Physics
Scientific paper
Mar 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983phrvl..50..925i&link_type=abstract
Physical Review Letters, vol. 50, Mar. 21, 1983, p. 925-927. Research supported by the U.S. Department of Energy and NSF.
Physics
84
Cosmology, Galactic Structure, Halos, Particle Theory, Spiral Galaxies, Weak Interactions (Field Theory), Neutrinos, Particle Flux Density
Scientific paper
If axions exist, they contribute significantly to the present energy density. These axions have been collisionless and nonrelativistic since their appearance at approximately 1 GeV. Hence axion density perturbations survive on essentially all scales, and once the axions are dominant, grow and in turn create and amplify baryon fluctuations. Axions can cluster into galactic halos even though the axion mass is not greater than approximately 0.01 eV. If galactic halo matter is mainly axions, the Peccei-Quinn order parameter not less than approximately 10 to the 10th GeV.
Ipser Jim
Sikivie Pierre
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