% 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{Pugnat:395493,
author = {Pugnat, P. and Ballou, R. and Camus, Ph. and Caspers, F.
and Ko, B. R. and Roch, N. and Semertzidis, Y. K.},
title = {{P}reliminary {S}tudy for a {N}ew {A}xion {D}ark-{M}atter
{H}aloscope},
address = {Hamburg},
publisher = {Verlag Deutsches Elektronen-Synchrotron},
reportid = {PUBDB-2017-12158, DESY-PROC-2016-03},
isbn = {978-3-945931-06-6},
series = {DESY-PROC},
pages = {129-132},
year = {2017},
comment = {Pugnat, P. "Preliminary Study for a New Axion Dark-Matter
Haloscope" in 12th "Patras" Workshop on Axions, WIMPs and
WISPs, PATRAS 2016 / Kim, Younglm, Lindner, Axel,
Semertzidis, Yannis K. (eds.), Verlag Deutsches
Elektronen-Synchrotron : 2017 ; PATRAS 2016 : 12th "Patras"
Workshop on Axions, WIMPs and WISPs, 2016-06-20 -
2016-06-24, Jeju Island},
booktitle = {Pugnat, P. "Preliminary Study for a
New Axion Dark-Matter Haloscope" in
12th "Patras" Workshop on Axions, WIMPs
and WISPs, PATRAS 2016 / Kim, Younglm,
Lindner, Axel, Semertzidis, Yannis K.
(eds.), Verlag Deutsches
Elektronen-Synchrotron : 2017 ; PATRAS
2016 : 12th "Patras" Workshop on
Axions, WIMPs and WISPs, 2016-06-20 -
2016-06-24, Jeju Island},
abstract = {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 $Q\sim10^5-10^6$ 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 $^3$He/$^4$He dilution refrigerator. This new haloscope
will be designed to probe QCD dark-matter Axions in the mass
range of 1-100~$\mu$eV with unprecedented sensitivity.},
month = {Jun},
date = {2016-06-20},
organization = {12th Patras Workshop on Axions, WIMPs
and WISPs, Jeju Island (South Korea),
20 Jun 2016 - 24 Jun 2016},
cin = {L},
cid = {I:(DE-H253)L-20120731},
pnm = {899 - ohne Topic (POF3-899)},
pid = {G:(DE-HGF)POF3-899},
experiment = {EXP:(DE-MLZ)NOSPEC-20140101},
typ = {PUB:(DE-HGF)29 / PUB:(DE-HGF)8 / PUB:(DE-HGF)7},
doi = {10.3204/DESY-PROC-2009-03/Pugnat_Pierre},
url = {https://bib-pubdb1.desy.de/record/395493},
}