Home > Publications database > WISPDMX: A Haloscope for WISP Dark Matter between 0.8-2 $\mu$eV |
Contribution to a conference proceedings/Contribution to a book | PUBDB-2017-00165 |
; ; ;
2015
Verlag Deutsches Elektronen-Synchrotron
Hamburg
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Please use a persistent id in citations: doi:10.3204/DESY-PROC-2015-02/nguyen_lehoang
Abstract: Weakly Interactive Slim Particles (WISPs), including the QCD axion, axion-like particles (ALPs), and hidden photons, are considered to be strong candidates for the dark matter carrier particle. The microwave cavity experiment WISPDMX is the first direct WISP dark matter search experiment probing particle masses in the 0.8-2.0~$\mu$eV range. The first stage of WISPDMX measurements has been completed at nominal resonant frequencies of the cavity. The second stage of WISPDMX is presently being prepared, targeting hidden photons and axions within 60\% of the entire 0.8-2.0~$\mu$eV mass range.
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Book/Proceedings/Report
Proceedings, 11th Patras Workshop on Axions, WIMPs and WISPs (Axion-WIMP 2015)
11th Patras Workshop on Axions, WIMPs and WISPs, AXION-WIMP 2015, ZaragozaZaragoza, Spain, 22 Jun 2015 - 26 Jun 2015
Hamburg : Verlag Deutsches Elektronen-Synchrotron, DESY-PROC 1-251 (2015) [10.3204/DESY-PROC-2015-02]
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