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Axion Dark Matter eXperiment: Run 1B Analysis Details
ADMX Collaboration, C. Bartram, T. Braine +45
Searching for axion dark matter, the ADMX collaboration acquired data from January to October 2018, over the mass range 2.81--3.31 eV, corresponding to the frequency range 680--…
Modulation Sensitive Search for Non-Virialized Dark-Matter Axions
J. Hoskins, N. Crisosto, J. Gleason +23
Non-virialized dark-matter axions may be present in the Milky Way halo in the form of low-velocity-dispersion flows. The Axion Dark Matter eXperiment performed a search for the con…
A search for non-virialized axionic dark matter
J. Hoskins, J. Hwang, C. Martin +14
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 sens…
A Search for Scalar Chameleons with ADMX
G. Rybka, M. Hotz, L. J Rosenberg +11
Scalar fields with a "chameleon" property, in which the effective particle mass is a function of its local environment, are common to many theories beyond the standard model and co…
A SQUID-based microwave cavity search for dark-matter axions
The ADMX Collaboration, S. J. Asztalos, G. Carosi +12
Axions in the micro eV mass range are a plausible cold dark matter candidate and may be detected by their conversion into microwave photons in a resonant cavity immersed in a stati…