Axion searches with helioscopes and astrophysical signatures for axion(-like) particles
New Journal of Physics2009Vol. 11(10), pp. 105020–105020
Citations Over TimeTop 10% of 2009 papers
Abstract
The first part reviews the working mechanisms, capabilities and performance of axion helioscopes, including the achieved results so far. The 2nd part is observationally driven. New simulation results obtained with the Geant4 code reconstruct spectral shape of solar X-ray spectra, and their isotropic emission and lateral size. The derived rst mass of the axion(-like) particles is ~10meV. The axion interaction with magnetic field gradient is a generic theoretical suggestion that could reconcile present limits with relevant solar X-ray activity. A short outlook of the experimentally expanding solar axion field is given.
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