% IMPORTANT: The following is UTF-8 encoded. This means that in the presence % of non-ASCII characters, it will not work with BibTeX 0.99 or older. % Instead, you should use an up-to-date BibTeX implementation like “bibtex8” or % “biber”. @INPROCEEDINGS{Asztalos:295126, author = {Asztalos, S. J. and Bradley, R. and Carosi, G. and Clarke, John and Hagmann, C. and Hoskins, J. and Hotz, M. and Kinion, D. and Martin, C. and Rosenberg, L. J. and Rybka, G. and Sikivie, P. and Sullivan, N. S. and Tanner, D. B. and van Bibber, K. and Wagner, A.}, title = {{T}he axion dark-matter e{X}periment: {R}esults and plans}, address = {Hamburg}, publisher = {Deutsches Elektronen-Synchrotron, DESY}, reportid = {PUBDB-2016-01074, DESY-PROC-2011-04}, pages = {47-50}, year = {2011}, abstract = {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.}, month = {Jun}, date = {2011-06-27}, organization = {7th Patras Workshop on Axions, WIMPs and WISPs, Mykonos (Greece), 27 Jun 2011 - 1 Jul 2011}, cin = {L}, cid = {I:(DE-H253)L-20120731}, pnm = {899 - ohne Topic (POF3-899)}, pid = {G:(DE-HGF)POF3-899}, experiment = {EXP:(DE-H253)HERA(machine)-20150101}, typ = {PUB:(DE-HGF)8 / PUB:(DE-HGF)15}, doi = {10.3204/DESY-PROC-2011-04/rybka_gray}, url = {https://bib-pubdb1.desy.de/record/295126}, }