We present a novel approach to investigating axions and axionlike particles by studying their potential conversion into x-rays within the Sun’s atmospheric magnetic field. Utilizing high-sensitivity data from the nuclear spectroscopic telescope array (NuSTAR) collected during the 2020 solar minimum, along with advanced solar atmospheric magnetic field models, we establish a new limit on the axion-photon coupling strength gaγ≲7.3×10−12 GeV−1 at 95% CL for axion masses ma≲4×10−7 eV. This constraint surpasses current ground-based experimental limits, studying previously unexplored regions of the axion-photon coupling parameter space up to masses of ma≲3.4×10−4 eV. These findings mark a significant advancement in our ability to probe axion properties and strengthen indirect searches for dark matter candidates.
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J. Ruz
Lawrence Livermore National Laboratory
Elisa Todarello
University of Nottingham
Julia K. Vogel
TU Dortmund University
Physical Review Letters
California Institute of Technology
University of California, Santa Barbara
University of Glasgow
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Ruz et al. (Thu,) studied this question.
synapsesocial.com/papers/68e034fdf0e39f13e7fa3547 — DOI: https://doi.org/10.1103/18sn-hxtb