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Related papers: QUEST-DMC superfluid $^3$He detector for sub-GeV d…

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We propose a new approach to search for light dark matter (DM), with keV-GeV mass, via inelastic nucleus scattering at large-volume neutrino detectors such as Borexino, DUNE, Super-K, Hyper-K, and JUNO. The approach uses inelastic nuclear…

High Energy Physics - Phenomenology · Physics 2024-10-21 Bhaskar Dutta , Wei-Chih Huang , Doojin Kim , Jayden L. Newstead , Jong-Chul Park , Iman Shaukat Ali

The next generation of rare-event searches, such as those aimed at determining the nature of particle dark matter or in measuring fundamental neutrino properties, will benefit from particle detectors with thresholds at the meV scale,…

The astrophysics community is considering plans for a variety of gamma-ray telescopes (including ACT and GRIPS) in the energy range 1--100 MeV, which can fill in the so-called "MeV gap" in current sensitivity. We investigate the utility of…

Cosmology and Nongalactic Astrophysics · Physics 2015-09-15 Kimberly K. Boddy , Jason Kumar

The Sub-Electron-Noise Skipper CCD Experimental Instrument (SENSEI) uses the recently developed Skipper-CCD technology to search for electron recoils from the interaction of sub-GeV dark matter particles with electrons in silicon. We report…

The SPICE/HeRALD collaboration is performing R&D to enable studies of sub-GeV dark matter models using a variety of target materials. Here we report our recent progress on instrumenting a superfluid $^4$He target mass with a transition-edge…

The problem of the dark matter in the universe is reviewed. A short history of the subject is given, and several of the most obvious particle candidates for dark matter are identified. Particular focus is given to weakly interacting,…

High Energy Astrophysical Phenomena · Physics 2012-06-15 Lars Bergström

This article presents constraints on dark-matter-electron interactions obtained from the first underground data-taking campaign with multiple SuperCDMS HVeV detectors operated in the same housing. An exposure of 7.63 g-days is used to set…

High Energy Physics - Experiment · Physics 2025-05-26 SuperCDMS Collaboration , M. F. Albakry , I. Alkhatib , D. Alonso-González , D. W. P. Amaral , J. Anczarski , T. Aralis , T. Aramaki , I. J. Arnquist , I. Ataee Langroudy , E. Azadbakht , C. Bathurst , R. Bhattacharyya , A. J. Biffl , P. L. Brink , M. Buchanan , R. Bunker , B. Cabrera , R. Calkins , R. A. Cameron , C. Cartaro , D. G. Cerdeño , Y. -Y. Chang , M. Chaudhuri , J. -H. Chen , R. Chen , N. Chott , J. Cooley , H. Coombes , P. Cushman , R. Cyna , S. Das , F. De Brienne , S. Dharani , M. L. di Vacri , M. D. Diamond , M. Elwan , E. Fascione , E. Figueroa-Feliciano , K. Fouts , M. Fritts , R. Germond , M. Ghaith , S. R. Golwala , J. Hall , S. A. S. Harms , K. Harris , N. Hassan , Z. Hong , E. W. Hoppe , L. Hsu , M. E. Huber , V. Iyer , D. Jardin , V. K. S. Kashyap , S. T. D. Keller , M. H. Kelsey , K. T. Kennard , A. Kubik , N. A. Kurinsky , M. Lee , J. Leyva , J. Liu , Y. Liu , B. Loer , E. Lopez Asamar , P. Lukens , D. B. MacFarlane , R. Mahapatra , J. S. Mammo , N. Mast , A. J. Mayer , H. Meyer zu Theenhausen , É. Michaud , E. Michielin , N. Mirabolfathi , M. Mirzakhani , B. Mohanty , D. Monteiro , J. Nelson , H. Neog , V. Novati , J. L. Orrell , M. D. Osborne , S. M. Oser , L. Pandey , S. Pandey , R. Partridge , D. S. Pedreros , W. Peng , L. Perna , W. L. Perry , R. Podviianiuk , S. S. Poudel , A. Pradeep , M. Pyle , W. Rau , E. Reid , R. Ren , T. Reynolds , M. Rios , A. Roberts , A. E. Robinson , J. L. Ryan , T. Saab , D. Sadek , B. Sadoulet , S. P. Sahoo , I. Saikia , J. Sander , A. Sattari , B. Schmidt , R. W. Schnee , S. Scorza , B. Serfass , A. Simchony , D. J. Sincavage , P. Sinervo , J. Street , H. Sun , E. Tanner , G. D. Terry , D. Toback , S. Verma , A. N. Villano , B. von Krosigk , S. L. Watkins , O. Wen , Z. Williams , M. J. Wilson , J. Winchell , K. Wykoff , S. Yellin , B. A. Young , T. C. Yu , B. Zatschler , S. Zatschler , A. Zaytsev , E. Zhang , L. Zheng , A. Zuniga , M. J. Zurowski

