Search for Resonant Absorption of Solar Axions Emitted in M1 Transition in Fe Nuclei
arXiv:0906.0256 · doi:10.1140/epjc/s10052-009-1095-y
Abstract
A search for resonant absorbtion of 14.4 keV solar axions by Fe target was performed. The Si(Li) detector placed inside the low-background setup was used to detect the -quanta appearing in the deexcitation of 14.4 keV nuclear level: . The new upper limit for the hadronic axion mass have been obtained: eV (90% C.L.) (=0.5, =0.56).
arXiv comment5 pages, 3 figures
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- Search for solar axions in XMASS, a large liquid-xenon detector
- Search for 14.4 keV solar axions emitted in the M1-transition of 57Fe nuclei with CAST
- Constraints on short-range spin-dependent interactions from scalar spin-spin coupling in deuterated molecular hydrogen
- Searching for solar axions using data from the Sudbury Neutrino Observatory
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- Fabrication of a 64-Pixel TES Microcalorimeter Array with Iron Absorbers Uniquely Designed for 14.4-keV Solar Axion Search
- Heat flow of the Earth and resonant capture of solar 57-Fe axions
- Performance of TES X-Ray Microcalorimeters Designed for 14.4-keV Solar Axion Search
- Astrophysical and cosmological problems of invisible mass and dark energy in the Universe
- Axion mechanism of Sun luminosity, dark matter and extragalactic background light