Calculations for cosmic axion detection

Details Calculations for cosmic axion detection Calculations for cosmic axion detection

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985phrvl..55.1797k&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 55, Oct. 21, 1985, p. 1797-1800. NASA-supported research.

Physics

67

Cavity Resonators, Cosmic Gases, Elementary Particles, Magnetic Fields, Radiation Counters, Decay, Galactic Structure, Signal To Noise Ratios

Scientific paper

The authors present calculations, using properly normalized 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. The authors mention spin-coupled detection as an alternative to magnetic-field - coupled detection.

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