We assess the prospects for attaining steady nuclear-flow equilibrium
in expanding r-process environments where beta decay and/or neutrino c
apture determine the nuclear charge-changing rates. For very rapid exp
ansions, we find that weak steady flow equilibrium normally cannot be
attained. However, even when neutron-capture processes freeze out in s
uch nonequilibrium conditions, abundance ratios of nuclear species in
the r-process peaks might still mimic those attained in weak steady fl
ow. This result suggests that the r-process yield in a regime of rapid
expansion can be calculated reliably only when all neutron-capture, p
hotodisintegration, and weak interaction processes are fully coupled i
n a dynamical calculation. We discuss the implications of these result
s for models of the r-process sited in rapidly expanding neutrino-heat
ed ejecta.