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WISPy cold dark matter

Open access
Paola Arias, Davide Cadamuro, Mark Goodsell, Joerg Jaeckel, Javier Redondo, Andreas Ringwald·2012·Journal of Cosmology and Astroparticle Physics

Abstract

Very weakly interacting slim particles (WISPs), such as axion-like particles (ALPs) or hidden photons (HPs), may be non-thermally produced via the misalignment mechanism in the early universe and survive as a cold dark matter population until today. We find that, both for ALPs and HPs whose dominant interactions with the standard model arise from couplings to photons, a huge region in the parameter spaces spanned by photon coupling and ALP or HP mass can give rise to the observed cold dark matter. Remarkably, a large region of this parameter space coincides with that predicted in well motivated models of fundamental physics. A wide range of experimental searches — exploiting haloscopes (direct dark matter searches exploiting microwave cavities), helioscopes (searches for solar ALPs or HPs), or light-shining-through-a-wall techniques — can probe large parts of this parameter space in the foreseeable future.

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Metadata

Authors
Arias, P., Cadamuro, D., Goodsell, M., Jaeckel, J., Redondo, J., & Ringwald, A.
Venue
Journal of Cosmology and Astroparticle Physics
Published
2012-06-01
Volume
2012
Issue
06
Pages
013-013
ISSN
  • 1475-7508 (ISSN-L)
  • 1475-7516
OpenAlex
W2040460574
Cited by
879
References
1
FWCI
12.59
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: WISPy cold dark matter. https://app.cochat.ai/papers/10.1088/1475-7516/2012/06/013
The paper
Arias, P., Cadamuro, D., Goodsell, M., Jaeckel, J., Redondo, J., & Ringwald, A. (2012). WISPy cold dark matter. Journal of Cosmology and Astroparticle Physics. https://doi.org/10.1088/1475-7516/2012/06/013

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

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