NASA NTRS · 19860028136
Calculations for cosmic axion detection
Abstract
Calculations are presented, using properly nomalized couplings and masses for Dine-Fischler-Srednicki axions, of power rates and signal temperatures for axion-photon conversion in microwave cavities. The importance of the galactic-halo axion line shape is emphasized. Spin-coupled detection as an alternative to magnetic-field-coupled detection is mentioned.
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Krauss, L., Moody, J., Wilczek, F., Morris, D. E.. 1985-10-21. Calculations for cosmic axion detection. https://ntrs.nasa.gov/citations/19860028136
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