Dark Matter experiments are recently focusing their detection techniques in low-mass WIMPs, which requires the use of light elements and low energy threshold. In this context, we present the TREX-DM experiment, a low background…

Dark matter lighter than 10 GeV/c$^2$ encompasses a promising range of candidates. A conceptual design for a new detector, DarkSide-LowMass, is presented, based on the DarkSide-50 detector and progress toward DarkSide-20k, optimized for a…

Instrumentation and Detectors · Physics 2023-06-21 P. Agnes , I. Ahmad , S. Albergo , I. F. M. Albuquerque , T. Alexander , A. K. Alton , P. Amaudruz , M. Atzori Corona , D. J. Auty , M. Ave , I. Ch. Avetisov , R. I. Avetisov , O. Azzolini , H. O. Back , Z. Balmforth , V. Barbarian , A. Barrado Olmedo , P. Barrillon , A. Basco , G. Batignani , E. Berzin , A. Bondar , W. M. Bonivento , E. Borisova , B. Bottino , M. G. Boulay , G. Buccino , S. Bussino , J. Busto , A. Buzulutskov , M. Cadeddu , M. Cadoni , A. Caminata , N. Canci , A. Capra , S. Caprioli , M. Caravati , M. Cárdenas-Montes , N. Cargioli , M. Carlini , P. Castello , V. Cataudella , P. Cavalcante , S. Cavuoti , S. Cebrian , J. M. Cela Ruiz , S. Chashin , A. Chepurnov , E Chyhyrynets , C. Cicalò , L. Cifarelli , D. Cintas , V. Cocco , E. Conde Vilda , L. Consiglio , S. Copello , G. Covone , S. Cross , P. Czudak , M. D'Aniello , S. D'Auria , M. D. Da Rocha Rolo , O. Dadoun , M. Daniel , S. Davini , A. De Candia , S. De Cecco , A. De Falco , G. De Filippis , D. De Gruttola , S. De Pasquale , G. De Rosa , G. Dellacasa , A. V. Derbin , A. Devoto , F. Di Capua , L. Di Noto , P. Di Stefano , C. Dionisi , G. Dolganov , F. Dordei , L. Doria , T. Erjavec , M. Fernandez Diaz , G. Fiorillo , A. Franceschi , P. Franchini , D. Franco , E. Frolov , N. Funicello , F. Gabriele , D. Gahan , C. Galbiati , G. Gallina , G. Gallus , M. Garbini , P. Garcia Abia , A. Gendotti , C. Ghiano , R. A. Giampaolo , C. Giganti , M. A. Giorgi , G. K. Giovanetti , V. Goicoechea Casanueva , A. Gola , D. Gorman , R. Graciani Diaz , G. Grauso , G. Grilli di Cortona , A. Grobov , M. Gromov , M. Guan , M. Guerzoni , M. Gulino , C. Guo , B. R. Hackett , J. B. Hall , A. L. Hallin , A. Hamer , H. Helton , M. Haranczyk , T. Hessel , S. Hill , S. Horikawa , F. Hubaut , T. Hugues , E. V. Hungerford , An. Ianni , V. Ippolito , C. Jillings , P. Kachru , A. A. Kemp , C. L. Kendziora , G. Keppel , A. V. Khomyakov , M. Kimura , I. Kochanek , K. Kondo , G. Korga , S. Koulosousas , A. Kubankin , M. Kuss , M. Kuźniak , M. La Commara , M. Lai , E. Le Guirriec , E. Leason , X. Li , L. Lidey , J. Lipp , M. Lissia , G. Longo , L. Luzzi , O. Macfadyen , I. N. Machulin , I. Manthos , L. Mapelli , A. Margotti , S. M. Mari , C. Mariani , J. Maricic , A. Marini , M. Martínez , C. J. Martoff , A. Masoni , K. Mavrokoridis , A. Mazzi , A. B. McDonald , A. Messina , R. Milincic , A. Moggi , A. Moharana , J. Monroe , M. Morrocchi , E. N. Mozhevitina , T. Mróz , V. N. Muratova , C. Muscas , P. Musico , R. Nania , T. Napolitano , M. Nessi , G. Nieradka , K. Nikolopoulos , I. Nikulin , 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 , C. Pellegrino , F. Perotti , V. Pesudo , S. Piacentini , F. Pietropaolo , N. Pino , C. Pira , A. Pocar , D. M. Poehlmann , S. Pordes , P. Pralavorio , D. Price , F. Raffaelli , F. Ragusa , Y. Ramachers , A. Ramirez , M. Razeti , A. Razeto , A. L. Renshaw , M. Rescigno , F. Resnati , F. Retiere , L. P. Rignanese , C. Ripoli , A. Rivetti , A. Roberts , C. Roberts , J. Rode , G. Rogers , L. Romero , M. Rossi , A. Rubbia , S. Sadashivajois , T. R. Saffold , O. Samoylov , E. Sandford , S. Sanfilippo , D. Santone , R. Santorelli , C. Savarese , E. Scapparone , G. Scioli , D. A. Semenov , A. Shchagin , A. Sheshukov , M. Simeone , P. Skensved , M. D. Skorokhvatov , O. Smirnov , T. Smirnova , B. Smith , A. Sokolov , M. Spangenberg , R. Stefanizzi , A. Steri , S. Stracka , V. Strickland , M. Stringer , S. Sulis , A. Sung , Y. Suvorov , A. M. Szelc , C. Türkoğ , R. Tartaglia , A. Taylor , J. Taylor , S. Tedesco , G. Testera , K. Thieme , T. N. Thorpe , A. Tonazzo , S. Torres-Lara , A. Tricomi , E. V. Unzhakov , T. Vallivilayil John , M. Van Uffelen , T. Viant , S. Viel , A. Vishneva , R. B. Vogelaar , J. Vossebeld , M. Wada , M. B. Walczak , Y. Wang , S. Westerdale , R. J. Wheadon , L. Williams , I. Wingerter-Seez , R. Wojaczyński , Ma. M. Wojcik , Ma. Wojcik , T. Wright , Y. Xie , C. Yang , A. Zabihi , P. Zakhary , A. Zani , A. Zichichi , G. Zuzel , M. P. Zykova

