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Experiments based on noble liquids and solid state cryogenic detectors have had a leading role in the direct detection of dark matter. But smaller scale projects can help to explore the new dark matter landscape with advanced,…

Instrumentation and Methods for Astrophysics · Physics 2020-05-20 Susana Cebrián

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

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

We examine the recently-reported low-energy electron recoil spectrum observed at the XENON1T underground dark matter direct detection experiment, in the context of new interactions with solar neutrinos. In particular we show that scalar and…

High Energy Physics - Phenomenology · Physics 2021-11-22 Celine Boehm , David G. Cerdeno , Malcolm Fairbairn , Pedro A. N. Machado , Aaron C. Vincent

This report describes the experimental strategy and technologies for XLZD, the next-generation xenon observatory sensitive to dark matter and neutrino physics. In the baseline design, the detector will have an active liquid xenon target of…

High Energy Physics - Experiment · Physics 2025-10-29 XLZD Collaboration , J. Aalbers , K. Abe , M. Adrover , S. Ahmed Maouloud , D. S. Akerib , A. K. Al Musalhi , F. Alder , L. Althueser , D. W. P. Amaral , C. S. Amarasinghe , A. Ames , B. Andrieu , N. Angelides , E. Angelino , B. Antunovic , E. Aprile , H. M. Araújo , J. E. Armstrong , M. Arthurs , M. Babicz , A. Baker , M. Balzer , J. Bang , E. Barberio , J. W. Bargemann , E. Barillier , A. Basharina-Freshville , L. Baudis , D. Bauer , M. Bazyk , K. Beattie , N. Beaupere , N. F. Bell , L. Bellagamba , T. Benson , A. Bhatti , T. P. Biesiadzinski , R. Biondi , Y. Biondi , H. J. Birch , E. Bishop , A. Bismark , C. Boehm , K. Boese , A. Bolotnikov , P. Brás , R. Braun , A. Breskin , C. A. J. Brew , S. Brommer , A. Brown , G. Bruni , R. Budnik , S. Burdin , C. Cai , C. Capelli , G. Carini , M. C. Carmona-Benitez , M. Carter , A. Chauvin , A. Chawla , H. Chen , J. J. Cherwinka , Y. T. Chin , N. I. Chott , A. P. Cimental Chavez , K. Clark , A. P. Colijn , D. J. Colling , J. Conrad , M. V. Converse , L. J. Cooper , R. Coronel , D. Costanzo , A. Cottle , G. Cox , J. J. Cuenca-García , D. Curran , D. Cussans , V. D'Andrea , L. C. Daniel Garcia , I. Darlington , S. Dave , A. David , G. J. Davies , M. P. Decowski , A. Deisting , J. Delgaudio , S. Dey , C. Di Donato , L. Di Felice , P. Di Gangi , S. Diglio , C. Ding , J. E. Y. Dobson , M. Doerenkamp , G. Drexlin , E. Druszkiewicz , C. L. Dunbar , K. Eitel , A. Elykov , R. Engel , S. R. Eriksen , S. Fayer , N. M. Fearon , A. D. Ferella , C. Ferrari , N. Fieldhouse , H. Fischer , H. Flaecher , T. Flehmke , M. Flierman , E. D. Fraser , T. M. A. Fruth , K. Fujikawa , W. Fulgione , C. Fuselli , P. Gaemers , R. Gaior , R. J. Gaitskell , N. Gallice , M. Galloway , F. Gao , N. Garroum , A. Geffre , J. Genovesi , C. Ghag , S. Ghosh , R. Giacomobono , R. Gibbons , F. Girard , R. Glade-Beucke , F. Glück , S. Gokhale , L. Grandi , J. Green , J. Grigat , M. G. D. van der Grinten , R. Größle , H. Guan , M. Guida , P. Gyorgy , J. J. Haiston , C. R. Hall , T. Hall , R. Hammann , V. Hannen , S. Hansmann-Menzemer , N. Hargittai , E. Hartigan-O'Connor , S. J. Haselschwardt , M. Hernandez , S. A. Hertel , A. Higuera , C. Hils , K. Hiraoka , L. Hoetzsch , M. Hoferichter , G. J. Homenides , N. F. Hood , M. Horn , D. Q. Huang , S. Hughes , D. Hunt , M. Iacovacci , Y. Itow , E. Jacquet , J. Jakob , R. S. James , F. Joerg , S. Jones , A. C. Kaboth , F. Kahlert , A. C. Kamaha , Y. Kaminaga , M. Kara , P. Kavrigin , S. Kazama , M. Keller , P. Kemp-Russell , D. Khaitan , P. Kharbanda , B. Kilminster , J. Kim , R. Kirk , M. Kleifges , M. Klute , M. Kobayashi , D. Kodroff , D. Koke , A. Kopec , E. V. Korolkova , H. Kraus , S. Kravitz , L. Kreczko , B. von Krosigk , V. A. Kudryavtsev , F. Kuger , N. Kurita , H. Landsman , R. F. Lang , C. Lawes , J. Lee , B. Lehnert , D. S. Leonard , K. T. Lesko , L. Levinson , A. Li , I. Li , S. Li , S. Liang , Z. Liang , J. Lin , Y. -T. Lin , S. Lindemann , S. Linden , M. Lindner , A. Lindote , W. H. Lippincott , K. Liu , J. Loizeau , F. Lombardi , J. A. M. Lopes , M. I. Lopes , W. Lorenzon , M. Loutit , C. Lu , G. M. Lucchetti , T. Luce , S. Luitz , Y. Ma , C. Macolino , J. Mahlstedt , B. Maier , P. A. Majewski , A. Manalaysay , A. Mancuso , L. Manenti , R. L. Mannino , F. Marignetti , T. Marley , T. Marrodán Undagoitia , K. Martens , J. Masbou , E. Masson , S. Mastroianni , C. Maupin , V. Mazza , C. McCabe , M. E. McCarthy , D. N. McKinsey , J. B. McLaughlin , A. Melchiorre , J. Menéndez , M. Messina , E. H. Miller , B. Milosovic , S. Milutinovic , K. Miuchi , R. Miyata , E. Mizrachi , A. Molinario , C. M. B. Monteiro , M. E. Monzani , K. Morå , S. Moriyama , E. Morrison , E. Morteau , Y. Mosbacher , B. J. Mount , J. Müller , M. Murdy , A. St. J. Murphy , M. Murra , A. Naylor , H. N. Nelson , F. Neves , J. L. Newstead , A. Nguyen , K. Ni , J. O'Dell , C. O'Hare , U. Oberlack , M. Obradovic , I. Olcina , K. C. Oliver-Mallory , G. D. Orebi Gann , J. Orpwood , S. Ouahada , K. Oyulmaz , B. Paetsch , K. J. Palladino , J. Palmer , Y. Pan , M. Pandurovic , N. J. Pannifer , S. Paramesvaran , S. J. Patton , Q. Pellegrini , B. Penning , G. Pereira , R. Peres , E. Perry , T. Pershing , F. Piastra , J. Pienaar , A. Piepke , M. Pierre , G. Plante , T. R. Pollmann , F. Pompa , L. Principe , J. Qi , K. Qiao , Y. Qie , J. Qin , S. Radeka , V. Radeka , M. Rajado , D. Ramírez García , A. Ravindran , A. Razeto , J. Reichenbacher , C. A. Rhyne , A. Richards , G. R. C. Rischbieter , H. S. Riyat , R. Rosero , A. Roy , T. Rushton , D. Rynders , R. Saakyan , L. Sanchez , P. Sanchez-Lucas , D. Santone , J. M. F. dos Santos , G. Sartorelli , A. B. M. R. Sazzad , A. Scaffidi , R. W. Schnee , J. Schreiner , P. Schulte , H. Schulze Eißing , M. Schumann , A. Schwenck , A. Schwenk , L. Scotto Lavina , M. Selvi , F. Semeria , P. Shagin , S. Sharma , S. Shaw , W. Shen , L. Sherman , S. Shi , S. Y. Shi , T. Shimada , T. Shutt , J. J. Silk , C. Silva , H. Simgen , G. Sinev , R. Singh , J. Siniscalco , M. Solmaz , V. N. Solovov , Z. Song , P. Sorensen , J. Soria , O. Stanley , M. Steidl , T. Stenhouse , A. Stevens , K. Stifter , T. J. Sumner , A. Takeda , P. -L. Tan , D. J. Taylor , W. C. Taylor , D. Thers , T. Thümmler , D. R. Tiedt , F. Tönnies , Z. Tong , F. Toschi , D. R. Tovey , J. Tranter , M. Trask , G. Trinchero , M. Tripathi , D. R. Tronstad , R. Trotta , C. D. Tunnell , P. Urquijo , A. Usón , M. Utoyama , A. C. Vaitkus , O. Valentino , K. Valerius , S. Vecchi , V. Velan , S. Vetter , L. de Viveiros , G. Volta , D. Vorkapic , A. Wang , J. J. Wang , Y. Wang , D. Waters , K. M. Weerman , C. Weinheimer , M. Weiss , D. Wenz , T. J. Whitis , K. Wild , M. Williams , M. Wilson , S. T. Wilson , C. Wittweg , J. Wolf , F. L. H. Wolfs , S. Woodford , D. Woodward , M. Worcester , C. J. Wright , V. H. S. Wu , S. Wüstling , M. Wurm , Q. Xia , Y. Xing , D. Xu , J. Xu , Y. Xu , Z. Xu , M. Yamashita , L. Yang , J. Ye , M. Yeh , B. Yu , G. Zavattini , W. Zha , M. Zhong , K. Zuber

