Calculations for cosmic axion detection
- 21 October 1985
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review Letters
- Vol. 55 (17), 1797-1800
- https://doi.org/10.1103/physrevlett.55.1797
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.Keywords
This publication has 9 references indexed in Scilit:
- Axion Emission From Neutron StarsPhysical Review Letters, 1984
- A stellar energy loss mechanism involving axionsPhysics Letters B, 1984
- Comparisons of a standard galaxy model with stellar observations in five fieldsThe Astrophysical Journal Supplement Series, 1984
- Experimental Tests of the "Invisible" AxionPhysical Review Letters, 1983
- Cosmology of the invisible axionPhysics Letters B, 1983
- Astrophysical constraints on a new light axion and other weakly interacting particlesPhysical Review D, 1982
- The mass distribution within our Galaxy - A three component modelThe Astrophysical Journal, 1981
- A simple solution to the strong CP problem with a harmless axionPhysics Letters B, 1981
- Statistical Mechanics of Violent Relaxation in Stellar SystemsMonthly Notices of the Royal Astronomical Society, 1967