Key points are not available for this paper at this time.
We compute the dominant QED correction to the neutrino-electron interaction rate in the vicinity of neutrino decoupling in the early universe, and estimate its impact on the effective number of neutrino species N ₄₅₅ in cosmic microwave background anisotropy observations. We find that the correction to the interaction rate is at the sub-percent level, consistent with a recent estimate by Jackson and Laine. Relative to that work we include the electron mass in our computations, but restrict our analysis to the enhanced t-channel contributions. The fractional change in N ₄₅₅^ SM due to the rate correction is of order 10^-5 or below, i. e. , about a factor of 30 smaller than that recently claimed by Cielo et al. , and below the nominal computational uncertainties of the current benchmark value of N ₄₅₅^ SM = 3. 0440 0. 0002. We therefore conclude that aforementioned number remains to be the state-of-the-art benchmark for N ₄₅₅^ SM in the standard model of particle physics.
Drewes et al. (Wed,) studied this question.