Journal
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
Volume -, Issue 12, Pages -Publisher
IOP PUBLISHING LTD
DOI: 10.1088/1475-7516/2009/12/002
Keywords
axions; solar physics
Funding
- NSERC (Canada)
- MSES (Croatia) [098-0982887-2872]
- CEA (France)
- BMBF (Germany) [05 CC2EEA/9, 05 CC1RD1/0]
- Virtuelles Institut fur Dunkle Materie und Neutrinos -VIDMAN (Germany)
- GSRT (Greece)
- RFFR (Russia)
- Spanish Ministry of Science and Innovation (MICINN) [FPA2004-00973, FPA2007-62833]
- NSF (USA)
- US Department of Energy
- NASA [NAG5-10842]
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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 Fe-57, 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 g(a gamma)vertical bar-1.19 g(aN)(0) + g(aN)(3)vertical bar < 1.36 x 10(-16) GeV-1 for m(a) < 0.03 eV at the 95% confidence level.
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