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The CYGNO collaboration is developing a novel strategy for directional Dark Matter searches based on a gaseous Time Projection Chamber (TPC). The detector is optimized for the exploration of light (0.5-50 GeV) WIMPs-like particles and…

We study the sensitivity of large-scale xenon detectors to low-energy solar neutrinos, to coherent neutrino-nucleus scattering and to neutrinoless double beta decay. As a concrete example, we consider the xenon part of the proposed DARWIN…

仪器与探测器 · 物理学 2014-02-10 L. Baudis , A. Ferella , A. Kish , A. Manalaysay , T. Marrodan Undagoitia , M. Schumann

Ton-scale liquid xenon detectors operated in two-phase mode are proposed and being constructed recently to explore the favored parameter space for the Weakly Interacting Massive Particles (WIMPs) dark matter. To achieve a better light…

仪器与探测器 · 物理学 2014-05-13 Y Wei , Q Lin , X Xiao , K Ni

We study a three stage dark matter and neutrino observatory based on multi-ton two-phase liquid Xe and Ar detectors with sufficiently low backgrounds to be sensitive to WIMP dark matter interaction cross sections down to 10E-47 cm^2, and to…

天体物理仪器与方法 · 物理学 2015-03-19 K. Arisaka , P. Beltrame , C. W. Lam , P. F. Smith , C. Ghag , D. B. Cline , K. Lung , Y. Meng , E. Pantic , P. R. Scovell , A. Teymourian , H. Wang

The dark matter track at ICRC~2025 showed a field in transition. Direct detection has entered the \emph{neutrino-floor era}, with XENONnT and PandaX-4T now limited by Solar neutrinos. Indirect searches have become truly…

高能天体物理现象 · 物理学 2025-10-21 Milena Crnogorčević

Experiments that use liquid noble gasses as target materials, such as argon and xenon, play a significant role in direct detection searches for WIMP(-like) dark matter. As these experiments grow in size, they will soon encounter a new…

高能物理 - 唯象学 · 物理学 2023-05-05 Andrea Gaspert , Pietro Giampa , David E. Morrissey

We report on a blinded analysis of low-energy electronic-recoil data from the first science run of the XENONnT dark matter experiment. Novel subsystems and the increased 5.9 tonne liquid xenon target reduced the background in the (1, 30)…

高能物理 - 实验 · 物理学 2022-11-16 E. Aprile , K. Abe , F. Agostini , S. Ahmed Maouloud , L. Althueser , B. Andrieu , E. Angelino , J. R. Angevaare , V. C. Antochi , D. Antón Martin , F. Arneodo , L. Baudis , A. L. Baxter , L. Bellagamba , R. Biondi , A. Bismark , A. Brown , S. Bruenner , G. Bruno , R. Budnik , T. K. Bui , C. Cai , C. Capelli , J. M. R. Cardoso , D. Cichon , M. Clark , A. P. Colijn , J. Conrad , J. J. Cuenca-García , J. P. Cussonneau , V. D'Andrea , M. P. Decowski , P. Di Gangi , S. Di Pede , A. Di Giovanni , R. Di Stefano , S. Diglio , K. Eitel , A. Elykov , S. Farrell , A. D. Ferella , C. Ferrari , H. Fischer , W. Fulgione , P. Gaemers , R. Gaior , A. Gallo Rosso , M. Galloway , F. Gao , R. Gardner , R. Glade-Beucke , L. Grandi , J. Grigat , M. Guida , R. Hammann , A. Higuera , C. Hils , L. Hoetzsch , J. Howlett , M. Iacovacci , Y. Itow , J. Jakob , F. Joerg , A. Joy , N. Kato , M. Kara , P. Kavrigin , S. Kazama , M. Kobayashi , G. Koltman , A. Kopec , F. Kuger , H. Landsman , R. F. Lang , L. Levinson , I. Li , S. Li , S. Liang , S. Lindemann , M. Lindner , K. Liu , J. Loizeau , F. Lombardi , J. Long , J. A. M. Lopes , Y. Ma , C. Macolino , J. Mahlstedt , A. Mancuso , L. Manenti , F. Marignetti , T. Marrodán Undagoitia , K. Martens , J. Masbou , D. Masson , E. Masson , S. Mastroianni , M. Messina , K. Miuchi , K. Mizukoshi , A. Molinario , S. Moriyama , K. Morå , Y. Mosbacher , M. Murra , J. Müller , K. Ni , U. Oberlack , B. Paetsch , J. Palacio , P. Paschos , R. Peres , C. Peters , J. Pienaar , M. Pierre , V. Pizzella , G. Plante , J. Qi , J. Qin , D. Ramírez García , S. Reichard , A. Rocchetti , N. Rupp , L. Sanchez , J. M. F. dos Santos , I. Sarnoff , G. Sartorelli , J. Schreiner , D. Schulte , P. Schulte , H. Schulze Eißing , M. Schumann , L. Scotto Lavina , M. Selvi , F. Semeria , P. Shagin , S. Shi , E. Shockley , M. Silva , H. Simgen , J. Stephen , A. Takeda , P. -L. Tan , A. Terliuk , D. Thers , F. Toschi , G. Trinchero , C. Tunnell , F. Tönnies , K. Valerius , G. Volta , Y. Wei , C. Weinheimer , M. Weiss , D. Wenz , C. Wittweg , T. Wolf , D. Xu , Z. Xu , M. Yamashita , L. Yang , J. Ye , L. Yuan , G. Zavattini , M. Zhong , T. Zhu

