Relic neutrino freeze-out: Dependence on natural constants
Jeremiah Birrell (Program in Applied Mathematics, The University of Arizona, Tucson, AZ, 85721, USA, Department of Physics, The University of Arizona, Tucson, AZ, 85721, USA); Cheng Tao Yang (Department of Physics, The University of Arizona, Tucson, AZ, 85721, USA, Department of Physics, Graduate Institute of Astrophysics, National Taiwan University, Taipei, 10617, Taiwan); Johann Rafelski (Department of Physics, The University of Arizona, Tucson, AZ, 85721, USA)
Analysis of cosmic microwave background radiation fluctuations favors an effective number of neutrinos, Nν>3 . This motivates a reinvestigation of the neutrino freeze-out process. Here we characterize the dependence of Nν on the Standard Model (SM) parameters that govern neutrino freeze-out. We show that Nν depends on a combination η of several natural constants characterizing the relative strength of weak interaction processes in the early Universe and on the Weinberg angle sin2θW . We determine numerically the dependence Nν(η,sin2θW) and discuss these results. The extensive numerical computations are made possible by two novel numerical procedures: a spectral method Boltzmann equation solver adapted to allow for strong reheating and emergent chemical non-equilibrium, and a method to evaluate Boltzmann equation collision integrals that generates a smooth integrand.
