  The Exact Parity Model (EPM) is, in part, a theory of neutrino mass and
mixing that can solve the atmospheric, solar and LSND anomalies. The central
feature of the neutrino sector is three pairs of maximally mixed ordinary and
mirror neutrinos. It has been shown that ordinary-mirror neutrino oscillations
can generate large neutrino asymmetries in the epoch of the early universe
immediately prior to Big Bang Nucleosynthesis (BBN). The large neutrino
asymmetries generically suppress the production of mirror neutrinos, and a
sufficiently large $\nu_e$ asymmetry can directly affect light element
synthesis through nuclear reaction rates. In this paper we present a detailed
calculation of neutrino asymmetry evolution driven by the six-flavour EPM
neutrino sector, focusing on implications for BBN.
