arXiv · 1305.6521
Self-interacting Dark Radiation
Abstract
We consider a simple class of models where dark radiation has self-interactions and therefore does not free stream. Such dark radiation has no anisotropic stress (or viscosity), leaving a distinct signature on the CMB angular power spectrum. Specifically we study a possibility that hidden gauge bosons and/or chiral fermions account for the excess of the effective number of neutrino species. They have gauge interactions and remain light due to the unbroken hidden gauge symmetry, leading to ΔN_{\rm eff} \simeq 0.29 in some case.
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Kwang Sik Jeong, Fuminobu Takahashi. 2013-08-13. Self-interacting Dark Radiation. https://doi.org/10.1016/j.physletb.2013.07.001
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