Wednesday, February 1, 2012

1201.5902 (Paola Arias et al.)

WISPy Cold Dark Matter    [PDF]

Paola Arias, Davide Cadamuro, Mark Goodsell, Joerg Jaeckel, Javier Redondo, Andreas Ringwald
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.
View original: http://arxiv.org/abs/1201.5902

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