2025/06/09 by Jun-Chen Wang, Shunshun Cao, Wang, Jun-Chen +9
Physics and Astronomy · #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #FOS: Physical sciences #High Energy Astrophysical Phenomena (astro-ph.HE) #High Energy Physics - Phenomenology (hep-ph) #Pulsars and Gravitational Waves Research
paper · pdf · doi:10.48550/arxiv.2506.07546
openalex publication_date 2025/06/09 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/31
We propose a novel method to detect axions which uniquely depends on the dimensionless axion-photon coupling gγ, independent of the suppressive axion decay constant fa. Using neutron star PSR B1919+21 data from the Five-hundred-meter Aperture Spherical Telescope, we derive the first constraint |gγ|<0.93 at 1σ confidence level for ultra-light axions (ma < 10-11 eV).