Calculations for cosmic axion detection

Lawrence Krauss, John Moody, Frank Wilczek, Donald E. Morris

Research output: Contribution to journalArticle

116 Citations (Scopus)

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 languageEnglish (US)
Pages (from-to)1797-1800
Number of pages4
JournalPhysical Review Letters
Volume55
Issue number17
DOIs
StatePublished - 1985
Externally publishedYes

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galactic halos
line shape
microwaves
cavities
photons
magnetic fields
temperature

ASJC Scopus subject areas

  • Physics and Astronomy(all)

Cite this

Krauss, L., Moody, J., Wilczek, F., & Morris, D. E. (1985). Calculations for cosmic axion detection. Physical Review Letters, 55(17), 1797-1800. https://doi.org/10.1103/PhysRevLett.55.1797

Calculations for cosmic axion detection. / Krauss, Lawrence; Moody, John; Wilczek, Frank; Morris, Donald E.

In: Physical Review Letters, Vol. 55, No. 17, 1985, p. 1797-1800.

Research output: Contribution to journalArticle

Krauss, L, Moody, J, Wilczek, F & Morris, DE 1985, 'Calculations for cosmic axion detection', Physical Review Letters, vol. 55, no. 17, pp. 1797-1800. https://doi.org/10.1103/PhysRevLett.55.1797
Krauss, Lawrence ; Moody, John ; Wilczek, Frank ; Morris, Donald E. / Calculations for cosmic axion detection. In: Physical Review Letters. 1985 ; Vol. 55, No. 17. pp. 1797-1800.
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