Search for solar hadronic axions produced by a bremsstrahlung-like process

We have searched for hadronic axions which may be produced in the Sun by a bremsstrahlung-like process, and observed in the HPGe detector by an axioelectric effect. A conservative upper limit on the hadronic axion mass m_a < 334 eV at 95% C.L. is obtained. Our experimental approach is based on the axion-electron coupling and it does not include the axion-nucleon coupling, which suffers from the large uncertainties related to the estimation of the flavor-singlet axial-vector matrix element.Comment: 9 pages, 3 figures; version to appear in PL

The CERN Axion Solar Telescope (CAST)

A decommissioned LHC test magnets is being prepared as the CERN Axion Solar Telescope (CAST) experiment. The magnet has a field of 9.6 Tesla and length of 10 meters. It is being mounted on a platform to track the sun over +/-8(0) vertically and +/-45(0), horizontally. A sensitivity in axion-photon coupling g(agammagamma) < 5 x 10(-11)GeV(-1) can be reached for m(a) less than or equal to 10(-2) eV, and with a gas filled tube-can reach g(agammagamma) less than or equal to 10(-10)GeV(-1) for axion masses m(a) < 2eV

The CERN Axion Solar Telescope (CAST)

A decommissioned LHC test magnet is being prepared as the CERN Axion Solar Telescope (CAST) experiment. The magnet has a field of 9.6 Tesla and length of 10 meters. It is being mounted on a platform to track the sun over +/-8(0) vertically and +/-45(0), horizontally. A sensitivity in axion-photon coupling g(agammagamma) < 5 x 10(-11)GeV(-1) can be reached for m(a) less than or equal to 10(-2) eV, and with a gas filled tube-can reach g(agammagamma) less than or equal to 10(-10)GeV(-1) for axion masses m(a) < 2eV

The CERN axion solar telescope (CAST)

A decommissioned LHC test magnet is being prepared as the CERN Axion Solar Telescope (CAST) experiment. The magnet has a field of 9.6 Tesla and length of 10 meters. It is being mounted on a platform to track the sun over +-8 deg. vertically and +-45 deg. , horizontally. A sensitivity in axion-photon coupling g alpha gamma gamma < 5 x 10 sup - sup 1 sup 1 GeV sup - sup 1 can be reached for m subalpha <= 10 sup - sup 2 eV, and with a gas filled tube-can reach g alpha gamma gamma <= 10 sup - sup 1 sup 0 GeV sup - sup 1 for axion masses m subalpha < 2eV