TY  - CONF
AU  - Asztalos, S. J.
AU  - Bradley, R.
AU  - Carosi, G.
AU  - Clarke, John
AU  - Hagmann, C.
AU  - Hoskins, J.
AU  - Hotz, M.
AU  - Kinion, D.
AU  - Martin, C.
AU  - Rosenberg, L. J.
AU  - Rybka, G.
AU  - Sikivie, P.
AU  - Sullivan, N. S.
AU  - Tanner, D. B.
AU  - van Bibber, K.
AU  - Wagner, A.
TI  - The axion dark-matter eXperiment: Results and plans
IS  - DESY-PROC-2011-04
CY  - Hamburg
PB  - Deutsches Elektronen-Synchrotron, DESY
M1  - PUBDB-2016-01074
M1  - DESY-PROC-2011-04
SP  - 47-50
PY  - 2011
AB  - 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 μeV-10 meV, with the low end of this range (1-10 μeV) 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  ∼ 100 mK.
T2  - 7th Patras Workshop on Axions, WIMPs and WISPs
CY  - 27 Jun 2011 - 1 Jul 2011, Mykonos (Greece)
Y2  - 27 Jun 2011 - 1 Jul 2011
M2  - Mykonos, Greece
LB  - PUB:(DE-HGF)8 ; PUB:(DE-HGF)15
DO  - DOI:10.3204/DESY-PROC-2011-04/rybka_gray
UR  - https://bib-pubdb1.desy.de/record/295126
ER  -