Abstract
Cold dark matter in the Milky Way halo may have structure defined by flows with low velocity dispersion. The Axion Dark Matter eXperiment high resolution channel is especially sensitive to axions in such low velocity dispersion flows. Results from a combined power spectra analysis of the high resolution channel axion search are presented along with a discussion of the assumptions underlying such an analysis. We exclude Kim-Shifman-Vainshtein-Zakharov axion dark matter densities of and Dine-Fischler-Srednicki-Zhitnitskii densities of over a mass range of to for models having velocity dispersions of .
- Received 13 September 2011
DOI:https://doi.org/10.1103/PhysRevD.84.121302
© 2011 American Physical Society