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Communication Dans Un Congrès Année : 2017

Preliminary Study for a New Axion Dark-Matter Haloscope

Rafik Ballou
Ph. Camus
  • Fonction : Auteur
F. Caspers
  • Fonction : Auteur
B.R. Ko
  • Fonction : Auteur
Nicolas Roch
Y.K. Semertzidis
  • Fonction : Auteur

Résumé

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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Dates et versions

hal-01703732 , version 1 (08-02-2018)

Identifiants

Citer

P. Pugnat, Rafik Ballou, Ph. Camus, F. Caspers, B.R. Ko, et al.. Preliminary Study for a New Axion Dark-Matter Haloscope. 12th Patras Workshop on Axions, WIMPs and WISPs, Jun 2016, Jeju Island, South Korea. pp.129-132, ⟨10.3204/DESY-PROC-2009-03/Pugnat_Pierre⟩. ⟨hal-01703732⟩
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