000395493 001__ 395493
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000395493 0247_ $$2datacite_doi$$a10.3204/DESY-PROC-2009-03/Pugnat_Pierre
000395493 0247_ $$2ISSN$$a1435-8077
000395493 037__ $$aPUBDB-2017-12158
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000395493 0881_ $$aDESY-PROC-2016-03
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000395493 1001_ $$0P:(DE-HGF)0$$aPugnat, P.$$b0
000395493 1112_ $$0C16-06-20.4$$2inspire$$a12th Patras Workshop on Axions, WIMPs and WISPs$$cJeju Island$$d2016-06-20 - 2016-06-24$$gAXION-WIMP 2016$$wSouth Korea
000395493 245__ $$aPreliminary Study for a New Axion Dark-Matter Haloscope
000395493 260__ $$aHamburg$$bVerlag Deutsches Elektronen-Synchrotron$$c2017
000395493 29510 $$aPugnat, P. "Preliminary Study for a New Axion Dark-Matter Haloscope" in 12th "Patras" Workshop on Axions, WIMPs and WISPs, PATRAS 2016 / Kim, Younglm, Lindner, Axel, Semertzidis, Yannis K. (eds.), Verlag Deutsches Elektronen-Synchrotron : 2017 ; PATRAS 2016 : 12th "Patras" Workshop on Axions, WIMPs and WISPs, 2016-06-20 - 2016-06-24, Jeju Island
000395493 300__ $$a129-132
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000395493 520__ $$aA new haloscope for Axion dark-matter search is under study using in a first step the large bore superconducting magnet in construction at the LNCMI in Grenoble, which will produce 9~T in 812~mm diameter and 1400~mm height. Microwave cavities of high quality factor $Q\sim10^5-10^6$ will be developed at CAPP/IBS in Daejeon. Low-noise microwave amplification of the signal will be ensured by DC superconducting quantum interference devices (SQUID) or/and Josephson parametric amplifiers (JPA) cooled-down to 20~mK by a $^3$He/$^4$He dilution refrigerator. This new haloscope will be designed to probe QCD dark-matter Axions in the mass range of 1-100~$\mu$eV with unprecedented sensitivity.
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000395493 7001_ $$0P:(DE-HGF)0$$aBallou, R.$$b1
000395493 7001_ $$0P:(DE-HGF)0$$aCamus, Ph.$$b2
000395493 7001_ $$0P:(DE-HGF)0$$aCaspers, F.$$b3
000395493 7001_ $$0P:(DE-HGF)0$$aKo, B. R.$$b4
000395493 7001_ $$0P:(DE-HGF)0$$aRoch, N.$$b5
000395493 7001_ $$0P:(DE-HGF)0$$aSemertzidis, Y. K.$$b6
000395493 7870_ $$0PUBDB-2017-11637$$aKim, Younglm et. al.$$dVerlag Deutsches Elektronen-Synchrotron$$iisPartOf$$rDESY-PROC-2016-03$$t12th "Patras" Workshop on Axions, WIMPs and WISPs, PATRAS 2016
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