  In the early universe, neutrinos decouple from equilibrium with the
electromagnetic plasma at a temperature which is only slightly higher than the
temperature where electrons and positrons annihilate. Therefore neutrinos to
some extent share in the entropy transfer from e^+e^- to other species, and
their final temperature is slightly higher than the canonical value T_nu =
(4/11)^{1/3} T_gamma. We study neutrino decoupling in the early universe with
effects of neutrino oscillations included, and find that the change in neutrino
energy density from e^+ e^- annihilations can be about 2-3% higher if
oscillation are included. The primordial helium abundance can be changed by as
much as 1.5 x 10^-4 by neutrino oscillations.
