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Related papers: A High Resolution Search for Dark-Matter Axions

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The microwave cavity experiment is the most sensitive way of looking for axions in the 0.1-10 GHz range, corresponding to masses of 0.5 - 40 $\mu$eV. The particular challenge for frequencies greater than 5 GHz is designing a cavity with a…

Instrumentation and Methods for Astrophysics · Physics 2021-03-11 Maria Simanovskaia , Alex Droster , Heather Jackson , Isabella Urdinaran , Karl van Bibber

Dark matter Axion search with riNg Cavity Experiment (DANCE) was proposed. To search for axion-like particles, we aim to detect the rotation and oscillation of optical linear polarization caused by axion-photon coupling with a bow-tie…

High Energy Physics - Phenomenology · Physics 2021-05-18 Yuka Oshima , Hiroki Fujimoto , Masaki Ando , Tomohiro Fujita , Yuta Michimura , Koji Nagano , Ippei Obata , Taihei Watanabe

A search for dark matter axions with masses $>10 \mu eV/c^{2}$ has been performed using the HAYSTAC experiment's squeezed state receiver to achieve sub-quantum limited noise. This report includes details of the design and operation of the…

The axion is a compelling hypothetical particle that could account for the dark matter in our universe, while simultaneously explaining why quark interactions within the neutron do not appear to give rise to an electric dipole moment. The…

High Energy Physics - Experiment · Physics 2025-12-11 Andrew Engel , Thomas Braine , Christian Boutan

The axion is a promising dark matter candidate, which was originally proposed to solve the strong-CP problem in particle physics. To date, the available parameter space for axion and axion-like particle dark matter is relatively unexplored,…

We discuss the sensitivity of the present and near-future axion dark matter experiments to a halo of axions or axion-like particles gravitationally bound to the Earth or the Sun. The existence of such halos, assuming they are formed,…

High Energy Physics - Phenomenology · Physics 2021-01-28 Abhishek Banerjee , Dmitry Budker , Joshua Eby , Victor V. Flambaum , Hyungjin Kim , Oleksii Matsedonskyi , Gilad Perez

The recently published GALFA-HI Compact Cloud Catalogue lists 20 neutral hydrogen clouds that might pinpoint previously undiscovered high-latitude dwarf galaxies. Detection of an associated gamma-ray dark matter signal could provide a route…

High Energy Astrophysical Phenomena · Physics 2015-06-15 N. Mirabal

Axions and axion-like particles are well-motivated dark matter candidates. We propose an experiment that uses single photon detection interferometry to search for axions and axion-like particles in the galactic halo. We show that photon…

Instrumentation and Detectors · Physics 2025-09-23 Haocun Yu , Ohkyung Kwon , Hartmut Grote , Denis Martynov

We performed the deepest search for an X-ray emission line between 0.5 and 7 keV from non-baryonic dark matter with the Suzaku XIS. Dark matter associated with the Milky Way galaxy was selected as the target to obtain the best…

High Energy Astrophysical Phenomena · Physics 2015-09-23 Norio Sekiya , Noriko Y. Yamasaki , Kazuhisa Mitsuda

We present systematic case studies to investigate the sensitivity of axion searches by liquid xenon detectors, using the axio-electric effect (analogue of the photoelectric effect) on xenon atoms. Liquid xenon is widely considered to be one…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-11 K. Arisaka , P. Beltrame , C. Ghag , J. Kaidi , K. Lung , A. Lyashenko , R. D. Peccei , P. Smith , K. Ye

A ferromagnetic axion haloscope searches for Dark Matter in the form of axions by exploiting their interaction with electronic spins. It is composed of an axion-to-electromagnetic field transducer coupled to a sensitive rf detector. The…

The axion is arguably one of the best motivated candidates for dark matter. For a decay constant greater than about 10^9 GeV, axions are dominantly produced non-thermally in the early universe and hence are "cold", their velocity dispersion…

High Energy Physics - Phenomenology · Physics 2016-12-30 Andreas Ringwald

The velocity distribution of cold dark matter within galaxies is expected to exhibit ultra-fine-grained substructure as a result of the many foldings of an initially smooth phase-space sheet under gravity. The innumerable folds of this…

High Energy Physics - Phenomenology · Physics 2025-09-19 Ciaran A. J. O'Hare , Giovanni Pierobon

We report first results from RadioAxion, an underground experiment searching for axion dark matter through periodic modulations of radioisotope decays. We monitor the $\alpha$ decay of ${^{241}}$Am via its $59.5$ keV $\gamma$ line using a…

High Energy Physics - Experiment · Physics 2026-05-25 Carlo Broggini , Giuseppe Di Carlo , Luca Di Luzio , Denise Piatti , Claudio Toni

Weakly interactive slim particles (WISPs), including the QCD axion, axion-like particles (ALPs), and hidden photons, are considered to be strong candidates for the dark matter carrier particle. The microwave cavity experiment WISPDMX is the…

Instrumentation and Detectors · Physics 2015-11-11 Le Hoang Nguyen , Dieter Horns , Andrei Lobanov , Andreas Ringwald

We report on a search for dark matter axion-like particles (ALPs) using a Ramsey-type apparatus for cold neutrons. A hypothetical ALP-gluon-coupling would manifest in a neutron electric dipole moment signal oscillating in time. Twenty-four…

Axion physics is briefly reviewed. Constraints from laboratory searches, astrophysics and cosmology require the axion mass to be in the range $10^{-6} \lesssim m_a < 3\cdot 10^{-3}$eV. Near the lower end of this range, axions are all or a…

High Energy Physics - Phenomenology · Physics 2017-08-23 P. Sikivie

RADES (Relic Axion Detector Exploratory Setup) is a project with the goal of directly searching for axion dark matter above the $30 \mu$eV scale employing custom-made microwave filters in magnetic dipole fields. Currently RADES is taking…

We propose a new strategy to search for dark matter axions in the mass range of 40--400 $\mu$eV by introducing dielectric haloscopes, which consist of dielectric disks placed in a magnetic field. The changing dielectric media cause…