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A novel mechanism to produce and detect Light Dark Matter in experiments making use of GeV electrons (and positrons) impinging on a thick target (beam-dump) is proposed. The positron-rich environment produced by the electromagnetic shower…

High Energy Physics - Experiment · Physics 2018-08-01 L. Marsicano , M. Battaglieri , M. Bondì , C. D. R. Carvajal , A. Celentano , M. De Napoli , R. De Vita , E. Nardi , M. Raggi , P. Valente

Semiconductors are by now well-established targets for direct detection of MeV to GeV dark matter via scattering off electrons. We show that semiconductor targets can also detect significantly lighter dark matter via an absorption process.…

High Energy Physics - Phenomenology · Physics 2017-04-17 Yonit Hochberg , Tongyan Lin , Kathryn M. Zurek

Dark matter (DM) particles with mass in the sub-GeV range are an attractive alternative to heavier weakly-interacting massive particles, but direct detection of such light particles is challenging. If however DM-nucleus scattering leads to…

High Energy Physics - Phenomenology · Physics 2018-09-12 Matthew J. Dolan , Felix Kahlhoefer , Christopher McCabe

Traditional direct searches for dark matter, looking for nuclear recoils in deep underground detectors, are challenged by an almost complete loss of sensitivity for light dark matter particles. Consequently, there is a significant effort in…

High Energy Physics - Phenomenology · Physics 2020-04-22 Kyrylo Bondarenko , Alexey Boyarsky , Torsten Bringmann , Marco Hufnagel , Kai Schmidt-Hoberg , Anastasia Sokolenko

Dark matter is poorly constrained by direct detection experiments at masses below 1 MeV. This is an important target for the next generation of experiments, and several methods have been proposed to probe this mass range. One class of such…

High Energy Physics - Phenomenology · Physics 2020-07-31 Benjamin V. Lehmann , Stefano Profumo

We present new constraints on sub-GeV dark matter particles scattering off electrons in argon based on an analysis of ionization signal data from the DarkSide-50 detector.

Cosmology and Nongalactic Astrophysics · Physics 2018-10-05 The DarkSide Collaboration , P. Agnes , I. F. M. Albuquerque , T. Alexander , A. K. Alton , G. R. Araujo , D. M. Asner , M. Ave , H. O. Back , B. Baldin , G. Batignani , K. Biery , V. Bocci , G. Bonfini , W. Bonivento , B. Bottino , F. Budano , S. Bussino , M. Cadeddu , M. Cadoni , F. Calaprice , A. Caminata , N. Canci , A. Candela , M. Caravati , M. Cariello , M. Carlini , M. Carpinelli , S. Catalanotti , V. Cataudella , P. Cavalcante , S. Cavuoti , R. Cereseto , A. Chepurnov , C. Cicalò , L. Cifarelli , A. G. Cocco , G. Covone , D. D'Angelo , M. D'Incecco , D. D'Urso , S. Davini , A. De Candia , S. De Cecco , M. De Deo , G. De Filippis , G. De Rosa , M. De Vincenzi , P. Demontis , A. V. Derbin , A. Devoto , F. Di Eusanio , G. Di Pietro , C. Dionisi , M. Downing , E. Edkins , A. Empl , A. Fan , G. Fiorillo , K. Fomenko , D. Franco , F. Gabriele , A. Gabrieli , C. Galbiati , P. Garcia Abia , C. Ghiano , S. Giagu , C. Giganti , G. K. Giovanetti , O. Gorchakov , A. M. Goretti , F. Granato , M. Gromov , M. Guan , Y. Guardincerri , M. Gulino , B. R. Hackett , M. H. Hassanshahi , K. Herner , B. Hosseini , D. Hughes , P. Humble , E. V. Hungerford , Al. Ianni , An. Ianni , V. Ippolito , I. James , T. N. Johnson , Y. Kahn , K. Keeter , C. L. Kendziora , I. Kochanek , G. Koh , D. Korablev , G. Korga , A. Kubankin , M. Kuss , M. La Commara , M. Lai , X. Li , M. Lisanti , M. Lissia , B. Loer , G. Longo , Y. Ma , A. A. Machado , I. N. Machulin , A. Mandarano , L. Mapelli , S. M. Mari , J. Maricic , C. J. Martoff , A. Messina , P. D. Meyers , R. Milincic , S. Mishra-Sharma , A. Monte , M. Morrocchi , B. J. Mount , V. N. Muratova , P. Musico , R. Nania , A. Navrer Agasson , A. O. Nozdrina , A. Oleinik , M. Orsini , F. Ortica , L. Pagani , M. Pallavicini , L. Pandola , E. Pantic , E. Paoloni , F. Pazzona , K. Pelczar , N. Pelliccia , V. Pesudo , E. Picciau , A. Pocar , S. Pordes , S. S. Poudel , D. A. Pugachev , H. Qian , F. Ragusa , M. Razeti , A. Razeto , B. Reinhold , A. L. Renshaw , M. Rescigno , Q. Riffard , A. Romani , B. Rossi , N. Rossi , D. Sablone , O. Samoylov , W. Sands , S. Sanfilippo , M. Sant , R. Santorelli , C. Savarese , E. Scapparone , B. Schlitzer , E. Segreto , D. A. Semenov , A. Shchagin , A. Sheshukov , P. N. Singh , M. D. Skorokhvatov , O. Smirnov , A. Sotnikov , C. Stanford , S. Stracka , G. B. Suffritti , Y. Suvorov , R. Tartaglia , G. Testera , A. Tonazzo , P. Trinchese , E. V. Unzhakov , M. Verducci , A. Vishneva , B. Vogelaar , M. Wada , T. J. Waldrop , H. Wang , Y. Wang , A. W. Watson , S. Westerdale , M. M. Wojcik , M. Wojcik , X. Xiang , X. Xiao , C. Yang , Z. Ye , C. Zhu , A. Zichichi , G. Zuzel

