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The International AXion Observatory (IAXO) will incorporate a new generation detector for axions, a hypothetical particle, which was postulated to solve one of the puzzles arising in the standard model of particle physics, namely the strong…

Instrumentation and Detectors · Physics 2016-11-17 I. Shilon , A. Dudarev , H. Silva , H. H. J. ten Kate

IAXO, the new International AXion Observatory, will feature the most ambitious detector for solar axions to date. Axions are hypothetical particles which were postulated to solve one of the puzzles arising in the standard model of particle…

Instrumentation and Detectors · Physics 2016-11-18 I. Shilon , A. Dudarev , H. Silva , U. Wagner , H. H. J. ten Kate

The International Axion Observatory (IAXO) will be a forth generation axion helioscope. As its primary physics goal, IAXO will look for axions or axion-like particles (ALPs) originating in the Sun via the Primakoff conversion of the solar…

The International Axion Observatory (IAXO) is a new generation axion helioscope aiming at a sensitivity to the axion-photon coupling of a few 10$^{12}$ GeV$^{-1}$, i.e. 1 - 1.5 orders of magnitude beyond the one currently achieved by CAST.…

Almost 35 years since their suggestion as a good solution to the strong CP-problem, axions remain one of the few viable candidates for the Dark Matter, although still eluding detection. Most of the methods for their detection are based on…

Instrumentation and Detectors · Physics 2019-08-14 T. Dafni , F. J. Iguaz

The International Axion Observatory (IAXO) is a next-generation axion helioscope designed to search for solar axions with unprecedented sensitivity. IAXO holds a unique position in the global landscape of axion searches, as it will probe a…

High Energy Physics - Phenomenology · Physics 2025-04-02 A. Arcusa , S. Ahyoune , K. Altenmuller , I. Antolin , S. Basso , P. Brun , V. Burwitz , F. R. Candon , J. F. Castel , S. Cebrian , D. Chouhan , R. Della Ceca , M. Cervera-Cortes , M. M. Civitani , C. Cogollos , E. Costa , V. Cotroneo , T. Dafni , K. Desch , M. C. Diaz-Martin , A. Diaz-Morcillo , D. Diez-Ibanez , C. Diez Pardos , M. Dinter , B. Dobrich , A. Dudarev , A. Ezquerro , S. Fabiani , E. Ferrer-Ribas , F. Finelli , I. Fleck , J. Galan , G. Galanti , M. Galaverni , J. Galindo Guarch , 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 , M. Iglesias , C. Iniguez , I. G. Irastorza , K. Jakovcic , D. Kafer , J. Kaminski , S. Karstensen , M. Law , A. Lindner , M. Loidl , C. Loiseau , G. Lopez-Alegre , A. Lozano-Guerrero , 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 , J. R. Navarro-Madrid , X. F. Navick , K. Nikolopoulos , A. Notari , 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. Schonfeld , M. Schott , L. Segui , U. R. Singh , P. Soffitta , D. Spiga , M. Stern , O. Straniero , F. Tavecchio , G. Vecchi , J. K. Vogel , R. Ward , A. Weltman , C. Wiesinger , R. Wolf , J. Woo , A. Yanes-Diaz , Y. Yu

Axion helioscopes search for solar axions and axion-like particles via inverse Primakoff conversion in strong laboratory magnets pointed at the Sun. Anticipating the detection of solar axions, we determine the potential for the planned…

Cosmology and Nongalactic Astrophysics · Physics 2020-08-28 Ciaran A. J. O'Hare , Andrea Caputo , Alexander J. Millar , Edoardo Vitagliano

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…

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

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

The International Axion Observatory (IAXO) is a forth generation axion helioscope designed to detect solar axions and axion-like particles (ALPs) with a coupling to the photon $g_{a\gamma}$ down to a few $10^{-12}$ GeV$^{-1}$, 1.5 orders of…

Instrumentation and Detectors · Physics 2016-11-16 Maurizio Giannotti , Jaime Ruz , Julia K. Vogel

Helioscopes, such as the proposed International Axion Observatory (IAXO), have significant discovery potential for axions and axion-like particles. In this note, we argue that beyond discovery they can resolve details of the model. In…

High Energy Physics - Phenomenology · Physics 2019-04-03 Joerg Jaeckel , Lennert J. Thormaehlen

The CERN Axion Solar Telescope (CAST) searches for solar axions employing a 9 Tesla superconducting dipole magnet equipped with 3 independent detection systems for X-rays from axion-photon conversions inside the 10 m long magnetic field.…

Astrophysics · Physics 2007-05-23 R. Kotthaus , H. Braeuninger , P. Friedrich , R. Hartmann , D. Kang , M. Kuster , G. Lutz , L. Strueder

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

We study the feasibility of a new generation axion helioscope, the most ambitious and promising detector of solar axions to date. We show that large improvements in magnetic field volume, x-ray focusing optics and detector backgrounds are…

Axions are well motivated particles proposed in an extension of the SM as a solution to the strong CP problem. Also, there is the category of Axion-Like Particles (ALPs) which appear in extensions of the SM and share the same phenomenology…

Solar and Stellar Astrophysics · Physics 2015-06-09 Juan Antonio García

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

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
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