Abstract
We present calculations, using the 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. We mention spin-coupled detection as an alternative to magnetic-field coupled detection.
Original language | English (US) |
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Pages (from-to) | 1797-1800 |
Number of pages | 4 |
Journal | Physical Review Letters |
Volume | 55 |
Issue number | 17 |
DOIs | |
State | Published - 1985 |
Externally published | Yes |
ASJC Scopus subject areas
- Physics and Astronomy(all)