We present constraints on low-mass dark matter electron scattering and absorption interactions using a SuperCDMS high-voltage eV-resolution (HVeV) detector. Data were taken underground in the NEXUS facility located at Fermilab with an…

High Energy Physics - Experiment · Physics 2026-03-17 SuperCDMS Collaboration , M. F. Albakry , I. Alkhatib , D. Alonso-González , J. Anczarski , T. Aralis , T. Aramaki , I. Ataee Langroudy , 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 , S. Dharani , M. L. di Vacri , M. D. Diamond , M. Elwan , S. Fallows , E. Fascione , E. Figueroa-Feliciano , S. L. Franzen , A. Gevorgian , M. Ghaith , G. Godden , J. Golatkar , S. R. Golwala , R. Gualtieri , J. Hall , S. A. S. Harms , C. Hays , B. A. Hines , Z. Hong , L. Hsu , M. E. Huber , V. Iyer , V. K. S. Kashyap , S. T. D. Keller , M. H. Kelsey , K. T. Kennard , Z. Kromer , A. Kubik , N. A. Kurinsky , M. Lee , J. Leyva , B. Lichtenberg , J. Liu , Y. Liu , E. Lopez Asamar , P. Lukens , R. López Noé , D. B. MacFarlane , R. Mahapatra , J. S. Mammo , N. Mast , A. J. Mayer , P. C. McNamara , H. Meyer zu Theenhausen , É. Michaud , E. Michielin , K. Mickelson , N. Mirabolfathi , M. Mirzakhani , B. Mohanty , D. Mondal , D. Monteiro , J. Nelson , H. Neog , V. Novati , J. L. Orrell , M. D. Osborne , S. M. Oser , L. Pandey , S. Pandey , R. Partridge , P. K. Patel , D. S. Pedreros , W. Peng , W. L. Perry , R. Podviianiuk , M. Potts , S. S. Poudel , A. Pradeep , M. Pyle , W. Rau , R. Ren , T. Reynolds , M. Rios , A. Roberts , A. E. Robinson , L. Rosado Del Rio , J. L. Ryan , T. Saab , D. Sadek , B. Sadoulet , S. P. Sahoo , I. Saikia , S. Salehi , J. Sander , B. Sandoval , A. Sattari , B. Schmidt , R. W. Schnee , B. Serfass , A. E. Sharbaugh , R. S. Shenoy , A. Simchony , P. Sinervo , Z. J. Smith , R. Soni , K. Stifter , J. Street , M. Stukel , H. Sun , E. Tanner , N. Tenpas , D. Toback , A. N. Villano , J. Viol , B. von Krosigk , Y. Wang , O. Wen , Z. Williams , M. J. Wilson , J. Winchell , S. Yellin , B. A. Young , B. Zatschler , S. Zatschler , A. Zaytsev , E. Zhang , L. Zheng , A. Zuniga , M. J. Zurowski