We employ an effective field theory to study the detectability of sub-GeV dark matter through its interaction with the gapless excitations of superfluid helium-4. In a quantum field theory language, the possible interactions between the…

High Energy Physics - Phenomenology · Physics 2019-07-03 Francesca Acanfora , Angelo Esposito , Antonio D. Polosa

Direct detection experiments for light (sub-GeV) dark matter are making enormous leaps in reaching previously unexplored theory space. The need for accurate characterizations of target responses has led to a growing interplay between…

High Energy Physics - Phenomenology · Physics 2022-03-16 Andrea Mitridate , Tanner Trickle , Zhengkang Zhang , Kathryn M. Zurek

Light Dark Matter (DM), defined here as having a mass between 1 MeV and about 1 GeV, is an interesting possibility both theoretically and phenomenologically, at one of the frontiers of current progress in the field of DM searches. Its…

High Energy Physics - Phenomenology · Physics 2022-07-06 Marco Cirelli , Nicolao Fornengo , Bradley J. Kavanagh , Elena Pinetti

This work analyzes the detection prospects for weakly interacting massive particles (WIMPs) in dark matter (DM) density spikes around nearby supermassive black holes (SMBHs) by observations in very high energy gamma-ray band. Such spikes…

High Energy Astrophysical Phenomena · Physics 2025-12-12 Andrei E. Egorov

The WIMPs are considered one of the favorable dark matter (DM) candidates, but as the upper bounds on the interactions between DM and standard model (SM) particles obtained by the upgraded facilities of DM direct detections get lower and…

High Energy Physics - Phenomenology · Physics 2017-02-01 Lian-Bao Jia , Xue-Qian Li

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…

Bosonic superweakly interacting massive particles (super-WIMPs) are a candidate for warm dark matter. With the absorption of such a boson by a xenon atom these dark matter candidates would deposit an energy equivalent to their rest mass in…

Superconducting targets have recently been proposed for the direct detection of dark matter as light as a keV, via elastic scattering off conduction electrons in Cooper pairs. Detecting such light dark matter requires sensitivity to…

High Energy Physics - Phenomenology · Physics 2016-07-27 Yonit Hochberg , Tongyan Lin , Kathryn M. Zurek

We demonstrate that current and planned underground neutrino experiments could offer a powerful probe of few-MeV dark matter when combined with a nearby high-intensity low-to-medium energy electron accelerator. This experimental setup, an…

High Energy Physics - Phenomenology · Physics 2015-11-18 Eder Izaguirre , Gordan Krnjaic , Maxim Pospelov

The GAPS experiment is foreseen to carry out a dark matter search by measuring low-energy cosmic-ray antideuterons and antiprotons with a novel detection approach. It will provide a new avenue to access a wide range of different dark matter…

Instrumentation and Methods for Astrophysics · Physics 2015-08-14 P. von Doetinchem , T. Aramaki , S. Boggs , H. Fuke , C. J. Hailey , S. I. Mognet , R. A. Ong , K. Perez , J. Zweerink
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