2007/02/28 by S. Andriamonje, CAST Collaboration, S. Aune +59 · 5 citations
Physics and Astronomy · #Axion #Cosmology and Gravitation Theories #Coupling (piping) #Dark Matter and Cosmic Phenomena #Dark matter #Limit (mathematics) #Nuclear physics #Particle physics #Particle physics theoretical and experimental studies #Photon #Physics #Quantum electrodynamics #Quantum mechanics #Theoretical physics #astro-ph #hep-ex
paper · pdf · doi:10.1088/1475-7516/2007/04/010
published as JCAP 0704:010,2007 · 24 pages, 8 figures, 1 table, to be submitted to JCAP; v2: minor changes in the exclusion plot; v3: minor changes to match accepted version
arxiv created 2007/03/23 · openalex publication_date 2007/04/17 · arxiv updated 2012/08/27 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/06
We have searched for solar axions or similar particles that couple to two photons by using the CERN Axion Solar Telescope (CAST) set-up with improved conditions in all detectors. From the absence of excess x-rays when the magnet was pointing to the Sun, we set an upper limit on the axion–photon coupling of g aγ <8.8 × 10 −11 GeV −1 at 95% CL for . This result is the best experimental limit over a broad range of axion masses and for also supersedes the previous limit derived from energy-loss arguments on globular cluster stars.