Results of a Search for Cold Flows of Dark Matter Axions

L. Duffy, P. Sikivie, D. B. Tanner, S. Asztalos, C. Hagmann, D. Kinion, L. J Rosenberg, K. van Bibber, D. Yu, and R. F. Bradley
Phys. Rev. Lett. 95, 091304 – Published 26 August 2005

Abstract

Theoretical arguments predict that the distribution of cold dark matter in spiral galaxies has peaks in velocity space associated with nonthermalized flows of dark matter particles. We searched for the corresponding peaks in the spectrum of microwave photons from axion to photon conversion in a cavity detector for dark matter axions. We found none and place limits on the density of any local flow of axions as a function of the flow velocity dispersion over the axion mass range 1.98 to 2.17μeV.

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  • Received 11 May 2005

DOI:https://doi.org/10.1103/PhysRevLett.95.091304

©2005 American Physical Society

Authors & Affiliations

L. Duffy1, P. Sikivie1, D. B. Tanner1, S. Asztalos2, C. Hagmann2, D. Kinion2, L. J Rosenberg2, K. van Bibber2, D. Yu2, and R. F. Bradley3

  • 1Physics Department, University of Florida, Gainesville, Florida 32611, USA
  • 2Lawrence Livermore National Laboratory, Livermore, California 94550, USA
  • 3National Radio Astronomy Observatory, Charlottesville, Virginia 22903, USA

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Issue

Vol. 95, Iss. 9 — 26 August 2005

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