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Driven by the null results in the searches for dark matter, the field of direct dark matter detection is constantly evolving to push new frontiers. Ultimately, a vast parameter space for dark matter masses below a few GeV is yet to be…

High Energy Physics - Experiment · Physics 2025-12-18 Melih Solmaz

We report on recent progress in the search for dark matter particles with masses from 1 MeV to 1 GeV. Several dark matter candidates in this mass range are expected to generate measurable electronic-recoil signals in direct-detection…

Cosmology and Nongalactic Astrophysics · Physics 2023-01-02 Alvaro E. Chavarria

At a level too faint for astronomy, particle dark matter may interact with Standard Model states via the photon. We derive limits from direct detection experiments on photon-mediated nuclear interactions up to operator dimension-6, viz.,…

High Energy Physics - Phenomenology · Physics 2025-09-30 Jason Kumar , Biprajit Mondal , Girish Muralidhara , Nirmal Raj

The EDELWEISS collaboration reports on the search for Dark Matter (DM) particle interactions via Migdal effect with masses between $32$ MeV$\cdot$c$^{-2}$ to $2$ GeV$\cdot$c$^{-2}$ using a $200$ g cryogenic Ge detector sensitive to…

The FASER experiment at the LHC is designed to search for light, weakly-interacting particles produced in proton-proton collisions at the ATLAS interaction point that travel in the far-forward direction. The first results from a search for…

High Energy Physics - Experiment · Physics 2023-12-27 FASER Collaboration

Direct dark matter detection experiments search for rare signals induced by hypothetical, galactic dark matter particles in low-background detectors operated deep underground. I will briefly review the direct detection principles, the…

Instrumentation and Methods for Astrophysics · Physics 2025-12-30 Laura Baudis

In the past decades, several detector technologies have been developed with the quest to directly detect dark matter interactions and to test one of the most important unsolved questions in modern physics. The sensitivity of these…

Instrumentation and Detectors · Physics 2017-04-04 Teresa Marrodan Undagoitia , Ludwig Rauch

Dark matter is five times more abundant than ordinary visible matter in our Universe. While laboratory searches hunting for dark matter have traditionally focused on the electroweak scale, theories of low mass hidden sectors motivate new…

High Energy Physics - Experiment · Physics 2023-02-08 S. A. Lyon , Kyle Castoria , Ethan Kleinbaum , Zhihao Qin , Arun Persaud , Thomas Schenkel , Kathryn Zurek

The EDELWEISS collaboration has performed a search for dark matter particles with masses below the GeV-scale with a 33.4-g germanium cryogenic detector operated in a surface lab. The energy deposits were measured using a…

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…

At Argonne National Laboratory, we are developing hard X-ray (2 to 20 keV) Transition Edge Sensor (TES) arrays for beamline science. The significantly improved energy resolution provided by superconducting detectors compared to…

Instrumentation and Detectors · Physics 2021-06-02 T. Guruswamy , L. Gades , A. Miceli , U. Patel , O. Quaranta

The main goal of the CRESST-III experiment is the direct detection of dark matter particles via their scattering off target nuclei in cryogenic detectors. In this work we present the results of a Silicon-On-Sapphire (SOS) detector with a…

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

Future far-infrared astronomy missions will need large arrays of detectors with exceptionally low noise-equivalent power (NEP), with some mission concepts calling for thousands of detectors with NEPs below a few $\times 10^{-20}$…

Instrumentation and Methods for Astrophysics · Physics 2020-12-14 Peter C. Nagler , John E. Sadleir , Edward J. Wollack

We present new observational constraints on the elastic scattering of dark matter with electrons for dark matter masses between 10 keV and 1 TeV. We consider scenarios in which the momentum-transfer cross section has a power-law dependence…

Cosmology and Nongalactic Astrophysics · Physics 2021-12-01 David Nguyen , Dimple Sarnaaik , Kimberly K. Boddy , Ethan O. Nadler , Vera Gluscevic

We perform the first high-throughput search and evaluation of materials that can serve as excellent low-mass dark matter detectors. Using properties of close to one thousand materials from the Materials Project database, we project the…

High Energy Physics - Phenomenology · Physics 2025-06-26 Sinéad M. Griffin , Yonit Hochberg , Benjamin V. Lehmann , Rotem Ovadia , Kristin A. Persson , Bethany A. Suter , Ruo Xi Yang , Wayne Zhao

The dark photon is a new gauge boson that naturally arises in many beyond the Standard Model theoretical models, featuring interactions that resemble quantum electrodynamics. Due to this feature, it is often considered the portal between…

High Energy Physics - Phenomenology · Physics 2026-03-03 L. Angel , G. Casse , G. Gambini , A. S. de Jesus , V. Kozhuharov , A. Machado , F. S. Queiroz , E. Segreto , J. Smirnov

A search is conducted for new physics in final states containing a photon and missing transverse momentum in proton-proton collisions at $\sqrt{s} =$ 13 TeV, using the data collected in 2016 by the CMS experiment at the LHC, corresponding…

High Energy Physics - Experiment · Physics 2019-03-05 CMS Collaboration

In this letter, we present the performance of a $100~\mu\mathrm{m}\times 400~\mu\mathrm{m} \times 40~\mathrm{nm}$ tungsten (W) Transition-Edge Sensor (TES) with a critical temperature of 40 mK. This device has a measured noise equivalent…

Transition Edge Sensor (TES) spectrometers for hard X-ray beamline science will enable improved X-ray emission and absorption spectroscopy in the information-rich 2 to 20 keV energy range. We are building a TES-based instrument for the…

Instrumentation and Detectors · Physics 2020-08-26 Tejas Guruswamy , Lisa M. Gades , Antonino Miceli , Umeshkumar M. Patel , John T. Weizeorick , Orlando Quaranta