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IAXO - The International Axion Observatory

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arxiv 1302.3273 v1 pith:GOSUT24N submitted 2013-02-13 physics.ins-det hep-ex

J. K. Vogel , F. T. Avignone , G. Cantatore , J. M. Carmona , S. Caspi , S. A. Cetin , F. E. Christensen , A. Dael
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T. Dafni M. Davenport A. V. Derbin K. Desch A. Diago A. Dudarev C. Eleftheriadis G. Fanourakis E. Ferrer-Ribas J. Galan J. A. Garcia J. G. Garza T. Geralis B. Gimeno I. Giomataris S. Gninenko H. Gomez C. J. Hailey T. Hiramatsu D. H. H. Hoffmann F. J. Iguaz I. G. Irastorza J. Isern J. Jaeckel K. Jakovcic J. Kaminski M. Kawasaki M. Krcmar C. Krieger B. Lakic A. Lindner A. Liolios G. Luzon I. Ortega T. Papaevangelou M. J. Pivovaroff G. Raffelt J. Redondo A. Ringwald S. Russenschuck J. Ruz K. Saikawa I. Savvidis T. Sekiguchi I. Shilon H. Silva H. H. J. ten Kate A. Tomas S. Troitsky K. van Bibber P. Vedrine J. A. Villar L. Walckiers W. Wester S. C. Yildiz K. Zioutas
This is my paper · ORCID
classification physics.ins-dethep-ex
keywords axioniaxoaxionscasthelioscopeinternationalobservatoryphysics
verification ladder T0 review T1 audit T2 compute T3 formal

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The International Axion Observatory (IAXO) is a next 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 sensitivities achieved by the currently most sensitive axion helioscope, the CERN Axion Solar Telescope (CAST). Crucial factors in improving the sensitivity for IAXO are the increase of the magnetic field volume together with the extensive use of x-ray focusing optics and low background detectors, innovations already successfully tested at CAST. Electron-coupled axions invoked to explain the white dwarf cooling, relic axions, and a large variety of more generic axion-like particles (ALPs) along with other novel excitations at the low-energy frontier of elementary particle physics could provide additional physics motivation for IAXO.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Search for solar axions produced through the axion-electron coupling $g_{ae}$ using a new GridPix detector at CAST

    hep-ex 2025-05 accept novelty 6.0 of 10

    A 160-hour solar tracking campaign with a 7-GridPix detector at CAST found no axion signal and set a new best helioscope limit g_ae*g_aγ < 7.35e-23 GeV^-1 at 95% confidence.

  2. Axion misalignment with memory-burdened PBH

    hep-ph 2025-01 conditional novelty 6.0 of 10

    Axion dark matter parameter space shifts dramatically when kinetic misalignment and memory-burdened primordial black hole evaporation are combined.

  3. Impact of First-order Electroweak Phase Transition on QCD Axion

    hep-ph 2025-07 conditional novelty 5.0 of 10

    A temporary axion mass spike during a first-order electroweak phase transition can make the QCD axion dark matter over a wide range of decay constants without a tuned initial angle.

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