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Related papers: The DAMIC-M Experiment: Status and First Results

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The DAMIC-M collaboration recently reported impressive bounds on sub-GeV dark matter, robustly testing both thermal and non-thermal models for the very first time. In this work we derive novel bounds from the recent PandaX-4T ionization…

High Energy Physics - Phenomenology · Physics 2025-07-23 Andrew Cheek , Pablo Figueroa , Gonzalo Herrera , Ian M. Shoemaker

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…

Direct detection experiments aimed at uncovering the elusive nature of dark matter (DM) have made significant progress in probing ever lower cross-sections for DM-nucleon interactions. At the same time, an upper limit in the cross-section…

A complete dedicated electronics, from front-end to back-end, was developed to instrument a MIMAC prototype. A front end ASIC able to monitor 64 strips of pixels and to provide their individual "Time Over Threshold" information has been…

Instrumentation and Methods for Astrophysics · Physics 2012-02-20 O. Bourrion , G. Bosson , C. Grignon , J. P. Richer , O. Guillaudin , F. Mayet , J. Billard , D. Santos

We improve limits on the spin-independent scattering cross section of Dark Matter on nucleons, for DM in the 300 MeV -- 100 GeV mass range, based on the DAMIC and XQC experiments. Our results close the window which previously existed in…

High Energy Physics - Phenomenology · Physics 2017-12-22 M. Shafi Mahdawi , Glennys R. Farrar

Models for light dark matter particles with masses below 1 GeV/c$^2$ are a natural and well-motivated alternative to so-far unobserved weakly interacting massive particles. Gram-scale cryogenic calorimeters provide the required detector…

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

The CBM experiment will investigate heavy-ion collisions at beam energies from 8 to 45 AGeV at the future accelerator facility FAIR. The goal of the experiment is to study the QCD phase diagram in the region of moderate temperatures and…

Nuclear Experiment · Physics 2010-02-17 M. Deveaux , S. Amar-Youcef , C. Dritsa , I. Froehlich , C. Muentz , S. Seddiki , J. Stroth , T. Tischler , C. Trageser

DAMPE (Dark Matter Particle Explorer) is a satellite-born experiment launched in 2015 in a sun-synchronous orbit at 500 km altitude, and it has been taking data in stable conditions ever since. Its main goals include the spectral…

High Energy Astrophysical Phenomena · Physics 2022-09-22 Leandro Silveri

With the large progress in searches for dark matter (DM) particles with indirect and direct methods, we develop a numerical tool that enables fast calculations of the likelihoods of specified DM particle models given a number of…

High Energy Physics - Phenomenology · Physics 2017-01-06 Xiaoyuan Huang , Yue-Lin Sming Tsai , Qiang Yuan

A selection of new results from the CMS experiment is presented. These results focus on searches for dark-sector particles using Run 2 or Run 3 data. Dedicated data streams were utilised to explore the low-mass parameter space. Machine…

High Energy Physics - Experiment · Physics 2026-01-16 Kai Hong Law

Dark matter plays a crucial role in our comprehension of the universe, but its mysterious nature poses challenges for direct detection. A primary obstacle in detecting dark matter is distinguishing genuine signals from the prevailing…

High Energy Physics - Experiment · Physics 2025-03-05 M. Mirzakhani , S. Maludze

The cold dark matter (CDM) paradigm provides a remarkably good description of the Universe's large-scale structure. However, some discrepancies exist between its predictions and observations at very small sub-galactic scales. To address…

Cosmology and Nongalactic Astrophysics · Physics 2024-01-04 Atrideb Chatterjee , Sourav Mitra , Amrita Banerjee

Cosmology observations indicate that our universe is composed of 25% dark matter (DM), yet we know little about its microscopic properties. Whereas the gravitational interaction of DM is well understood, its interaction with the Standard…

High Energy Physics - Experiment · Physics 2015-01-05 R. T. Thornton , MiniBooNE-DM collaboration

Recent years have seen dramatic improvements in the sensitivity of electron-based direct detection experiments. Typically, the sensitivity to dark matter scattering is determined in the light and heavy mediator mass limits. In this paper we…

High Energy Physics - Phenomenology · Physics 2026-05-13 Connor Stratman , Tanner Trickle

Collider signatures with top quarks provide sensitive probes of dark matter (DM) production at the Large Hadron Collider (LHC). In this article, we review the results of DM searches in final states with top quarks conducted by the ATLAS and…

High Energy Physics - Experiment · Physics 2023-02-14 J. Katharina Behr , Alexander Grohsjean

In this paper, we introduce a novel program of fixed-target searches for thermal-origin Dark Matter (DM), which couples inelastically to the Standard Model. Since the DM only interacts by transitioning to a heavier state, freeze-out…

High Energy Physics - Phenomenology · Physics 2018-04-05 Eder Izaguirre , Yonatan Kahn , Gordan Krnjaic , Matthew Moschella

Dark Matter (DM) detection prospects at future e+e- colliders are reviewed under the assumption that DM particles are fermions of the Majorana or Dirac type. Although the discussion is quite general, one will keep in mind the recently…

High Energy Physics - Experiment · Physics 2014-11-04 Francois Richard , Giorgio Arcadi , Yann Mambrini

We search for the dark photon dark matter (DPDM) using a cryogenic millimeter-wave receiver. DPDM has a kinetic coupling with electromagnetic fields with a coupling constant of $\chi$, and is converted into ordinary photons at the surface…

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