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Dark matter annihilation or decay may produce striking signatures in millimeter, sub-millimeter and radio frequencies — for example, via electrons that produce synchrotron radiation in galactic/cluster magnetic fields, heating of the intergalactic medium during the epoch of reionization, or distortions to the spectrum of the cosmic microwave background. The small-scale structure of dark matter may be probed by improved lensing observations, in turn constraining new physics in the dark matter sector. Finally, searches for dark matter signatures at all wavelengths are complicated by astrophysical backgrounds that radio/mm/sub-mm searches could help address. I will discuss the current status and future prospects of these various directions.
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