  We review the relevance of neutrino-nucleus interactions at energy transfers
below 100 MeV for accelerator-based experiments, experiments at lower energies
and for astrophysical neutrinos. The impact of low-energy scattering processes
in the energy reconstruction analysis of oscillation experiments is
investigated. We discuss the modeling of coherent scattering processes and
compare its strength to that of inelastic interactions. The presented results
are obtained within a continuum random phase approximation approach.
