Search for solar axions by the cern axion solar telescope with he-3 buffer gas: closing the hot dark matter gap
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CitationARIK, M., AUNE, S., BARTH, K., BELOV, A., BORGHI, S., BRAUNINGER, H., CAST Collaboration. (2014). Search for solar axions by the cern axion solar telescope with he-3 buffer gas: closing the hot dark matter gap. Physical Review Letters, 112 (9), 6p. http://dx.doi.org/10.1103/PhysRevLett.112.091302.
The CERN Axion Solar Telescope has finished its search for solar axions with He-3 buffer gas, covering the search range 0.64 eV less than or similar to ma less than or similar to 1.17 eV. This closes the gap to the cosmological hot dark matter limit and actually overlaps with it. From the absence of excess x rays when the magnet was pointing to the Sun we set a typical upper limit on the axion-photon coupling of g(a gamma) less than or similar to 3.3 x 10(-10) GeV-1 at 95% C.L., with the exact value depending on the pressure setting. Future direct solar axion searches will focus on increasing the sensitivity to smaller values of g(a gamma), for example by the currently discussed next generation helioscope International AXion Observatory.