Experimental investigation of the sub-barrier fusion of neutron-rich light nuclei is important
in understanding the crusts of neutron stars, the structure of neutron-rich nuclei, and fusion dynamics of
neutron-rich nuclei. Moreover, the proposed experimental procedure is unique in allowing efficient
measurement of the excitation function below the Coulomb barrier with exotic beams delivered by
cyclotrons such as CIME of the SPIRAL facility at GANIL.