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An experiment is described to detect dark matter axions trapped in the halo of our galaxy. Galactic axions are converted into microwave photons via the Primakoff effect in a static background field provided by a superconducting magnet. The…

Axions solve the Strong CP Problem and are a cold dark matter candidate. The combined constraints from accelerator searches, stellar evolution limits and cosmology suggest that the axion mass is in the range $3 \cdot 10^{-3} > m_a >…

High Energy Physics - Phenomenology · Physics 2007-05-23 Pierre Sikivie

We propose an experimental scheme to search for galactic halo axions with mass $m_a \sim 10^{-3}$eV, which is above the range accessible with cavity techniques. The detector consists of a large number of parallel superconducting wires…

High Energy Physics - Phenomenology · Physics 2009-12-30 Pierre Sikivie , D. B. Tanner , Yun Wang

Axions, if discovered, could serve as a powerful new messenger for studying astrophysical objects. In this study we show how the Sun's spatial and spectral "axion image" can be inverted to infer the radial dependence of solar properties in…

High Energy Physics - Phenomenology · Physics 2023-10-09 Sebastian Hoof , Joerg Jaeckel , Lennert J. Thormaehlen

We provide the first investigation of the solar production of symmetrons, a well-motivated class of screened scalar fields with density dependent couplings to the Standard Model, and their subsequent absorption in underground direct…

High Energy Physics - Phenomenology · Physics 2026-04-13 Hannah Banks , Anne-Christine Davis , Luca Visinelli

We report new searches for the solar axions and galactic axion-like dark matter particles, using the first low-background data from PandaX-II experiment at China Jinping Underground Laboratory, corresponding to a total exposure of about…

We consider liquid xenon dark matter detectors for searching a light scalar particle produced in the solar core, specifically one that couples to electrons. Through its interaction with the electrons, the scalar particle can be produced in…

High Energy Physics - Phenomenology · Physics 2020-09-01 Ranny Budnik , Oz Davidi , Hyungjin Kim , Gilad Perez , Nadav Priel

A search of axions produced in nuclear transitions was performed at the Kuo-Sheng Nuclear Power Station with a high-purity germanium detector of mass 1.06 kg at a distance of 28 m from the 2.9 GW reactor core. The expected experimental…

High Energy Physics - Experiment · Physics 2008-11-26 H. M. Chang , TEXONO Collaboration

Axions are hypothetical particles that were postulated to solve one of the puzzles arising in the standard model of particle physics, namely the strong CP (Charge conjugation and Parity) problem. The new International AXion Observatory…

Instrumentation and Detectors · Physics 2014-03-05 I. Shilon , A. Dudarev , H. Silva , U. Wagner , H. H. J. ten Kate

A haloscope of the QUAX--$a\gamma$ experiment, composed of an high-Q resonant cavity immersed in a 8 T magnet and cooled to $\sim 4.5$~K is operated to search for galactic axion with mass $m_a\simeq42.8~\mu\text{eV}$. The design of the…

We present a proposal to search for QCD axions with mass in the 200 $\mu$eV range, assuming that they make a dominant component of dark matter. Due to the axion-electron spin coupling, their effect is equivalent to the application of an…

High Energy Physics - Phenomenology · Physics 2017-03-24 R. Barbieri , C. Braggio , G. Carugno , C. S. Gallo , A. Lombardi , A. Ortolan , R. Pengo , G. Ruoso , C. C. Speake

Axion dark matter (DM) is predicted to convert into radio waves in neutron star magnetospheres. We assess the detectability of this signal using a 5 m radio telescope to be installed at the Fan Mountain Observatory, operating in the UHF, L-…

The SUPerconduction AXion search experiment (Supax) is a future haloscope-type detector designed to probe axion-like particles (ALPs) as candidates for dark matter and solutions to the strong-CP problem in the mass range between $8\,\mu$eV…

High Energy Physics - Experiment · Physics 2026-03-12 Tim Schneemann , Hendrik Bekker , Dmitry Budker , Kristof Schmieden , Matthias Schott , Malavika Unni , Arne Wickenbrock

We investigate the 5.49 MeV solar axions flux produced in the $p(d,\, ^{3}{\rm He})a$ reaction and analyze the potential to detect it with the forthcoming large underground neutrino oscillation experiment Jiangmen Underground Neutrino…

High Energy Physics - Phenomenology · Physics 2022-12-14 Giuseppe Lucente , Newton Nath , Francesco Capozzi , Maurizio Giannotti , Alessandro Mirizzi

We report details on the axion dark matter search experiment that uses the innovative technologies of a High-Temperature Superconducting (HTS) magnet and a Josephson Parametric Converter (JPC). An 18 T HTS solenoid magnet is developed for…

High Energy Physics - Experiment · Physics 2022-12-14 Hojin Yoon , Moohyun Ahn , Byeongsu Yang , Youngjae Lee , DongLak Kim , Heejun Park , Byeonghun Min , Jonghee Yoo

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…

Axions and axion-like pseudoscalar particles with dimension-5 couplings to photons exhibit coherent Primakoff scattering with ordered crystals at keV energy scales, making for a natural detection technique in searches for solar axions. We…

High Energy Physics - Phenomenology · Physics 2023-07-13 James B. Dent , Bhaskar Dutta , Adrian Thompson

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…

High Energy Physics - Experiment · Physics 2022-06-20 Youngjae Lee , Byeongsu Yang , Hojin Yoon , Moohyun Ahn , Heejun Park , Byeonghun Min , DongLak Kim , Jonghee Yoo

A calculation of the expected signal due to Primakoff coherent conversion of solar axions into photons via Bragg scattering in several crystal detectors is presented. The results are confronted with the experimental sensitivities of present…