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| Preprint | PUBDB-2023-05534 |
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2014
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Please use a persistent id in citations: doi:10.3204/PUBDB-2023-05534
Report No.: DESY-14-191; arXiv:1410.6302
Abstract: Light cold dark matter consisting of weakly interacting slim (or sub-eV) particles (WISPs) has been in the focus of a large number of studies made over the past two decades. The QCD axion and axion-like particles with masses in the 0.1,$\mu$eV-100,meV are strong candidates for the dark matter particle, together with hidden photons with masses below $\lesssim 100$,meV. This motivates several new initiatives in the field, including the WISP Dark Matter eXperiment (WISPDMX) and novel conceptual approaches for broad-band WISP searches using radiometry measurements in large volume chambers. First results and future prospects for these experiments are discussed in this contribution.
Keyword(s): quantum chromodynamics: axion ; photon: hidden sector ; dark matter ; WISP ; axion-like particles
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Contribution to a conference proceedings/Contribution to a book
WISP Dark Matter eXperiment and Prospects for Broadband Dark Matter Searches in the 1 $\mu$eV-10 meV Mass Range
Proceedings, 10th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2014) 10th Patras Workshop on Axions, WIMPs and WISPs, AXION-WIMP 2014, Geneva, Switzerland, 29 Jun 2014 - 4 Jul 2014 ; DESY-PROC 94-101(2014). doi:10.3204/DESY-PROC-2014-03/lobanov_andrei
10th Patras Workshop on Axions, WIMPs and WISPs, AXION-WIMP 2014, GenevaGeneva, Switzerland, 29 Jun 2014 - 4 Jul 2014
Hamburg : Verlag Deutsches Elektronen-Synchrotron, DESY-PROC 94-101 (2014) [10.3204/DESY-PROC-2014-03/lobanov_andrei]
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