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100 1 _ |a Asztalos, S. J.
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111 2 _ |a 7th Patras Workshop on Axions, WIMPs and WISPs
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|d 2011-06-27 - 2011-07-01
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245 _ _ |a The axion dark-matter eXperiment: Results and plans
260 _ _ |c 2011
|b Deutsches Elektronen-Synchrotron, DESY
|a Hamburg
300 _ _ |a 47-50
336 7 _ |a Conference Paper
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336 7 _ |a INPROCEEDINGS
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520 _ _ |a The axion affects issues of the origin of CP symmetry in the strong interactions and the composition of the dark matter of the universe. Current constraints limit its mass to 1 $\mu$eV-10 meV, with the low end of this range (1-10 $\mu$eV) especially significant for dark-matter axions. Axions may be detected by their coupling to photons in a resonant cavity in a strong magnetic field. The Axion Dark-Matter eXperiment (ADMX) recently completed Phase I of an upgrade to its detector, incorporating SQUID electronics in the receiver front end and conducting a year-long data run. Phase II of the upgrade will install a high-capacity dilution refrigerator to cool the SQUID and cavity to $\sim$100 mK.
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700 1 _ |a Bradley, R.
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700 1 _ |a Carosi, G.
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700 1 _ |a Clarke, John
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700 1 _ |a Hagmann, C.
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700 1 _ |a Hoskins, J.
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700 1 _ |a Hotz, M.
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700 1 _ |a Kinion, D.
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700 1 _ |a Martin, C.
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700 1 _ |a Rosenberg, L. J.
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700 1 _ |a Rybka, G.
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700 1 _ |a Sikivie, P.
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700 1 _ |a Sullivan, N. S.
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700 1 _ |a Tanner, D. B.
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700 1 _ |a van Bibber, K.
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700 1 _ |a Wagner, A.
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773 _ _ |a 10.3204/DESY-PROC-2011-04/rybka_gray
787 0 _ |a Schumann, Marc et.al.
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|t Proceedings, 7th Patras Workshop on Axions, WIMPs and WISPs
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