Dissociative recombination is the main destruction process for ground-state
H-3(+) in diffuse interstellar medium. Experiments agree on relatively lar
ge cross-sections for this reaction. Time-dependent two-dimensional calcula
tions confirm the experimental results at high energy as well as the observ
ed predissociation rates of Hg Rydberg states, due to non-adiabatic interac
tions. However, the value for low-energy cross-section, deduced from the pr
edissociation rates by an extrapolation procedure, is about four orders of
magnitude lower than the measured one. A calculation based on multichannel
quantum defect theory suggests that an indirect non-adiabatic process may p
revail in this case. The cross-section increases by orders of magnitude com
pared with the extrapolated value when indirect couplings via apparently in
effective channels are properly considered. We discuss ho iv this channel-m
ixing mechanism can be effective in the case of H-3(+), and show encouragin
g results stressing the role of Rydberg series or 'closed channels'. We als
o discuss possible three-dimensional effects that could enhance the process
at low energy.