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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 introduce a new experimental method for solar hadronic axions search. It is suggested that these axions are created in the Sun during M1 transition between the first thermally excited level at 9.4 keV and the ground state in $^{83}Kr$.…

Nuclear Experiment · Physics 2009-12-08 K. Jakovcic , Z. Krecak , M. Krcmar , A. Ljubicic

Dark Matter searches have been ongoing for three decades; the lack of a positive discovery of the main candidate, the WIMP, after dedicated efforts, has put axions and axion-like-particles in the spotlight. The three main techniques…

Instrumentation and Methods for Astrophysics · Physics 2022-04-08 T. Dafni , J. Galan

We present a method to determine the sensitivity of a closed dielectric haloscope to axion dark matter. Dielectric haloscopes aim to probe the theoretically well-motivated axion mass range of ~26 $\mathrm{\mu}$eV to ~500 $\mathrm{\mu}$eV by…

Axions are a natural consequence of the Peccei-Quinn mechanism, the most compelling solution to the strong-CP problem. Similar axion-like particles (ALPs) also appear in a number of possible extensions of the Standard Model, notably in…

Instrumentation and Detectors · Physics 2020-12-15 Javier Galan

The CAST (CERN Axion Solar Telescope) experiment is searching for axions, an hypothetical particle that emerges as a possible solution to the well known CP violation problem in strong interactions. CAST is using a decommissioned LHC dipole…

Instrumentation and Methods for Astrophysics · Physics 2015-03-18 J. Galan

We report an axion dark matter search with a haloscope equipped with a microwave photon counter. The haloscope is a tunable high quality factor 3-dimensional microwave cavity placed in a magnetic field. The photon counter, operated…

Axions are a well-motivated dark matter candidate, with a host of experiments around the world searching for direct evidence of their existence. The ORGAN Experiment is a type of axion detector known as an axion haloscope, which takes the…

High Energy Physics - Phenomenology · Physics 2023-06-08 Ben T. McAllister , Aaron Quiskamp , Ciaran O'Hare , Paul Altin , Eugene Ivanov , Maxim Goryachev , Michael Tobar

GPS, an excellent tool for geodesy, may serve also particle physics. In the presence of Earth's magnetic field, a GPS photon may be transformed into an axion. The proposed experimental setup involves the transmission of a GPS signal from a…

High Energy Physics - Phenomenology · Physics 2017-10-11 A. Nicolaidis

We report on a scheme for highly efficient detection of single microwave photons, with application to detecting certain exotic particles such as the axion. This scheme utilises an experiment known as the micromaser and the phenomenon of…

Instrumentation and Detectors · Physics 2007-05-23 M. L. Jones , G. J. Wilkes , B. T. H. Varcoe

The possibility of axion detection by observing axion induced atomic excitations as suggested by Sikivie is discussed. The atom is cooled at low temperature and it is chosen to posses three levels. The first is the ground state, the second…

High Energy Physics - Phenomenology · Physics 2022-12-08 J. D. Vergados , F. T. Avignone , S. Cohen , R. J. Creswick

The invisible axion is a hypothetical particle that arises from the Peccei-Quinn mechanism proposed to resolve the CP problem in quantum chromodynamics, and is considered one of the most favoured candidates for cold dark matter. Dish…

High Energy Physics - Phenomenology · Physics 2023-09-06 Junu Jeong , Sungwoo Youn , Yannis K. Semertzidis

We have searched for solar hidden photons in the eV energy range using a dedicated hidden photon detector. The detector consisted of a parabolic mirror with a diameter of 500mm and a focal length of 1007mm installed in a vacuum chamber, and…

Solar and Stellar Astrophysics · Physics 2013-07-11 T. Mizumoto , R. Ohta , T. Horie , J. Suzuki , Y. Inoue , M. Minowa

It is known that magnetic fields exist near black holes and photons can go around black holes due to strong gravity. Utilizing these facts, we can probe hypothetical pseudoscalar particles, so-called axions. In fact, photons can be…

High Energy Physics - Phenomenology · Physics 2023-06-12 Kimihiro Nomura , Kaishu Saito , Jiro Soda

Massive axions of the Kaluza-Klein type, created inside the solar core, can be gravitationally trapped by the Sun itself in orbits inside/outside the Sun, where they accumulate over cosmic times. Their radiative decay can give rise to…

Astrophysics · Physics 2007-05-23 K. Zioutas

Axion helioscopes aim at the detection of solar axions through their conversion into x-rays in laboratory magnetic fields. The use of low background x-ray detectors is an essential component contributing to the sensitivity of these…

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

Axion-like particles (ALPs), hypothetical extensions of the Standard Model, can convert into photons in an external magnetic field. Two recent studies~\cite{Todarello:2023ptf, Ruz:2024gkl} explored the phenomenology of ALP-photon conversion…

High Energy Physics - Phenomenology · Physics 2025-01-28 Elisa Todarello

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
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