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Related papers: Towards a new generation axion helioscope

200 papers

Axions are a promising cold dark matter candidate. Haloscopes, which use the conversion of axions to photons in the presence of a magnetic field to detect axions, are the basis of microwave cavity searches such as the Axion Dark Matter…

Cosmology and Nongalactic Astrophysics · Physics 2020-07-01 N. Crisosto , G. Rybka , P. Sikivie , N. S. Sullivan , D. B. Tanner , J. Yang

A new technique has been used to search for solar axions using a single crystal germanium detector. It exploits the coherent conversion of axions into photons when their angle of incidence satisfies a Bragg condition with a crystalline…

Magnetic field dependent transient solar observations are suggestive for axion-photon oscillations with light axion(-like) particle involvement. Novel dark-moon measurements with the SMART X-ray detectors can be conclusive for radiatively…

Light new particles with masses below 10 keV, often considered as a plausible extension of the Standard Model, will be emitted from the solar interior, and can be detected on the Earth with a variety of experimental tools. Here we analyze…

High Energy Physics - Phenomenology · Physics 2013-08-21 Haipeng An , Maxim Pospelov , Josef Pradler

The axion, which has yet to be discovered, is a promising candidate for dark matter that emerges from Peccei-Quinn theory. This article presents the search for axion dark matter with the "Student Project for an Axion Cavity Experiment"…

High Energy Physics - Experiment · Physics 2025-10-29 M. A. Akgümüs , N. Salama , J. Egge , E. Garutti , M. Maroudas , L. H. Nguyen , D. Leppla-Weber

In this work, prospects to probe an overlooked facet of axion-like particles (ALPs) -- their potential couplings to sterile neutrinos -- are presented. We found that mono-photon searches have the potential to constrain ALP couplings to…

High Energy Physics - Phenomenology · Physics 2020-08-18 Alexandre Alves , Alex G. Dias , Diego D. Lopes

First experimental results from a room-temperature table-top phase-sensitive axion haloscope experiment are presented. The technique exploits the axion-photon coupling between two photonic resonator-oscillators excited in a single cavity,…

High Energy Physics - Experiment · Physics 2025-06-18 Catriona A. Thomson , Ben T. McAllister , Maxim Goryachev , Eugene N. Ivanov , Michael E. Tobar

An x-ray detector for a solar axion search was developed. The detector is operated at 60K in a cryostat of a superconducting magnet. Special care was paid to microphonic noise immunity and mechanical structure against thermal contraction.…

Astrophysics · Physics 2009-11-07 T. Namba , Y. Inoue , S. Moriyama , M. Minowa

We apply novel, recently developed plasma ray-tracing techniques to model the propagation of radio photons produced by axion dark matter in neutron star magnetospheres and combine this with both archival and new data for the galactic centre…

Cosmology and Nongalactic Astrophysics · Physics 2022-01-13 R. A. Battye , J. Darling , J. McDonald , S. Srinivasan

The latest result from the ORGAN experiment, an axion haloscope is presented. This iteration of the experiment operated at millikelvin temperatures using a flux-driven Josephson parametric amplifier for reduced noise, along with various…

Core-collapse supernovae provide a unique opportunity to probe axions because they can be a copious source of the particles. It has recently been proposed that axion helioscopes can be used for the direct search for supernova axions if a…

High Energy Astrophysical Phenomena · Physics 2025-11-19 Kanji Mori , Masamitsu Mori

We discuss the discovery potential of the Dark-photons & Axion-Like particles Interferometer (DALI) in this letter. The apparatus, currently in a design and prototyping phase, will probe axion dark matter from the Teide Observatory, an…

If dark matter is composed of axions, then axion stars form in the cores of dark matter halos. These stars are unstable above a critical mass, decaying to radio photons that heat the intergalactic medium, offering a new channel for axion…

High Energy Physics - Phenomenology · Physics 2024-02-09 Miguel Escudero , Charis Kaur Pooni , Malcolm Fairbairn , Diego Blas , Xiaolong Du , David J. E. Marsh

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

High Energy Physics - Phenomenology · Physics 2023-09-06 Adrian Thompson

The axion is a well-motivated cold dark matter (CDM) candidate first postulated to explain the absence of $CP$ violation in the strong interactions. CDM axions may be detected via their resonant conversion into photons in a "haloscope"…

