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In the presence of a magnetic field, axions can convert into photons and vice versa. The phenomenology of the conversion is captured by a system of two coupled Klein-Gordon equations, which, assuming that the axion is relativistic, is…

High Energy Physics - Phenomenology · Physics 2025-03-24 Clemente Smarra , Pierluca Carenza

For the first time, we predict the axion spectra and their associated luminosities for several low-mass stars -- one and two solar masses stars in the main sequence and post-main sequence stages of evolution. Equally, we also compute the…

High Energy Astrophysical Phenomena · Physics 2021-08-03 Ilídio Lopes

We propose the use of the Earth as a transducer for ultralight dark-matter detection. In particular we point out a novel signal of kinetically mixed dark-photon dark matter: a monochromatic oscillating magnetic field generated at the…

High Energy Physics - Phenomenology · Physics 2021-10-22 Michael A. Fedderke , Peter W. Graham , Derek F. Jackson Kimball , Saarik Kalia

If axions or axion-like particles exist and are detected, they will not only extend the standard model of particle physics but will also open a new way to probe their sources. Axion helioscopes aim to detect axions which are produced in the…

Solar and Stellar Astrophysics · Physics 2020-01-28 Joerg Jaeckel , Lennert J. Thormaehlen

It is shown that the hypothesis of the axion mechanism of Sun luminosity suggesting that the solar axion particles are born in the core of the Sun and may be efficiently converted back into $\gamma$-quanta in the magnetic field of the solar…

Solar and Stellar Astrophysics · Physics 2014-12-17 V. D. Rusov , K. Kudela , I. V. Sharph , M. V. Eingorn , V. P. Smolyar , D. S. Vlasenko , T. N. Zelentsova , M. E. Beglaryan , E. P. Linnik

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

The possibility of detection of 5.5 MeV and 14.4 keV solar axions by observing axion-induced nuclear and atomic transitions is investigated. The presence of nuclear transitions between spin-orbit partners can be manifested by the subsequent…

High Energy Physics - Phenomenology · Physics 2021-12-14 John D. Vergados , Paraskevi C. Divari , Hiroyasu Ejiri

Light boson dark matter such as axion or hidden photon can be resonantly converted into a magnon in a magnetic insulator under the magnetic field, which can be detected experimentally. We provide a quantum mechanical formulation for the…

High Energy Physics - Phenomenology · Physics 2020-05-21 So Chigusa , Takeo Moroi , Kazunori Nakayama

We present calculations of the reflection of the cosmic X-ray background (CXB) by the Earth's atmosphere in the 1--1000 keV energy range. The calculations include Compton scattering and X-ray fluorescent emission and are based on a…

Astrophysics · Physics 2008-02-11 E. Churazov , S. Sazonov , R. Sunyaev , M. Revnivtsev

We develop a theoretical framework for axion dark matter (DM) searches using terrestrial electromagnetic (EM) fields. Axions couple to the geomagnetic field and generate a monochromatic EM signal at a frequency set by the axion mass.…

High Energy Physics - Phenomenology · Physics 2025-09-19 Atsushi Taruya , Atsushi Nishizawa , Yoshiaki Himemoto

A search for the axioelectric absorption of 5.5-MeV solar axions produced in the $p+d\rightarrow \rm{^3He}+\gamma(5.5 \rm{MeV})$ reaction was performed with two BGO detectors placed inside a low-background setup. A model independent limit…

High Energy Physics - Experiment · Physics 2014-11-21 A. V. Derbin , A. S. Kayunov , V. N. Muratova

In this letter we describe our novel photon regeneration experiment for the axionlike particle search using a x-ray beam with a photon energy of 50.2 keV and 90.7 keV, two superconducting magnets of 3 T, and a Ge detector with a high…

High Energy Physics - Experiment · Physics 2010-12-28 Remy Battesti , Mathilde Fouché , C. Detlefs , T. Roth , Paul Berceau , F. Duc , P. Frings , G. L. J. A. Rikken , Carlo Rizzo

It has recently been observed that solar spicules covering almost of all solar surface have strong magnetic field $B\sim 10^2$G. They are supposed to be plasma jets emitted from chromosphere and they arrive up to $\sim 10^4$km. Their…

High Energy Physics - Phenomenology · Physics 2023-05-17 Aiichi Iwazaki

We have proposed a method for the detection of dark matter axion. It uses superconductor under strong magnetic field. As is well known, the dark matter axion induces oscillating electric field under magnetic field. The electric field is…

