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If dark matter is composed of weakly interacting particles, Earth's orbital motion may induce a small annual variation in the rate at which these particles interact in a terrestrial detector. The DAMA collaboration has identified at a…

High Energy Physics - Phenomenology · Physics 2018-11-29 Chris Kelso , Christopher Savage , Pearl Sandick , Katherine Freese , Paolo Gondolo

Weakly Interacting Massive Particles (WIMPs) are well-established dark matter candidates. WIMP interactions with sensitive detectors are expected to display a characteristic annual modulation in rate. We release a dataset spanning 3.4 years…

The existence of dark sectors, consisting of weakly-coupled particles that do not interact with the known Standard Model forces, is theoretically and phenomenologically motivated. The hidden particles are candidates for Dark Matter and can…

High Energy Physics - Phenomenology · Physics 2020-06-17 D. T. Binh , V. H. Binh , H. N. Long

A well-studied possibility is that dark matter may reside in a sector secluded from the Standard Model, except for the so-called photon portal: kinetic mixing between the ordinary and dark photons. Such interactions can be probed at dark…

High Energy Physics - Phenomenology · Physics 2017-07-26 Timon Emken , Chris Kouvaris , Ian M. Shoemaker

Mirror and more generic hidden sector dark matter models can simultaneously explain the DAMA, CoGeNT and CRESST dark matter signals consistently with the null results of the other experiments. This type of dark matter can be captured by the…

High Energy Physics - Phenomenology · Physics 2015-05-30 R. Foot

This report presents an overview of the unconventional use of charge-coupled devices (CCDs) to search for Dark Matter (DM). The DArk Matter In CCDs (DAMIC Experiment) employs the bulk silicon of thick, fully-depleted CCDs as a target for…

Instrumentation and Detectors · Physics 2020-01-14 N. Castello-Mor , DAMIC-M Collaboration

The DAMIC-M (DArk Matter In CCDs at Modane) experiment will use skipper CCDs to search for low mass (sub-GeV) dark matter underground at the Laboratoire Souterrain de Modane (LSM) in France. With about 1 kg of silicon target mass and…

High Energy Physics - Experiment · Physics 2024-10-01 R. Smida

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

We derive constraints on the annual modulation signal in Dark Matter (DM) direct detection experiments in terms of the unmodulated event rate. A general bound independent of the details of DM distribution follows from the assumption that…

High Energy Physics - Phenomenology · Physics 2015-06-03 Juan Herrero-Garcia , Thomas Schwetz , Jure Zupan

Dark matter in the form of particles from a hidden mirror sector has recently been proposed as an explanation for the DAMA annual modulation signal. Here one assumes that there exists a small mixing between photons and mirror photons. We…

Astrophysics · Physics 2007-05-23 Saibal Mitra

A search for dark matter was conducted by looking for an annual modulation signal due to the Earth's rotation around the Sun using XMASS, a single phase liquid xenon detector. The data used for this analysis was 359.2 live days times 832 kg…

We calculate the diurnal and annual modulation of the signals in axion and WIMP dark matter detectors on Earth caused by a cold flow of dark matter in the Solar neighborhood. The effects of the Sun's and the Earth's gravity, and of the…

Astrophysics · Physics 2009-11-10 Fu-Sin Ling , Pierre Sikivie , Stuart Wick

Recently, the DAMA/LIBRA collaboration released updated results from their search for the annual modulation signal from Dark Matter (DM) scattering in the detector. Besides approximately doubling the exposure of the DAMA/LIBRA data set, the…

Cosmology and Nongalactic Astrophysics · Physics 2019-01-03 Sebastian Baum , Katherine Freese , Chris Kelso

Direction sensitive direct detection of Weakly Interacting Massive Particles (WIMPs) as dark matter would provide an unambiguous non-gravitational signature of dark matter (DM). The diurnal variation of DM signal due to earth's rotation…

High Energy Physics - Phenomenology · Physics 2012-04-16 Abhijit Bandyopadhyay , Debasish Majumdar

The aim of the current work is a detailed time-series analysis of the data from Dark Matter direct detection experiments as well as related datasets. We examine recent claims that the cosmic ray muon flux can be responsible for generating…

High Energy Physics - Phenomenology · Physics 2015-03-19 Spencer Chang , Josef Pradler , Itay Yavin

We investigate the diurnal modulation of the event rate for dark matter scattering on solid targets arising from the directionally dependent defect creation threshold energy. In particular, we quantify how this effect would help in…

High Energy Physics - Phenomenology · Physics 2021-09-29 Sebastian Sassi , Abolfazl Dinmohammadi , Matti Heikinheimo , Nader Mirabolfathi , Kai Nordlund , Hossein Safari , Kimmo Tuominen

We study the effect of gravitational focusing of the earth on dark matter. We find that the effect can produce a detectable diurnal modulation in the dark matter signal for part of the parameter space which for high dark matter masses is…

High Energy Physics - Phenomenology · Physics 2015-11-06 Chris Kouvaris , Niklas Grønlund Nielsen

An annual modulation signal due to the Earth orbiting around the Sun would be one of the strongest indications of the direct detection of dark matter. In 2016, we reported a search for dark matter by looking for this annual modulation with…

The DAMIC experiment employs large-area, thick charge-coupled devices (CCDs) to search for the interactions of low-mass dark matter particles in the galactic halo with silicon atoms in the CCD target. From 2017 to 2019, DAMIC collected data…

Cosmology and Nongalactic Astrophysics · Physics 2022-10-04 Alvaro E. Chavarria