Cosmology and Nongalactic Astrophysics · Physics 2018-01-04 Benjamin M. Brubaker

An axion dark matter search with the CAPP-8TB haloscope is reported. Our results are sensitive to axion-photon coupling $g_{a\gamma\gamma}$ down to the QCD axion band over the axion mass range between 6.62 and 6.82 $\mu$eV at a 90\%…

High Energy Physics - Experiment · Physics 2020-03-18 S. Lee , S. Ahn , J. Choi , B. R. Ko , Y. K. Semertzidis

Axions and other very light axion-like particles appear in many extensions of the Standard Model, and are leading candidates to compose part or all of the missing matter of the Universe. They also appear in models of inflation, dark…

High Energy Physics - Phenomenology · Physics 2018-08-01 Igor G. Irastorza , Javier Redondo

In the near future BabyIAXO will be the most powerful axion helioscope, relying on a custom-made magnet of two bores of 70 cm diameter and 10 m long, with a total available magnetic volume of more than 7 m$^3$. In this document, we propose…

This article describes BabyIAXO, an intermediate experimental stage of the International Axion Observatory (IAXO), proposed to be sited at DESY. IAXO is a large-scale axion helioscope that will look for axions and axion-like particles…

Instrumentation and Detectors · Physics 2021-03-05 A. Abeln , K. Altenmüller , S. Arguedas Cuendis , E. Armengaud , D. Attié , S. Aune , S. Basso , L. Bergé , B. Biasuzzi , P. T. C. Borges De Sousa , P. Brun , N. Bykovskiy , D. Calvet , J. M. Carmona , J. F. Castel , S. Cebrián , V. Chernov , F. E. Christensen , M. M. Civitani , C. Cogollos , T. Dafní , A. Derbin , K. Desch , D. Díez , M. Dinter , B. Döbrich , I. Drachnev , A. Dudarev , L. Dumoulin , D. D. M. Ferreira , E. Ferrer-Ribas , I. Fleck , J. Galán , D. Gascón , L. Gastaldo , M. Giannotti , Y. Giomataris , A. Giuliani , S. Gninenko , J. Golm , N. Golubev , L. Hagge , J. Hahn , C. J. Hailey , D. Hengstler , P. L. Henriksen , T. Houdy , R. Iglesias-Marzoa , F. J. Iguaz , I. G. Irastorza , C. Iñiguez , K. Jakovcic , J. Kaminski , B. Kanoute , S. Karstensen , L. Kravchuk , B. Lakic , T. Lasserre , P. Laurent , O. Limousin , A. Lindner , M. Loidl , I. Lomskaya , G. López-Alegre , B. Lubsandorzhiev , K. Ludwig , G. Luzón , C. Malbrunot , C. Margalejo , A. Marin-Franch , S. Marnieros , F. Marutzky , J. Mauricio , Y. Menesguen , M. Mentink , S. Mertens , F. Mescia , J. Miralda-Escudé , H. Mirallas , J. P. Mols , V. Muratova , X. F. Navick , C. Nones , A. Notari , A. Nozik , L. Obis , C. Oriol , F. Orsini , A. Ortiz de Solórzano , S. Oster , H. P. Pais Da Silva , V. Pantuev , T. Papaevangelou , G. Pareschi , K. Perez , O. Pérez , E. Picatoste , M. J. Pivovaroff , D. V. Poda , J. Redondo , A. Ringwald , M. Rodrigues , F. Rueda-Teruel , S. Rueda-Teruel , E. Ruiz-Choliz , J. Ruz , E. O. Saemann , J. Salvado , T. Schiffer , S. Schmidt , U. Schneekloth , M. Schott , L. Segui , F. Tavecchio , H. H. J. ten Kate , I. Tkachev , S. Troitsky , D. Unger , E. Unzhakov , N. Ushakov , J. K. Vogel , D. Voronin , A. Weltman , U. Werthenbach , W. Wuensch , A. Yanes-Díaz

The effects of absorption in the gas, and of density variations on the sensitivity of gas-filled solar-axion helioscopes are theoretically investigated. It is concluded that the 10-meter long CAST helioscope, the most sensitive experiment…

Astrophysics · Physics 2008-11-26 R. J. Creswick , S. Nussinov , F. T. Avignone