High Energy Physics - Phenomenology · Physics 2021-02-03 Aiichi Iwazaki

Axions may be produced in abundance inside stellar cores and then convert into observable X-rays in the Galactic magnetic fields. We focus on the Quintuplet and Westerlund 1 super star clusters, which host large numbers of hot, young stars…

High Energy Physics - Phenomenology · Physics 2021-03-03 Christopher Dessert , Joshua W. Foster , Benjamin R. Safdi

We show that a stable vortex soliton, carrying a constant magnetic flux, exists in the homogeneous medium of axions with a constant time-derivative. Axions can be bound in the vortex, having energy less than the axion mass. If the observed…

High Energy Physics - Phenomenology · Physics 2024-04-02 Deog Ki Hong , Stephen J. Lonsdale

BabyIAXO is the intermediate stage of the International Axion Observatory (IAXO) to be hosted at DESY. Its primary goal is the detection of solar axions following the axion helioscope technique. Axions are converted into photons in a large…

High Energy Physics - Experiment · Physics 2024-12-02 S. Ahyoune , K. Altenmueller , I. Antolin , S. Basso , P. Brun , F. R. Candon , J. F. Castel , S. Cebrian , D. Chouhan , R. Della Ceca , M. Cervera-Cortes , V. Chernov , M. M. Civitani , C. Cogollos , E. Costa , V. Cotroneo , T. Dafni , A. Derbin , K. Desch , M. C. Diaz-Martin , A. Diaz-Morcillo , D. Diez-Ibanez , C. Diez Pardos , M. Dinter , B. Doebrich , I. Drachnev , A. Dudarev , A. Ezquerro , S. Fabiani , E. Ferrer-Ribas , F. Finelli , I. Fleck , J. Galan , G. Galanti , M. Galaverni , J. A. Garcia , J. M. Garcia-Barcelo , L. Gastaldo , M. Giannotti , A. Giganon , C. Goblin , N. Goyal , Y. Gu , L. Hagge , L. Helary , D. Hengstler , D. Heuchel , S. Hoof , R. Iglesias-Marzoa , F. J. Iguaz , C. Iniguez , I. G. Irastorza , K. Jakovcic , D. Kaefer , J. Kaminski , S. Karstensen , M. Law , A. Lindner , M. Loidl , C. Loiseau , G. Lopez-Alegre , A. Lozano-Guerrero , B. Lubsandorzhiev , G. Luzon , I. Manthos , C. Margalejo , A. Marin-Franch , J. Marques , F. Marutzky , C. Menneglier , M. Mentink , S. Mertens , J. Miralda-Escude , H. Mirallas , F. Muleri , V. Muratova , J. R. Navarro-Madrid , X. F. Navick , K. Nikolopoulos , A. Notari , A. Nozik , L. Obis , A. Ortiz-de-Solorzano , T. O'Shea , J. von Oy , G. Pareschi , T. Papaevangelou , K. Perez , O. Perez , E. Picatoste , M. J. Pivovaroff , J. Porron , M. J. Puyuelo , A. Quintana , J. Redondo , D. Reuther , A. Ringwald , M. Rodrigues , A. Rubini , S. Rueda-Teruel , F. Rueda-Teruel , E. Ruiz-Choliz , J. Ruz , J. Schaffran , T. Schiffer , S. Schmidt , U. Schneekloth , L. Schoenfeld , M. Schott , L. Segui , U. R. Singh , P. Soffitta , D. Spiga , M. Stern , O. Straniero , F. Tavecchio , E. Unzhakov , N. A. Ushakov , G. Vecchi , J. K. Vogel , D. M. Voronin , R. Ward , A. Weltman , C. Wiesinger , R. Wolf , A. Yanes-Diaz , Y. Yu

We discuss axion dark matter detection via two mechanisms: spontaneous decays and resonant conversion in neutron star magnetospheres. For decays, we show that the brightness temperature signal, rather than flux, is a less ambiguous measure…

Cosmology and Nongalactic Astrophysics · Physics 2020-07-15 Richard A. Battye , Bjoern Garbrecht , Jamie I. McDonald , Francesco Pace , Sankarshana Srinivasan

Ground-based radio telescopes are routinely used to search for light dark matter (DM) candidates such as axion-like particles or dark photons. These instruments face however inherent limitations to push the searches to masses below…

High Energy Physics - Phenomenology · Physics 2026-05-19 Ruben Zatini , Francesca Calore , Pasquale Dario Serpico
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