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Related papers: The Tokyo Axion Helioscope Experiment

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Motivated by a possible $\sim$ eV-mass solar axion explanation to excess events recently detected by the XENON1T experiment, I revisit and update cosmological constraints on axions in this mass range. I find that of the allowed XENON1T mass…

Cosmology and Nongalactic Astrophysics · Physics 2020-07-16 Marius Millea

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

The axion is a hypothetical elementary particle and a cold dark matter candidate. It could dominate potential wells of most astrophysical objects. Axions spontaneously decay into nearly monochromatic microwave photons. We present results…

Astrophysics · Physics 2009-10-31 B. D. Blout , E. J. Daw , M. P. Decowski , Paul T. P. Ho , L. J Rosenberg , D. B. Yu

In non-hadronic axion models, which have a tree-level axion-electron interaction, the Sun produces a strong axion flux by bremsstrahlung, Compton scattering, and axio-recombination, the "BCA processes." Based on a new calculation of this…

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…

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…

High Energy Physics - Phenomenology · Physics 2021-11-08 Javier Galan

We review the physics potential of a next generation search for solar axions: the International Axion Observatory (IAXO). Endowed with a sensitivity to discover axion-like particles (ALPs) with a coupling to photons as small as…

A search for 5.5-MeV solar axions produced in the $p+d\rightarrow\rm{^3He}+A (5.5 \rm{MeV})$ reaction was performed using the Borexino detector. The Compton conversion of axions to photons, ${\rm A}+e\rightarrow e+\gamma$; the axio-electric…

High Energy Physics - Experiment · Physics 2012-08-27 The Borexino Collaboration

The CERN Axion Solar Telescope (CAST) searches for axions coming from photon to axion conversion in the sun's core, as stated by the Primakoff effect. Axions arise in particle physics as a consequence of the breaking of Peccei-Quinn…

Astrophysics · Physics 2017-08-23 C. Eleftheriadis et al

The search for solar axions produced by Compton ($\gamma+e^-\rightarrow e^-+A$) and bremsstrahlung-like ($e^-+Z \rightarrow Z+e^-+A$) processes has been performed. The axion flux in the both cases depends on the axion-electron coupling…

High Energy Physics - Experiment · Physics 2011-02-25 A. V. Derbin , A. S. Kayunov , V. N. Muratova , D. A. Semenov , E. V. Unzhakov

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 analyze the data from two recent experiments designed to search for solar axions within the context of multidimensional theories of the Kaluza-Klein type. In these experiments, axions were supposed to be emitted from the solar core, in…

High Energy Physics - Phenomenology · Physics 2009-11-07 R. Horvat , M. Krcmar , B. Lakic

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 present new results of a room temperature resonant AC haloscope, which searches for axions via photon upconversion. Traditional haloscopes require a strong applied DC magnetic background field surrounding the haloscope cavity resonator,…

High Energy Physics - Experiment · Physics 2023-06-08 Catriona A. Thomson , Maxim Goryachev , Ben T. McAllister , Eugene N. Ivanov , Paul Altin , Michael E. Tobar

We estimate the production rate of axion-type particles in the core of the Earth, at a temperature T~5000K. We constrain thermal geo-axion emission by demanding a core-cooling rate less than 100K/Gyr, as suggested by geophysics. This yields…

High Energy Physics - Phenomenology · Physics 2010-04-15 Hooman Davoudiasl , Patrick Huber

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

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…

A search for resonant absorption of solar axions by $^{169}$Tm nuclei was carried out. A newly developed approach involving low-background cryogenic bolometer based on Tm$_3$Al$_5$O$_{12}$ crystal was used that allowed for significant…

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

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