Axion Searches with Helioscopes and astrophysical signatures for axion(-like) particles

Details Axion Searches with Helioscopes and astrophysical signatures for axion(-like) particles Axion Searches with Helioscopes and astrophysical signatures for axion(-like) particles

2009-03-10

arxiv.org/abs/0903.1807v4

New J. Phys. 11 (2009) 105020

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

31 pages, 18 figures. Aded 1 author, updated references. Accepted for the special issue of NJP on dark matter (July 2009)

Scientific paper

10.1088/1367-2630/11/10/105020

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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