TY  - CONF
AU  - Pugnat, P.
AU  - Ballou, R.
AU  - Camus, Ph.
AU  - Caspers, F.
AU  - Ko, B. R.
AU  - Roch, N.
AU  - Semertzidis, Y. K.
TI  - Preliminary Study for a New Axion Dark-Matter Haloscope
IS  - DESY-PROC-2016-03
CY  - Hamburg
PB  - Verlag Deutsches Elektronen-Synchrotron
M1  - PUBDB-2017-12158
M1  - DESY-PROC-2016-03
SN  - 978-3-945931-06-6
T2  - DESY-PROC
SP  - 129-132
PY  - 2017
AB  - A new haloscope for Axion dark-matter search is under study using in a first step the large bore superconducting magnet in construction at the LNCMI in Grenoble, which will produce 9 T in 812 mm diameter and 1400 mm height. Microwave cavities of high quality factor Q ∼ 10<sup>5</sup>−10<sup>6</sup> will be developed at CAPP/IBS in Daejeon. Low-noise microwave amplification of the signal will be ensured by DC superconducting quantum interference devices (SQUID) or/and Josephson parametric amplifiers (JPA) cooled-down to 20 mK by a <sup>3</sup>He/<sup>4</sup>He dilution refrigerator. This new haloscope will be designed to probe QCD dark-matter Axions in the mass range of 1-100 μeV with unprecedented sensitivity.
T2  - 12th Patras Workshop on Axions, WIMPs and WISPs
CY  - 20 Jun 2016 - 24 Jun 2016, Jeju Island (South Korea)
Y2  - 20 Jun 2016 - 24 Jun 2016
M2  - Jeju Island, South Korea
LB  - PUB:(DE-HGF)29 ; PUB:(DE-HGF)8 ; PUB:(DE-HGF)7
DO  - DOI:10.3204/DESY-PROC-2009-03/Pugnat_Pierre
UR  - https://bib-pubdb1.desy.de/record/395493
ER  -