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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

We present the first limits on inelastic electron-scattering dark matter and dark photon absorption using a prototype SuperCDMS detector having a charge resolution of 0.1 electron-hole pairs (CDMS HVeV, a 0.93 gram CDMS HV device). These…

Light new particles with masses below 10 keV, often considered as a plausible extension of the Standard Model, will be emitted from the solar interior, and can be detected on the Earth with a variety of experimental tools. Here we analyze…

High Energy Physics - Phenomenology · Physics 2013-08-21 Haipeng An , Maxim Pospelov , Josef Pradler

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 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

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 describe the TREX-DM experiment, a low background…

Instrumentation and Detectors · Physics 2016-06-22 F. J. Iguaz , J. G. Garza , F. Aznar , J. F. Castel , S. Cebrian , T. Dafni , J. A. Garcia , I. G. Irastorza , A. Lagraba , G. Luzon , A. Peiro

The nature of dark matter (DM) remains a mystery since it has so far eluded detection in the laboratory. To that end, the Large Underground Xenon (LUX) experiment was built to directly observe the interaction of DM with xenon target nuclei.…

Instrumentation and Methods for Astrophysics · Physics 2019-04-22 Lucie Tvrznikova

Existing xenon dark matter (DM) direct detection experiments can probe the DM-nucleon interaction of DM with a sub-GeV mass through a search for photon emission from the recoiling xenon atom. We show that LUX's constraints on sub-GeV DM,…

High Energy Physics - Phenomenology · Physics 2017-08-23 Christopher McCabe

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

Low Temperature Detectors (LTDs) offer the best signal-to-noise performance and thus, lowest energy threshold among other particle detection technologies available today. The excellent background rejection provided by these detectors is…

Instrumentation and Methods for Astrophysics · Physics 2013-08-02 Nader Mirabolfathi

Axion Dark Matter eXperiment (ADMX) ultra low noise haloscope technology has enabled the successful completion of two science runs (1A and 1B) that looked for dark matter axions in the $2.66$ to $3.1$ $\mu$eV mass range with…

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…

An ongoing challenge in dark matter direct detection is to improve the sensitivity to light dark matter in the MeV--GeV mass range. One proposal is to dope a liquid noble-element direct detection experiment with a lighter element such as…

High Energy Physics - Phenomenology · Physics 2024-05-10 Nicole F. Bell , Peter Cox , Matthew J. Dolan , Jayden L. Newstead , Alexander C. Ritter

To reach ultra-low detection thresholds necessary to probe unprecedentedly low Dark Matter masses, target material alternatives and novel detector designs are essential. One such target material is superfluid $^4$He which has the potential…

We propose a new method to detect low-energy neutrinos and low-mass dark matter at or below the MeV scale, through their coherent scatterings from freely falling heavy atoms and the resulting kinematic shifts. We start with a simple…

High Energy Physics - Phenomenology · Physics 2023-03-07 Alim Ruzi , Sitian Qian , Tianyi Yang , Qiang Li

By extracting the beam with a bent crystal or by using an internal gas target, the multi-TeV proton and lead LHC beams allow one to perform the most energetic fixed-target experiments ever and to study $pp$, $p$d and $p$A collisions at…