Standard and non-standard primordial neutrinos

The standard cosmological model predicts the existence of a cosmic neutrino background (CνB) with a present density of about n_{\nu}+n_{\vec{\nu}}\simeq 110\;cm^{- 3} per flavour, which affects big-bang nucleosynthesis (BBN), cosmic microwave background (CMB) anisotropies, and the evolution of large scale structures (LSS). We report on a precision calculation of the CνB properties including the modification introduced by neutrino oscillations. The role of a possible neutrino antineutrino asymmetry and the impact of non-standard neutrino electron interactions on the CνB are also briefly discussed.