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In this paper we calculate the potential sensitivity of the CUORE detector to axions produced in the Sun through the Primakoff process and detected by the inverse coherent Bragg-Primakoff process. The conversion rate is calculated using…

Cosmology and Nongalactic Astrophysics · Physics 2015-11-04 Dawei. Li , R. J. Creswick , F. T. Avignone , Yuanxu. Wang

Theoretical axion models state that axions are very weakly interacting particles. In order to experimentally detect them, the use of colorful and inspired techniques becomes mandatory. There is a wide variety of experimental approaches that…

High Energy Physics - Experiment · Physics 2011-04-11 R. Battesti , B. Beltran , H. Davoudiasl , M. Kuster , P. Pugnat , R. Rabadan , A. Ringwald , N. Spooner , K. Zioutas

The CDMS-II experiment operates 19 germanium detectors with a mass of 250g each in a very low background environment. Originally designed for the search for Dark Matter the experiment can also detect solar axions by Primakoff conversion to…

Astrophysics · Physics 2019-08-13 T. Bruch

In this manuscript we anticipate axion detection in order to theorize on a novel telecommunications system based on the coherent axion-two-photon vertex Primakoff effect conversion and reversion of microwave photons transmitting a modulated…

Instrumentation and Detectors · Physics 2025-12-12 Javier De Miguel-Hernández

Axions generated thermally in the solar core can convert nearly directly to X-rays as they pass through the solar atmosphere via interaction with the magnetic field. The result of this conversion process would be a diffuse…

Solar and Stellar Astrophysics · Physics 2012-01-24 Hugh S. Hudson , L. W. Acton , E. DeLuca , I. G. Hannah , K. Reardon , K. Van Bibber

The Cern Axion Solar Telescope (CAST) is in operation and taking data since 2003. The main objective of the CAST experiment is to search for a hypothetical pseudoscalar boson, the axion, which might be produced in the core of the sun. The…

The working principle of axion helioscopes can be behind unexpected solar X-ray emission, being associated with solar magnetic fields, which become the catalyst. Solar axion signals can be transient brightenings as well as continuous…

Astrophysics · Physics 2016-11-09 K. Zioutas , M. Tsagri , Y. Semertzidis , Th. Papaevangelou , A. Nordt , V. Anastassopoulos

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 advocate the idea that there is a fundamentally new mechanism for the axion production in the Sun, which has never been discussed previously in the literature. This novel mechanism of the axion production is based on the so-called Axion…

High Energy Physics - Phenomenology · Physics 2018-08-22 H. Fischer , X. Liang , Y. Semertzidis , A. Zhitnitsky , K. Zioutas

In this paper we present a calculation of the expected flux of the mono-energetic 14.4 keV solar axions emitted by the M1 type nuclear transition of $^{57}$Fe in the Sun. These axions can be detected, e.g., by inverse coherent…

High Energy Physics - Phenomenology · Physics 2018-01-31 F. T. Avignone , R. J. Creswick , J. D. Vergados , P. Pirinen , P. C. Srivastava , J. Suhonen

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 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

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…

We propose a laser-plasma wakefield interaction based scheme for in situ axion generation and detection through the Primakoff process. Strong electromagnetic fields ($\gtrsim 10^{11}$\,V/m) in the wakefield can enhance axion production…

Plasma Physics · Physics 2025-12-23 Xiangyan An , Min Chen , Jianglai Liu , Zhan Bai , Liangliang Ji , Zhengming Sheng , Jie Zhang

Axion-photon conversion at dielectric interfaces, immersed in a near-homogeneous magnetic field, is the basis for the dielectric haloscope method to search for axion dark matter. In analogy to transition radiation, this process is possible…

High Energy Physics - Phenomenology · Physics 2017-09-07 Ara N. Ioannisian , Narine Kazarian , Alexander J. Millar , Georg G. Raffelt

We present a new mechanism to produce the dark photon ($\gamma'$) in the early universe with a help of the axion ($a$) using a recently proposed dark axion portal. The dark photon, a light gauge boson in the dark sector, can be a relic dark…

High Energy Physics - Phenomenology · Physics 2017-07-05 Kunio Kaneta , Hye-Sung Lee , Seokhoon Yun

Hypothetical axion-like particles with a two-photon interaction would be produced in the sun by the Primakoff process. In a laboratory magnetic field they would be transformed into X-rays with energies of a few keV. The CAST experiment at…

High Energy Physics - Experiment · Physics 2019-08-14 Berta Beltran

We show that XENON1T and future liquid xenon (LXe) direct detection experiments are sensitive to axions through the standard $g_{a\gamma}aF\tilde{F}$ operators due to inverse-Primakoff scattering. This previously neglected channel…

High Energy Physics - Phenomenology · Physics 2021-03-02 James B. Dent , Bhaskar Dutta , Jayden L. Newstead , Adrian Thompson

In certain laboratory experiments the production and/or detection of axions is due to the photon-axion transformations in a strong magnetic field. This process is coherent, and the rate of the transformation is proportional to the length…

High Energy Physics - Phenomenology · Physics 2018-12-05 V. V. Flambaum , I. B. Samsonov , H. B. Tran Tan , D. Budker

The solar abundance controversy inspires renewed investigations of the basic physics used to develop solar models. Here we examine the correction to the proton-proton reaction rate due to dynamic screening effects. Starting with the dynamic…

Solar and Stellar Astrophysics · Physics 2011-02-25 Katie Mussack , Werner Dappen