Search for solar axions with mass around 1 eV using coherent conversion of axions into photons
Y. Inoue, Y. Akimoto, R. Ohta, T. Mizumoto, A. Yamamoto, M. Minowa

TL;DR
This paper reports a search for solar axions around 1 eV mass using a helioscope with a superconducting magnet, setting new limits on axion-photon coupling in a previously unexplored parameter region.
Contribution
The study introduces a novel search for axions near 1 eV mass with a helioscope, providing the first constraints in the relevant parameter space for preferred axion models.
Findings
No evidence of axions was found.
Set upper limits on axion-photon coupling constant g < 5.6-13.4×10^{-10} GeV^{-1}.
Explored the axion mass region around 1 eV for the first time.
Abstract
A search for solar axions has been performed using an axion helioscope which is equipped with a 2.3m-long 4T superconducting magnet, a gas container to hold dispersion-matching gas, PIN-photodiode X-ray detectors, and a telescope mount mechanism to track the sun. A mass region around m_a = 1eV was newly explored. From the absence of any evidence, analysis sets a limit on axion-photon coupling constant to be g < 5.6-13.4x10^{-10} GeV^{-1} for the axion mass of 0.84<m_a<1.00eV at 95% confidence level. It is the first result to search for the axion in the g-m_a parameter region of the preferred axion models with a magnetic helioscope.
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