Direct detection of light dark matter (DM), below the GeV scale, through electron recoil can be efficient if DM has a velocity well above the virial value of $v\sim 10^{-3}$. We point out that if there is a long range attractive force…

High Energy Physics - Phenomenology · Physics 2021-09-14 Hooman Davoudiasl , Peter B. Denton , Julia Gehrlein

Solving the Dark Matter enigma represents one of the key objectives of contemporary physics. Recent astrophysical and cosmological measurements have unambiguously demonstrated that ordinary matter contributes to less than 5 % of the energy…

Astrophysics · Physics 2015-06-24 Gabriel Chardin

The XMASS detector is a large single phase liquid Xenon scintillator.After its feasibility had been studied using a 100 kg size prototype detector, an 800 kg size detector is being built for dark matter search with the sensitivity of…

Instrumentation and Methods for Astrophysics · Physics 2019-08-13 Hiroyuki Sekiya

In recent years a new field emerged in dark matter community and immediately attracted a multitude of theoriests and experimentalists, that of light dark matter direct detection in electronic systems. The phenomenon is similar with nuclear…

High Energy Physics - Phenomenology · Physics 2018-08-29 Tairan Liang , Bin Zhu , Ran Ding , Tianjun Li

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…

Instrumentation and Detectors · Physics 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

Models of nuclear dark matter propose that the dark sector contains large composite states consisting of dark nucleons in analogy to Standard Model nuclei. We examine the direct detection phenomenology of a particular class of nuclear dark…

High Energy Physics - Phenomenology · Physics 2017-11-01 A. Butcher , R. Kirk , J. Monroe , S. M. West

AXEL is a high pressure xenon gas TPC detector being developed for neutrinoless double-beta decay search. We use the proportional scintillation mode with a new electroluminescence light detection system to achieve high energy resolution in…

Instrumentation and Detectors · Physics 2017-11-27 S. Ban , K. D. Nakamura , S. Akiyama , M. Hirose , A. K. Ichikawa , Y. Ishiyama , A. Minamino , K. Miuchi , T. Nakaya , H. Sekiya , S. Tanaka , K. Ueshima , S. Yanagita

As liquid xenon time projection chambers scale to ever-larger sizes, so too do the engineering challenges they pose. We describe a large, flexible, multipurpose test facility capable of supporting the development of a number of key aspects…

Instrumentation and Detectors · Physics 2025-11-14 Evan Angelico , Jacopo Dalmasson , Ralph DeVoe , Giorgio Gratta , Clarke A. Hardy , Brian Lenardo , Lin Si , Marie Vidal , Shuoxing Wu

In a seminal paper now a decade old, it was shown that dark matter detectors geared at probing interactions with nucleons could also be used to probe dark matter interactions with electrons. In this work, we show that new detector concepts…

High Energy Physics - Phenomenology · Physics 2024-12-24 Sinéad M. Griffin , Guy Daniel Hadas , Yonit Hochberg , Katherine Inzani , Benjamin V. Lehmann

We present the design and the sensitivity reach of the Qubit-based Light Dark Matter detection experiment. We propose the novel two-chip design to reduce signal dissipation, with quantum parity measurement to enhance single-phonon detection…

High Energy Physics - Phenomenology · Physics 2025-12-24 Xuegang Li , Yuxiang Liu , Jing Shu , Ningqiang Song , Yidong Song , Junhua Wang , Yue-Liang Wu , Tiantian Zhang , Yu-Feng Zhou

Underground laboratories host two kind of experiments at the frontier of our knowledge in Particle Physics, Astrophysics and Cosmology: the direct detection of the Dark Matter of the Universe and the search for the Neutrinoless Double Beta…

Cosmology and Nongalactic Astrophysics · Physics 2009-11-17 Igor G. Irastorza

We report the first precision measurement of the superheat temperature required for bubble nucleation in liquid xenon of $\Delta T_{wall,ONB}$ = (16.9$\pm$0.5) K and $\Delta T_{wall,ONB}$ = (19.2$^{+0.4}_{-1.1}$) K at pressures of P =…

Instrumentation and Detectors · Physics 2021-03-24 P. A. Breur , G. S. Ortega , P. C. Rowson , R. Saldanha , B. Mong , M. Oriunno , C. Mo

CERN has launched a study phase to evaluate the feasibility of a new high-intensity beam dump facility at the CERN Super Proton Synchrotron accelerator with the primary goal of exploring Hidden Sector models and searching for Light Dark…

Numerous astrophysical and cosmological observations are best explained by the existence of dark matter, a mass density which interacts only very weakly with visible, baryonic matter. Searching for the extremely weak signals produced by…

Current and future neutrino experiments can be used to discover dark matter, not only in searches for dark matter annihilating to neutrinos, but also in scenarios where dark matter itself scatters off Standard Model particles in the…

High Energy Physics - Phenomenology · Physics 2017-04-19 Lina Necib , Jarrett Moon , Taritree Wongjirad , Janet M. Conrad