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The hunt for dark matter remains one of the principal objectives of modern physics and cosmology. Searches for dark matter in the form of axions are proposed or underway across a range of experimental collaborations. As we look to the next…

高能物理 - 唯象学 · 物理学 2022-05-04 J. I. McDonald

We propose a new method for detecting dark matter axions using a resonant cavity coupled with a quantum Hall system. When a small sample exhibiting quantum Hall effect is placed inside the cavity and the cavity is tuned to resonance,…

高能物理 - 唯象学 · 物理学 2026-04-24 Aiichi Iwazaki

Metamaterials based on regular two-dimensional arrays of thin wires have attracted renewed attention in light of a recently proposed strategy to search for dark matter axions. When placed in the external magnetic field, such metamaterials…

We report the results of an axion dark matter search over an axion mass range of 9.39-9.51 ${\mu}$eV. A flux-driven Josephson parametric amplifier (JPA) was added to the cryogenic receiver chain. A system noise temperature of as low as 200…

We describe a novel search strategy for axions (or hadronically coupled axion-like particles) in the mass range of $m_a \lesssim 350\,{\rm MeV}$. The search relies on kaon decay at rest, which produces a mono-energetic signal in a large…

高能物理 - 唯象学 · 物理学 2024-09-04 Yohei Ema , Zhen Liu , Ryan Plestid

Experiments aimed at detecting ultralight dark matter typically rely on resonant effects, which are sensitive to the dark matter mass that matches the resonance frequency. In this study, we investigate the nucleon couplings of ultralight…

高能物理 - 唯象学 · 物理学 2024-07-12 Zitong Xu , Xiaolin Ma , Kai Wei , Yuxuan He , Xing Heng , Xiaofei Huang , Tengyu Ai , Jian Liao , Wei Ji , Jia Liu , Xiao-Ping Wang , Dmitry Budker

In dark matter axion searches, quantum uncertainty manifests as a fundamental noise source, limiting the measurement of the quadrature observables used for detection. We use vacuum squeezing to circumvent the quantum limit in a search for a…

The ADAMOS (Axion Daily Modulation Searches) project aims to explore the nature of dark matter (DM) through a novel axion haloscope experiment. We propose to construct a fixed-frequency cavity resonator operating at 20 GHz at the University…

高能物理 - 实验 · 物理学 2026-03-20 Marios Maroudas , Toma-Stefan Cezar , Antonios Gardikiotis , Dieter Horns

A resonantly-enhanced photon-regeneration experiment to search for the axion or axion-like particles is described. This experiment is a shining light through walls study, where photons travelling through a strong magnetic field are (in…

高能物理 - 唯象学 · 物理学 2009-10-29 Guido Mueller , Pierre Sikivie , D. B. Tanner , Karl van Bibber

It is demonstrated that detection of putative particles such as paraphotons and axions constituting the dark sector of the universe can be reduced to detection of extremely weak links or couplings between cavities and modes. This method…

高能物理 - 实验 · 物理学 2019-01-09 Maxim Goryachev , Ben McAllister , Michael E. Tobar

We report the first search results for axion dark matter using an 18\,T high-temperature superconducting magnet haloscope. The scan frequency ranges from 4.7789 to 4.8094\,GHz. No significant signal consistent with the Galactic halo dark…

高能物理 - 实验 · 物理学 2022-06-20 Youngjae Lee , Byeongsu Yang , Hojin Yoon , Moohyun Ahn , Heejun Park , Byeonghun Min , DongLak Kim , Jonghee Yoo

Non-virialized dark-matter axions may be present in the Milky Way halo in the form of low-velocity-dispersion flows. The Axion Dark Matter eXperiment performed a search for the conversion of these axions into microwave photons using a…

There are a number of theoretical predictions for astrophysical and cosmological objects, which emit high frequency ($10^6-10^9$~Hz) Gravitation Waves (GW) or contribute somehow to the stochastic high frequency GW background. Here we…

广义相对论与量子宇宙学 · 物理学 2025-06-18 Maxim Goryachev , Michael E. Tobar

The realization and characterization of a high quality factor resonator composed of two hollow-dielectric cylinders with its pseudo-TM$_{030}$ mode resonating at 10.9 GHz frequency is discussed. The quality factor was measured at the…

We study the underlying theory of dielectric haloscopes, a new way to detect dark matter axions. When an interface between different dielectric media is inside a magnetic field, the oscillating axion field acts as a source of…

高能物理 - 唯象学 · 物理学 2017-02-01 Alexander J. Millar , Georg G. Raffelt , Javier Redondo , Frank D. Steffen

Axions are hypothetical particles that provide a compelling solution to two major mysteries in modern physics: the strong CP problem and the nature of dark matter. The plasma haloscope has been proposed as a promising approach for probing…

We report the results of Phase 1b of The ORGAN Experiment, a microwave cavity haloscope searching for dark matter axions in the $107.42-111.93~\mu$eV mass range. The search excludes axions with two-photon coupling $g_{a\gamma\gamma}\geq…

高能物理 - 实验 · 物理学 2025-04-11 Aaron Quiskamp , Ben T. McAllister , Paul Altin , Eugene N. Ivanov , Maxim Goryachev , Michael E. Tobar

In the space-based gravitational wave detections, the axion-like dark matter would alter the polarization state of the laser link between spacecrafts due to the birefringence effect. However, current designs of space-based laser…

广义相对论与量子宇宙学 · 物理学 2026-04-08 Yong-Yong Liu , Jing-Rui Zhang , Ming-Hui Du , He-Shan Liu , Peng Xu , Yun-Long Zhang

Dark matter makes up 85% of the matter in the universe and 27% of its energy density, but we do not know what comprises dark matter. It is possible that dark matter may be composed of either axions or dark photons, both of which can be…

高能物理 - 实验 · 物理学 2022-11-10 R. Cervantes , G. Carosi , C. Hanretty , S. Kimes , B. H. LaRoque , G. Leum , P. Mohapatra , N. S. Oblath , R. Ottens , Y. Park , G. Rybka , J. Sinnis , J. Yang

We investigate the prospect of an alternative laboratory-based search for the coupling of axions and axion-like particles to photons. Here, the collision of two laser beams resonantly produces axions, and a signal photon is detected after…

高能物理 - 唯象学 · 物理学 2020-05-18 K. A. Beyer , G. Marocco , R. Bingham , G. Gregori