Large-scale microwave cavity search for dark-matter axions

By S. Asztalos, E. Daw, H. Peng, L. Rosenberg, C. Hagmann, D. Kinion, W. Stoeffl, K. Bibber, P. Sikivie, N. Sullivan and 9 more. 2001

191 citations recorded by the source corpus.

How researchers see this paper

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Microwave cavity searches for dark-matter axions (2003, methodology): “The medium-resolution data from this experiment were analyzed to search for dark-matter axions under two hypotheses (Asztalos et al., 2001).”
Search for New Physics with Atoms and Molecules (2017, methodology): “The first experiment to search for light DM composed of QCD axions was the Axion DM eXperiment (ADMX), which began its work in the 1990s (Asztalos et al., 2001, 2010).”
The type IIB string axiverse and its low-energy phenomenology (2012, background): “A number of experiments of this type have already been done [81–85] and further improvements are underway [86–88].”
Revealing the dark matter halo with axion direct detection (2017, methodology): “For example, ADMX implements exactly such a strategy, as described in [2].”
Towards a new generation axion helioscope (2011, methodology): “ADMX contemplates the exploration of the 1–10 µeV decade with sufficient sensitivity in gaγ to exclude or detect the QCD axion band, corresponding to gaγ in the approximate range 10 −17–10−14 GeV−1.”