• Rapid Communication

Search for nonvirialized axionic dark matter

J. Hoskins, J. Hwang, C. Martin, P. Sikivie, N. S. Sullivan, D. B. Tanner, M. Hotz, L. J Rosenberg, G. Rybka, A. Wagner, S. J. Asztalos, G. Carosi, C. Hagmann, D. Kinion, K. van Bibber, R. Bradley, and J. Clarke
Phys. Rev. D 84, 121302(R) – Published 28 December 2011

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 ρ0.2GeV/cm3 and Dine-Fischler-Srednicki-Zhitnitskii densities of ρ1.4GeV/cm3 over a mass range of ma=3.3μeV to 3.69μeV for models having velocity dispersions of Δβ3×106.

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  • Received 13 September 2011

DOI:https://doi.org/10.1103/PhysRevD.84.121302

© 2011 American Physical Society

Authors & Affiliations

J. Hoskins, J. Hwang*, C. Martin, P. Sikivie, N. S. Sullivan, and D. B. Tanner

  • University of Florida, Gainesville, Florida 32611

M. Hotz, L. J Rosenberg, G. Rybka, and A. Wagner

  • University of Washington, Seattle, Washington 98195

S. J. Asztalos, G. Carosi, C. Hagmann, D. Kinion, and K. van Bibber

  • Lawrence Livermore National Laboratory, Livermore, California, 94550

R. Bradley

  • National Radio Astronomy Observatory, Charlottesville, Virginia 22903

J. Clarke

  • University of California, and Lawrence Berkeley National Laboratory, Berkeley, California 94720

  • *Currently at Department of Physics, Sungkyunkwan University, Suwon, Gyeonggi-do 440-746, Republic of Korea.
  • Currently at XIA LLC, 31057 Genstar Road, Hayward CA, 94544
  • Currently at Naval Postgraduate School, Monterey CA, 93943

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Issue

Vol. 84, Iss. 12 — 15 December 2011

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