Measurements of interaction cross sections for light neutron-rich nuclei at relativistic energies and determination of effective matter radii

By A. Ozawa, O. Bochkarev, L. Chulkov, D. Cortina, H. Geissel, M. Hellström, M. Ivanov, R. Janik, K. Kimura, Toshio Kobayashi and 15 more. 2001

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Postbounce Evolution of Core-Collapse Supernovae: Long-Term Effects of the Equation of State (2005, background): “One of stringent tests on the isovector interaction is passed in excellent agreement of the theoretical prediction with the experimental data on neutron and proton distributions in isotopes including neutron-rich ones with neutron-skins (Suzuki et al. 1995; Ozawa et al. 2001).”
Effective field theory description of halo nuclei (2017, methodology): “[77] using matter radii [85] determined from σI .”