel

In this paper we assess the present status of dark matter direct searches by means of Bayesian statistics. We consider three particle physics models for spin-independent dark matter interaction with nuclei: elastic, inelastic and isospin…

High Energy Physics - Phenomenology · Physics 2013-05-30 Chiara Arina

The NEXT-100 time projection chamber, currently under construction, will search for neutrinoless double beta decay (bb0nu) using 100-150 kg of high-pressure xenon gas enriched in the Xe-136 isotope to ~91%. The detector possesses two…

Instrumentation and Detectors · Physics 2019-08-13 J. Martin-Albo , J. J. Gomez-Cadenas

As astronomical observations and their interpretation improve, the case for cold dark matter (CDM) becomes increasingly persuasive. A particularly appealing version of CDM is a weakly interacting massive particle (WIMP) with a mass near the…

High Energy Physics - Phenomenology · Physics 2022-10-28 Bailey Tallman , Alexandra Boone , Adhithya Vijayakumar , Fiona Lopez , Samuel Apata , Jehu Martinez , Roland Allen

The EDELWEISS-II collaboration has performed a direct search for WIMP dark matter with an array of ten 400-g heat-and-ionization cryogenic detectors equipped with Inter-Digit electrodes for the rejection of near-surface events. Results from…

High Energy Physics - Experiment · Physics 2011-06-09 Torrento-Coello , A. S

Multiply-interacting massive particles (MIMPs) are heavy (>10^10 GeV/c^2) dark matter particles that interact strongly with regular matter, but may have evaded detection due to the low number density required to make up the local dark…

High Energy Physics - Phenomenology · Physics 2022-01-12 Michael Clark , Amanda Depoian , Bahaa Elshimy , Abigail Kopec , Rafael F. Lang , Shengchao Li , Juehang Qin

An ultimate liquid xenon experiment would be limited in its dark matter science reach by irreducible neutrino backgrounds, which are an exciting signal in their own right. To achieve such sensitivity, other backgrounds that currently plague…

High Energy Physics - Experiment · Physics 2024-02-27 Abigail Kopec

A recently proposed dark matter WIMP has only second-order couplings to gauge bosons and itself. As a result, it has small annihilation, scattering, and creation cross-sections, and is consequently consistent with all current experiments…

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

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

Direct detection experiments turn to lose sensitivity of searching for a sub-MeV light dark matter candidate due to the threshold of recoil energy. However, such light dark matter particles can be accelerated by energetic cosmic-rays such…

High Energy Physics - Phenomenology · Physics 2021-05-26 Qing-Hong Cao , Ran Ding , Qian-Fei Xiang

Now that conventional weakly interacting massive particle (WIMP) dark matter searches are approaching the neutrino floor, there has been a resurgence of interest in detectors with sensitivity to nuclear recoil directions. A large-scale…

We report the results of a weakly-interacting massive particle (WIMP) dark matter search using the full 80.1\;live-day exposure of the first stage of the PandaX experiment (PandaX-I) located in the China Jin-Ping Underground Laboratory. The…

As part of the T-REX project, a number of R&D and prototyping activities have been carried out during the last years to explore the applicability of Micromegas-read gaseous TPCs in rare event searches like double beta decay (DBD), axion…

The CDMS II experiment uses Z-dependent Ionization Phonon (ZIP) detectors made of Germanium and Silicon to identify nuclear recoils from Weakly Interacting Massive Particles (WIMPs) with near complete event-by-event rejection of various…

Astrophysics · Physics 2007-05-23 Samuel Leclercq

We report a new search of weakly interacting massive particles (WIMPs) using the combined low background data sets in 2016 and 2017 from the PandaX-II experiment in China. The latest data set contains a new exposure of 77.1 live day, with…

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