The detection of Dark Matter (DM) remains a significant challenge in particle physics. This study exploits advanced machine learning models to improve detection capabilities of liquid xenon time projection chamber experiments, utilizing…

天体物理仪器与方法 · 物理学 2025-01-17 Daniel E. Lopez-Fogliani , Andres D. Perez , Roberto Ruiz de Austri

The GENIUS project is a proposal for a new dark matter detector, with an increased sensitivity of three orders of magnitude relative to existing direct dark matter detection experiments. We performed a technical study and calculated the…

高能物理 - 实验 · 物理学 2010-11-30 L. Baudis , G. Heusser , B. Majorovits , Y. Ramachers , H. Strecker , H. V. Klapdor--Kleingrothaus

If the dark matter particle has spin 0, only two types of WIMP-nucleon interaction can arise from the non-relativistic reduction of renormalisable single-mediator models for dark matter-quark interactions. Based on this crucial observation,…

高能物理 - 唯象学 · 物理学 2018-01-17 Riccardo Catena , Jan Conrad , Christian Döring , Alfredo Davide Ferella , Martin B. Krauss

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…

LUX is a dual-phase xenon TPC designed for the direct detection of dark matter. Using 370 kg of xenon, LUX is capable of setting a WIMP-nucleon cross section limit at 2 x 10^-46 cm^2 after 300 days of running. LUX will surpass all existing…

天体物理仪器与方法 · 物理学 2019-08-13 Michael Woods

An observation of the anisotropy of dark matter interactions in a direction-sensitive detector would provide decisive evidence for the discovery of galactic dark matter. Directional information would also provide a crucial input to…

高能物理 - 唯象学 · 物理学 2015-11-20 Gopolang Mohlabeng , Kyoungchul Kong , Jin Li , Adam Para , Jonghee Yoo

CDEX-50 is a next-generation project of the China Dark Matter Experiment (CDEX) that aims to search for dark matter using a 50-kg germanium detector array. This paper comprises a thorough summary of the CDEX-50 dark matter experiment,…

Dark matter detectors that utilize liquid xenon have now achieved tonne-scale targets, giving them sensitivity to all flavours of supernova neutrinos via coherent elastic neutrino-nucleus scattering. Considering for the first time a…

高能天体物理现象 · 物理学 2016-12-21 Rafael F. Lang , Christopher McCabe , Shayne Reichard , Marco Selvi , Irene Tamborra

The design and performance of the LUX-ZEPLIN (LZ) detector is described as of March 2015 in this Conceptual Design Report. LZ is a second-generation dark-matter detector with the potential for unprecedented sensitivity to weakly interacting…

