A precision calculation of relic neutrino decoupling

By K. Akita, Masahide Yamaguchi. Journal of Cosmology and Astroparticle Physics, 2020

294 citations recorded by the source corpus.

We study the distortions of equilibrium spectra of relic neutrinos due to the interactions with electrons, positrons, and neutrinos in the early Universe. We solve the integro-differential kinetic equations for the neutrino density matrix, including three-flavor oscillations and finite temperature corrections from QED up to the next-to-leading order O(e3) for the first time. In addition, the equivalent kinetic equations in the mass basis of neutrinos are directly solved, and we numerically evaluate the distortions of the neutrino spectra in the mass basis as well, which can be easily extrapolated into those for non-relativistic neutrinos in the current Universe. In both bases, we find the same value of the effective number of neutrinos, Neff=3.044, which parameterizes the total neutrino energy density. The estimated error for the value of Neff due to the numerical calculations and the choice of neutrino mixing parameters would be at most 0.0005.

Subfields: Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/32fd8c74493c08785e9385e82f48ae965f8e9e44

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Nuclear and High Energy Physics

  1. M. Drewes
  2. S. Pastor
  3. Y. Wong
  4. Stefano Gariazzo
  5. P. F. de Salas
  6. K. G'orski
  7. A. Banday
  8. Gilles Buldgen

Citations in the corpus