Relic Neutrino Freeze-out: Dependence on Natural Constants

Abstract

Analysis of cosmic microwave background radiation fluctuations favors an effective number of neutrinos, $N_{\nu }>3$. This motivates a reinvestigation of the neutrino freeze-out process. Here we characterize the dependence of $N_{\nu }$ on the Standard Model (SM) parameters that govern neutrino freeze-out. We show that $N_{\nu }$ depends on a combination $\eta$ of several natural constants characterizing the relative strength of weak interaction processes in the early Universe and on the Weinberg angle ${\sin }^2{\theta }_W$. We determine numerically the dependence $N_{\nu }(\eta ,{\sin }^2{\theta }_W)$ 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 emerging chemical non-equilibrium, and a method to evaluate Boltzmann equation collision integrals that generates a smooth integrand.

38 pages, 14 figures

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Cited by in corpus (4)

• Relic neutrino decoupling with flavour oscillations revisited
• Insights into neutrino decoupling gleaned from considerations of the role of electron mass
• Big Bang Nucleosynthesis and Neutrino Cosmology
• Lepton Number and Expansion of the Universe