仪器与探测器 · 物理学 2015-10-05 The LZ Collaboration , D. S. Akerib , C. W. Akerlof , D. Yu. Akimov , S. K. Alsum , H. M. Araújo , X. Bai , A. J. Bailey , J. Balajthy , S. Balashov , M. J. Barry , P. Bauer , P. Beltrame , E. P. Bernard , A. Bernstein , T. P. Biesiadzinski , K. E. Boast , A. I. Bolozdynya , E. M. Boulton , R. Bramante , J. H. Buckley , V. V. Bugaev , R. Bunker , S. Burdin , J. K. Busenitz , C. Carels , D. L. Carlsmith , B. Carlson , M. C. Carmona-Benitez , M. Cascella , C. Chan , J. J. Cherwinka , A. A. Chiller , C. Chiller , W. W. Craddock , A. Currie , J. E. Cutter , J. P. da Cunha , C. E. Dahl , S. Dasu , T. J. R. Davison , L. de Viveiros , A. Dobi , J. E. Y. Dobson , E. Druszkiewicz , T. K. Edberg , B. N. Edwards , W. R. Edwards , M. M. Elnimr , W. T. Emmet , C. H. Faham , S. Fiorucci , P. Ford , V. B. Francis , C. Fu , R. J. Gaitskell , N. J. Gantos , V. M. Gehman , R. M. Gerhard , C. Ghag , M. G. D. Gilchriese , B. Gomber , C. R. Hall , A. Harris , S. J. Haselschwardt , S. A. Hertel , M. D. Hoff , B. Holbrook , E. Holtom , D. Q. Huang , T. W. Hurteau , C. M. Ignarra , R. G. Jacobsen , W. Ji , X. Ji , M. Johnson , Y. Ju , K. Kamdin , K. Kazkaz , D. Khaitan , A. Khazov , A. V. Khromov , A. M. Konovalov , E. V. Korolkova , H. Kraus , H. J. Krebs , V. A. Kudryavtsev , A. V. Kumpan , S. Kyre , N. A. Larsen , C. Lee , B. G. Lenardo , K. T. Lesko , F. -T. Liao , J. Lin , A. Lindote , W. H. Lippincott , J. Liu , X. Liu , M. I. Lopes , W. Lorenzon , S. Luitz , P. Majewski , D. C. Malling , A. G. Manalaysay , L. Manenti , R. L. Mannino , D. J. Markley , T. J. Martin , M. F. Marzioni , D. N. McKinsey , D. -M. Mei , Y. Meng , E. H. Miller , J. Mock , M. E. Monzani , J. A. Morad , A. St. J. Murphy , H. N. Nelson , F. Neves , J. A. Nikkel , F. G. O'Neill , J. O'Dell , K. O'Sullivan , M. A. Olevitch , K. C. Oliver-Mallory , K. J. Palladino , M. Pangilinan , S. J. Patton , E. K. Pease , A. Piepke , S. Powell , R. M. Preece , K. Pushkin , B. N. Ratcliff , J. Reichenbacher , L. Reichhart , C. Rhyne , J. P. Rodrigues , H. J. Rose , R. Rosero , J. S. Saba , M. Sarychev , R. W. Schnee , M. S. G. Schubnell , P. R. Scovell , S. Shaw , T. A. Shutt , C. Silva , K. Skarpaas , W. Skulski , V. N. Solovov , P. Sorensen , V. V. Sosnovtsev , I. Stancu , M. R. Stark , S. Stephenson , T. M. Stiegler , T. J. Sumner , K. Sundarnath , M. Szydagis , D. J. Taylor , W. Taylor , B. P. Tennyson , P. A. Terman , K. J. Thomas , J. A. Thomson , D. R. Tiedt , W. H. To , A. Tomás , M. Tripathi , C. E. Tull , L. Tvrznikova , S. Uvarov , J. Va'vra , M. G. D. van der Grinten , J. R. Verbus , C. O. Vuosalo , W. L. Waldron , L. Wang , R. C. Webb , W. -Z. Wei , M. While , D. T. White , T. J. Whitis , W. J. Wisniewski , M. S. Witherell , F. L. H. Wolfs , E. Woods , D. Woodward , S. D. Worm , M. Yeh , J. Yin , S. K. Young , C. Zhang

NEXT-DEMO is a large-scale prototype of the NEXT-100 detector, an electroluminescent time projection chamber that will search for the neutrinoless double beta decay of Xe-136 using 100 to 150 kg of enriched xenon gas. NEXT-DEMO was built to…

Indirect detection of dark matter particles, i.e. the detection of annihilation or decay products of Weakly Interacting Massive Particles, has entered a pivotal phase as experiments reach sensitivities that probe the most interesting…

高能物理 - 唯象学 · 物理学 2014-11-10 Jan Conrad

Two-phase noble liquid detectors, with large target masses and effective background reduction, are currently leading the dark matter direct detection for WIMP masses above a few GeV. Due to their sensitivity to single ionized electron…

仪器与探测器 · 物理学 2020-03-24 A. Bernstein , M. Clark , R. Essig , M. Fernandez-Serra , A. Kopec , R. F. Lang , J. Long , K. Ni , S. Pereverzev , J. Qi , P. Sorensen , Y. Wei , J. Xu , J. Ye , C. Zhen

We present first competitive results on WIMP dark matter using the phonon-light-detection technique. A particularly strong limit for WIMPs with coherent scattering results from selecting a region of the phonon-light plane corresponding to…