Dark matter in the sub-GeV mass range is a theoretically motivated but largely unexplored paradigm. Such light masses are out of reach for conventional nuclear recoil direct detection experiments, but may be detected through the small…

High Energy Physics - Phenomenology · Physics 2016-04-26 Rouven Essig , Marivi Fernandez-Serra , Jeremy Mardon , Adrian Soto , Tomer Volansky , Tien-Tien Yu

Dark matter with mass below about a GeV is essentially unobservable in conventional direct detection experiments. However, newly proposed technology will allow the detection of single electron events in semiconductor materials with…

High Energy Physics - Phenomenology · Physics 2012-11-13 Peter W. Graham , David E. Kaplan , Surjeet Rajendran , Matthew T. Walters

One of the next frontiers in dark-matter direct-detection experiments is to explore the MeV to GeV mass regime. Such light dark matter does not carry enough kinetic energy to produce an observable nuclear recoil, but it can scatter off…

High Energy Physics - Phenomenology · Physics 2017-09-11 Samuel K. Lee , Mariangela Lisanti , Siddharth Mishra-Sharma , Benjamin R. Safdi

We report on a search for sub-GeV dark matter (DM) particles interacting with electrons using the DAMIC-M prototype detector at the Modane Underground Laboratory. The data feature a significantly lower detector single $e^-$ rate (factor 50)…

Dark matter particles may bind with nuclei if there exists an attractive force of sufficient strength. We show that a dark photon mediator of mass $\sim (10 - 100)$ MeV that kinetically mixes with Standard Model electromagnetism at the…

High Energy Physics - Phenomenology · Physics 2021-10-14 Asher Berlin , Hongwan Liu , Maxim Pospelov , Harikrishnan Ramani

We describe an approach to detect dark matter and other invisible particles with mass below a GeV, exploiting missing energy-momentum measurements and other kinematic features of fixed-target production. In the case of an invisibly decaying…

High Energy Physics - Phenomenology · Physics 2015-05-27 Eder Izaguirre , Gordan Krnjaic , Philip Schuster , Natalia Toro

We study in detail sub-GeV dark matter scattering off electrons in xenon, including the expected electron recoil spectra and annual modulation spectra. We derive improved constraints using low-energy XENON10 and XENON100 ionization-only…

High Energy Physics - Phenomenology · Physics 2017-09-06 Rouven Essig , Tomer Volansky , Tien-Tien Yu

We revisit the detection of luminous dark matter in direct detection experiments. In this scenario, dark matter scatters endothermically to produce an excited state, which decays to produce a photon. We explore ways in which the electron…

High Energy Physics - Phenomenology · Physics 2022-11-17 Nicole F. Bell , James B. Dent , Bhaskar Dutta , Jason Kumar , Jayden L. Newstead

We present improved germanium-based constraints on sub-GeV dark matter via dark matter--electron ($\chi$-$e$) scattering using the 205.4 kg$\cdot$day dataset from the CDEX-10 experiment. Using a novel calculation technique, we attain…

We derive new bounds on hadronically-interacting, sub-GeV mass dark matter. First, we show that one-loop interactions with photons can be sufficient to maintain equilibrium between the dark matter and Standard Model sectors at MeV…

High Energy Physics - Phenomenology · Physics 2025-12-17 Peter Cox , Matthew J. Dolan , Joshua Wood

Proposed dark matter detectors with eV-scale sensitivities will detect a large background of atomic (nuclear) recoils from coherent photon scattering. This background climbs steeply below $\sim10$~eVnr, far exceeding the declining rate of…

Instrumentation and Methods for Astrophysics · Physics 2017-04-05 Alan E. Robinson

GeV-scale dark matter particles with strong coupling to baryons evade the standard direct detection limits as they are efficiently stopped in the overburden and, consequently, are not able to reach the underground detectors. On the other…

High Energy Physics - Phenomenology · Physics 2022-11-15 Helena Kolesova