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 magnitude beyond the current best astrophysical and experimental upper bounds. This range includes parameter values invoked in the context of the observed anomalies in light propagation over astronomical distances and to explain the excessive cooling observed in a number of stellar objects.
Here we review the status of the IAXO project and of its potential to probe the most physically motivated regions of the axion/ALPs parameter space.
Volume 282 -
38th International Conference on High Energy Physics (ICHEP2016) -
Dark Matter Detection
IAXO, next-generation of helioscopes
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Pre-published on:
February 06, 2017
Published on:
April 19, 2017
Abstract
DOI: https://doi.org/10.22323/1.282.0195
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Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.