Contributions to from the dark photon of
arXiv:2002.01137 · doi:10.1103/PhysRevD.102.015013
Abstract
We consider the effect on early Universe cosmology of the dark photon associated with the gauging of , a symmetry group under which only right-handed Standard Model fermions transform non-trivially. We find that cosmological constraints on this scenario are qualitatively much more severe than on other well-studied cases of a new gauge group, because the dark photon couples to chiral fermions. In particular, the dark photon of is always produced and equilibrates in the early Universe, no matter how small the gauge coupling, unless the symmetry-breaking scale is extremely large. This occurs because, no matter how the weak the coupling, the Goldstone mode (equivalently, the longitudinal polarization) does not decouple. As a result, even the limit of an extremely light and weakly-coupled dark photon of is effectively ruled out by cosmological constraints, unless the symmetry-breaking scale is extremely large. We also discuss the possibility of ameliorating Hubble tension in this model.
Updated figure and discussions, matches the journal version
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