Relativistic mean field theory in finite nuclei

Bound state properties of Borromean halo nuclei: 6He and 11Li

Energy levels of light nuclei A=8,9,10

Empirical evidence suggests that neutron pairing plays an important role for the stability of nuclei near the neutron drip line. It is shown that the low binding of these nuclei will lead to a neutronization of the nuclear surface and possibly to large cross-sections for Coulomb dissociation, which then offers a new way to study clusters and their binding energies.

http://iopscience.iop.org/article/10.1209/0295-5075/4/4/005/pdf

The Neutron Halo of Extremely Neutron-Rich Nuclei

Energy levels of light nuclei A = 5–10

https://escholarship.org/content/qt40n8x7p3/qt40n8x7p3.pdf?t=p0lm6b

D.E. Greiner

Papers

Measurements of interaction cross sections and radii of He isotopes