We review and clarify the assumptions of our basic model for neutrino
production in the cores of quasars, as well as those modifications to
the model made subsequently by other workers. We also present a revise
d estimate of the neutrino background flux and spectrum obtained using
more recent empirical studies of quasars and their evolution. We comp
are our results with other theoretical calculations and experimental u
pper limits on the AGN neutrino background flux. We also estimate poss
ible neutrino fluxes from the jets of blazars detected recently by the
EGRET experiment on the Compton Gamma Ray Observatory. We discuss the
theoretical implications of these estimates.