Viable twin cosmology from neutrino mixing

Twin Higgs models solve the little hierarchy problem without introducing new colored particles; however, they are often in tension with measurements of the radiation density at late times. Here we explore viable cosmological histories for twin Higgs models. In particular, we show that mixing between the Standard Model (SM) and twin neutrinos can thermalize the two sectors below the twin QCD phase transition, significantly reducing the twin sector's contribution to the radiation density. The requisite twin neutrino masses of O(1-20)GeV and mixing angle with SM neutrinos of 10(-3) - 10(-5) can be probed in a variety of current and planned experiments. We further find that these parameters can be naturally accessed in a warped UV completion, where the neutrino sector can also generate the Z(2)-breaking Higgs mass term needed to produce the hierarchy between the symmetry breaking scales f and v.