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Preliminary Study for a New Axion Dark-Matter Haloscope
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...
| Autores principales: | , , , , , , |
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| Lenguaje: | eng |
| Publicado: |
2017
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| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.3204/DESY-PROC-2009-03/Pugnat_Pierre http://cds.cern.ch/record/2315130 |
| _version_ | 1780958189784662016 |
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| author | Pugnat, P Ballou, R Camus, Ph Caspers, F Ko, B R Roch, N Semertzidis, Y K |
| author_facet | Pugnat, P Ballou, R Camus, Ph Caspers, F Ko, B R Roch, N Semertzidis, Y K |
| author_sort | Pugnat, P |
| collection | CERN |
| description | 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. |
| id | oai-inspirehep.net-1645383 |
| institution | Organización Europea para la Investigación Nuclear |
| language | eng |
| publishDate | 2017 |
| record_format | invenio |
| spelling | oai-inspirehep.net-16453832019-09-30T06:29:59Zdoi:10.3204/DESY-PROC-2009-03/Pugnat_Pierrehttp://cds.cern.ch/record/2315130engPugnat, PBallou, RCamus, PhCaspers, FKo, B RRoch, NSemertzidis, Y KPreliminary Study for a New Axion Dark-Matter HaloscopeDetectors and Experimental TechniquesAstrophysics and AstronomyA 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.oai:inspirehep.net:16453832017 |
| spellingShingle | Detectors and Experimental Techniques Astrophysics and Astronomy Pugnat, P Ballou, R Camus, Ph Caspers, F Ko, B R Roch, N Semertzidis, Y K Preliminary Study for a New Axion Dark-Matter Haloscope |
| title | Preliminary Study for a New Axion Dark-Matter Haloscope |
| title_full | Preliminary Study for a New Axion Dark-Matter Haloscope |
| title_fullStr | Preliminary Study for a New Axion Dark-Matter Haloscope |
| title_full_unstemmed | Preliminary Study for a New Axion Dark-Matter Haloscope |
| title_short | Preliminary Study for a New Axion Dark-Matter Haloscope |
| title_sort | preliminary study for a new axion dark-matter haloscope |
| topic | Detectors and Experimental Techniques Astrophysics and Astronomy |
| url | https://dx.doi.org/10.3204/DESY-PROC-2009-03/Pugnat_Pierre http://cds.cern.ch/record/2315130 |
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