Contribution to a conference proceedings/Contribution to a book PUBDB-2017-00165

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WISPDMX: A Haloscope for WISP Dark Matter between 0.8-2 $\mu$eV

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2015
Verlag Deutsches Elektronen-Synchrotron Hamburg

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 20152015-06-222015-06-26
Hamburg : Verlag Deutsches Elektronen-Synchrotron, DESY-PROC 219-223 () [10.3204/DESY-PROC-2015-02/nguyen_lehoang]  GO

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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.


Note: PIF-2013-08

Contributing Institute(s):
  1. Theorie-Gruppe (T)
  2. Any Light Particle Search (ALPS)
Research Program(s):
  1. 611 - Fundamental Particles and Forces (POF3-611) (POF3-611)
Experiment(s):
  1. No specific instrument

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Creative Commons Attribution CC BY 4.0 ; OpenAccess
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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 20152015-06-222015-06-26 Hamburg : Verlag Deutsches Elektronen-Synchrotron, DESY-PROC 1-251 () [10.3204/DESY-PROC-2015-02]  GO OpenAccess  Download fulltext Files BibTeX | EndNote: XML, Text | RIS


 Record created 2017-01-05, last modified 2023-09-18


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