001     395493
005     20211110145214.0
020 _ _ |a 978-3-945931-06-6
020 _ _ |a 978-3-945931-06-6
024 7 _ |a 10.3204/DESY-PROC-2009-03/Pugnat_Pierre
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024 7 _ |a 1435-8077
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037 _ _ |a PUBDB-2017-12158
041 _ _ |a English
088 1 _ |a DESY-PROC-2016-03
088 _ _ |a DESY-PROC-2016-03
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100 1 _ |a Pugnat, P.
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111 2 _ |a 12th Patras Workshop on Axions, WIMPs and WISPs
|c Jeju Island
|d 2016-06-20 - 2016-06-24
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245 _ _ |a Preliminary Study for a New Axion Dark-Matter Haloscope
260 _ _ |a Hamburg
|c 2017
|b Verlag Deutsches Elektronen-Synchrotron
295 1 0 |a 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
300 _ _ |a 129-132
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520 _ _ |a 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.
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700 1 _ |a Ballou, R.
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700 1 _ |a Camus, Ph.
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700 1 _ |a Caspers, F.
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700 1 _ |a Ko, B. R.
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700 1 _ |a Roch, N.
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700 1 _ |a Semertzidis, Y. K.
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787 0 _ |a Kim, Younglm et. al.
|d Verlag Deutsches Elektronen-Synchrotron
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|t 12th "Patras" Workshop on Axions, WIMPs and WISPs, PATRAS 2016
856 4 _ |u https://bib-pubdb1.desy.de/record/395493/files/fulltext.pdf
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