I. J. Thompson
Published 1997-05-01Version 1
Our understanding of halo nuclei has so far relied on high-energy scattering and reactions, but a number of uncertainties remain. I discuss in general terms the new range of observables which will be measured by experiments around the Coulomb barrier, and how some details of the reaction mechanisms still need to be clarified.
Comments: Proceedings of FUSION97 conference (March 1997), South Durras, Australia. Submitted to J. Physics G: special issue `Heavy ion collisions at near barrier energies'. No figures; uses IOPConf.sty (included)
Journal: J.Phys.G23:1245-1250,1997
Near-Far Description of Elastic and Breakup Reactions of Halo Nuclei
Positron Tunnelling through the Coulomb Barrier of Superheavy Nuclei
Investigation of low-lying resonances in breakup of halo nuclei within the time-dependent approach
