Published December 1, 2009 | Version v1
Journal article

Search for 14.4 keV solar axions emitted in the M1-transition of 57Fe nuclei with CAST

  • 1. IRFU, Centre d'Études Nucléaires de Saclay, Gif-sur-Yvette (France)
  • 2. European Organization for Nuclear Research (CERN), CH-1211 Genève 23 (Switzerland)
  • 3. Institute for Nuclear Research, Russian Academy of Sciences, Moscow (Russian Federation)
  • 4. Instituto de Física Nuclear y Altas Energías, Universidad de Zaragoza, Zaragoza (Spain)
  • 5. Max-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse, 85748 Garching (Germany)
  • 6. Enrico Fermi Institute and KICP, University of Chicago, Chicago, IL (United States)
  • 7. Aristotle University of Thessaloniki, Thessaloniki (Greece)
  • 8. National Center for Scientific Research ''Demokritos'', Athens (Greece)
  • 9. Albert-Ludwigs-Universität Freiburg, Freiburg (Germany)

Description

We have searched for 14.4 keV solar axions or more general axion-like particles (ALPs), that may be emitted in the M1 nuclear transition of 57Fe, by using the axion-to-photon conversion in the CERN Axion Solar Telescope (CAST) with evacuated magnet bores (Phase I). From the absence of excess of the monoenergetic X-rays when the magnet was pointing to the Sun, we set model-independent constraints on the coupling constants of pseudoscalar particles that couple to two photons and to a nucleon gaγ|−1.19gaN0+gaN3| < 1.36 × 10−16 GeV−1 for ma < 0.03 eV at the 95% confidence level

Availability note (English)

Available from http://dx.doi.org/10.1088/1475-7516/2009/12/002

Additional details

Publishing Information

Journal Title
Journal of Cosmology and Astroparticle Physics
Journal Volume
2009
Journal Issue
12
Journal Page Range
p. 002
ISSN
1475-7516

Optional Information

Collaborations
CAST collaboration